FN Thomson Reuters Web of Science™ VR 1.0 PT B AU Milosch, J AF Milosch, Jane BE Murphy, BL TI ADVOCATING FOR INTERNATIONAL COLLABORATIONS World War II-era provenance research in museums SO Museums, Ethics and Cultural Heritage LA English DT Article; Book Chapter C1 [Milosch, Jane] Smithsonian Inst, Off Secretary Hist Art & Culture, Smithsonians Provenance Res Initiat, Washington, DC 20560 USA. [Milosch, Jane] Smithsonian, Art Directing Paninst Art Programmes New Interdis, Washington, DC USA. [Milosch, Jane] Smithsonian Amer Art Museum, Renwick Gallery, Washington, DC USA. [Milosch, Jane] Cedar Rapids Museum Art, Cedar Rapids, IA USA. [Milosch, Jane] Detroit Inst Arts, Detroit, MI USA. RP Milosch, J (reprint author), Smithsonian Inst, Off Secretary Hist Art & Culture, Smithsonians Provenance Res Initiat, Washington, DC 20560 USA. NR 31 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE PI ABINGDON PA 2 PARK SQ, MILTON PARK, ABINGDON OX14 4RN, OXFORD, ENGLAND BN 978-1-138-67632-9; 978-1-315-56015-1 PY 2016 BP 193 EP 209 PG 17 WC Archaeology; Cultural Studies; Ethics SC Archaeology; Cultural Studies; Social Sciences - Other Topics GA BG4MB UT WOS:000388987700019 ER PT B AU West, WR AF West, W. Richard, Jr. BE Murphy, BL TI NATIVE AMERICA IN THE TWENTY-FIRST CENTURY SO Museums, Ethics and Cultural Heritage LA English DT Article; Book Chapter C1 [West, W. Richard, Jr.] Autry Museum Amer West, Los Angeles, CA 90027 USA. [West, W. Richard, Jr.] Smithsonian Inst, Natl Museum Amer Indian, Washington, DC 20560 USA. [West, W. Richard, Jr.] Amer Alliance Museums, Washington, DC USA. [West, W. Richard, Jr.] ICOM US, Kirkland, WA 98034 USA. RP West, WR (reprint author), Autry Museum Amer West, Los Angeles, CA 90027 USA.; West, WR (reprint author), ICOM US, Kirkland, WA 98034 USA. NR 1 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE PI ABINGDON PA 2 PARK SQ, MILTON PARK, ABINGDON OX14 4RN, OXFORD, ENGLAND BN 978-1-138-67632-9; 978-1-315-56015-1 PY 2016 BP 278 EP 288 PG 11 WC Archaeology; Cultural Studies; Ethics SC Archaeology; Cultural Studies; Social Sciences - Other Topics GA BG4MB UT WOS:000388987700026 ER PT J AU Parr, CS Schulz, KS Hammock, J Wilson, N Leary, P Rice, J Corrigan, RJ AF Parr, Cynthia S. Schulz, Katja S. Hammock, Jennifer Wilson, Nathan Leary, Patrick Rice, Jeremy Corrigan, Robert J., Jr. TI TraitBank: Practical semantics for organism attribute data SO Semantic Web LA English DT Article DE Biodiversity; ontologies; Semantic Web; traits; ecology; evolution; taxonomy; data aggregation ID ONTOLOGY; ENCYCLOPEDIA; ANNOTATION; LIFE AB Encyclopedia of Life (EOL) has developed TraitBank (http://eol.org/traitbank), a new repository for organism attribute (trait) data. TraitBank aggregates, manages and serves attribute data for organisms across the tree of life, including life history characteristics, habitats, distributions, ecological relationships and other data types. We describe how TraitBank ingests and manages these data in a way that leverages EOL's existing infrastructure and semantic annotations to facilitate reasoning across the TraitBank corpus and interoperability with other resources. We also discuss TraitBank's impact on users and collaborators and the challenges and benefits of our lightweight, scalable approach to the integration of biodiversity data. C1 [Parr, Cynthia S.; Schulz, Katja S.; Hammock, Jennifer; Corrigan, Robert J., Jr.] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20560 USA. [Wilson, Nathan; Leary, Patrick; Rice, Jeremy] Marine Biol Lab, Woods Hole, MA 02543 USA. [Parr, Cynthia S.] ARS, USDA, Beltsville, MD USA. [Wilson, Nathan] MassChallenge, Boston, MA USA. [Leary, Patrick] Calif Acad Sci, San Francisco, CA 94118 USA. RP Schulz, KS (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20560 USA. EM csparr@gmail.com; schulzk@si.edu FU Alfred P. Sloan Foundation; Smithsonian Institution; Marine Biological Laboratory; John D. and Catherine T. MacArthur Foundation; Harvard Faculty of Arts and Sciences (FAS) Sciences Division Research Computing Group FX Support for TraitBank was provided by the Alfred P. Sloan Foundation, the Smithsonian Institution, the Marine Biological Laboratory, and the John D. and Catherine T. MacArthur Foundation. The production hardware infrastructure for the EOL website was supported by the Harvard Faculty of Arts and Sciences (FAS) Sciences Division Research Computing Group and the Smithsonian Institution. The TraitBank development team wishes to specifically thank Dr. Jesse Ausubel for his support and for his commitment to the entire Encyclopedia of Life initiative. NR 44 TC 1 Z9 1 U1 2 U2 2 PU IOS PRESS PI AMSTERDAM PA NIEUWE HEMWEG 6B, 1013 BG AMSTERDAM, NETHERLANDS SN 1570-0844 EI 2210-4968 J9 SEMANT WEB JI Semant. Web PY 2016 VL 7 IS 6 BP 577 EP 588 DI 10.3233/SW-150190 PG 12 WC Computer Science, Artificial Intelligence; Computer Science, Information Systems; Computer Science, Theory & Methods SC Computer Science GA EE0AR UT WOS:000389236100001 ER PT S AU Jones, PL Page, RA Ratcliffe, JM AF Jones, Patricia L. Page, Rachel A. Ratcliffe, John M. BE Fenton, MB Grinnell, AD Popper, AN Fay, RR TI To Scream or to Listen? Prey Detection and Discrimination in Animal-Eating Bats SO BAT BIOACOUSTICS: WITH 62 ILLUSTRATIONS SE Springer Handbook of Auditory Research LA English DT Article; Book Chapter DE Aerial hawking; Bat echolocation; Eavesdropping; Signal intensity; Substrate gleaning ID LONG-EARED BAT; DOGBANE TIGER MOTH; FEMALE MATE CHOICE; ECHOLOCATING BATS; AERIAL-HAWKING; FROG CALLS; TRACHOPS-CIRRHOSUS; ARCTIID MOTH; GLEANING BAT; BEHAVIORAL FLEXIBILITY C1 [Jones, Patricia L.] Cornell Univ, Dept Ecol & Evolutionary Biol, Corson Hall, Ithaca, NY 14853 USA. [Page, Rachel A.] Smithsonian Trop Res Inst, Balboa, Panama. [Ratcliffe, John M.] Univ Toronto, Dept Ecol & Evolutionary Biol, 25 Willcocks St, Toronto, ON M5S 3B2, Canada. RP Ratcliffe, JM (reprint author), Univ Toronto, Dept Ecol & Evolutionary Biol, 25 Willcocks St, Toronto, ON M5S 3B2, Canada. EM plj6@cornell.edu; pager@si.edu; j.ratcliffe@utoronto.ca NR 119 TC 0 Z9 0 U1 1 U2 1 PU SPRINGER PI NEW YORK PA 233 SPRING STREET, NEW YORK, NY 10013, UNITED STATES SN 0947-2657 BN 978-1-4939-3527-7; 978-1-4939-3525-3 J9 SPRINGER HANDB AUDIT JI Springer Handb. Audit. Res. PY 2016 VL 54 BP 93 EP 116 DI 10.1007/978-1-4939-3527-7_4 D2 10.1007/978-1-4939-3527-7 PG 24 WC Acoustics; Zoology SC Acoustics; Zoology GA BG4KZ UT WOS:000388941000007 ER PT S AU Denzinger, A Kalko, EKV Tschapka, M Grinnell, AD Schnitzler, HU AF Denzinger, Annette Kalko, Elisabeth K. V. Tschapka, Marco Grinnell, Alan D. Schnitzler, Hans-Ulrich BE Fenton, MB Grinnell, AD Popper, AN Fay, RR TI Guild Structure and Niche Differentiation in Echolocating Bats SO BAT BIOACOUSTICS: WITH 62 ILLUSTRATIONS SE Springer Handbook of Auditory Research LA English DT Article; Book Chapter DE Bat; Echolocation; Foraging; Guild; Habitat; Masking; Niche differentiation; Resource partitioning ID FRUIT-EATING BATS; CAROLLIA-PERSPICILLATA PHYLLOSTOMIDAE; FLOWER-VISITING BATS; NECTAR-FEEDING BATS; OLD-WORLD TROPICS; PREY DETECTION; FORAGING BEHAVIOR; INSECTIVOROUS BATS; HORSESHOE BATS; SEED PREDATION C1 [Denzinger, Annette; Schnitzler, Hans-Ulrich] Univ Tubingen, Inst Neurobiol, Anim Physiol, Morgenstelle 28, D-72076 Tubingen, Germany. [Kalko, Elisabeth K. V.] Univ Ulm, Inst Expt Ecol, Albert Einstein Allee 11, D-89069 Ulm, Germany. [Kalko, Elisabeth K. V.; Tschapka, Marco] Smithsonian Trop Res Inst, POB 0843-03092, Panama City, Panama. [Tschapka, Marco] Inst Evolutionary Ecol & Conservat Genom, Albert Einstein Allee 11, D-89069 Ulm, Germany. [Grinnell, Alan D.] Univ Calif Los Angeles, David Geffen Sch Med, Dept Physiol, Los Angeles, CA 90095 USA. RP Denzinger, A (reprint author), Univ Tubingen, Inst Neurobiol, Anim Physiol, Morgenstelle 28, D-72076 Tubingen, Germany. EM annette.denzinger@uni-tuebingen.de; marco.tschapka@uni-ulm.de; marco.tschapka@uni-ulm.de; adg@mednet.ucla.edu; hans-ulrich.schnitzler@uni-tuebingen.de NR 109 TC 0 Z9 0 U1 0 U2 0 PU SPRINGER PI NEW YORK PA 233 SPRING STREET, NEW YORK, NY 10013, UNITED STATES SN 0947-2657 BN 978-1-4939-3527-7; 978-1-4939-3525-3 J9 SPRINGER HANDB AUDIT JI Springer Handb. Audit. Res. PY 2016 VL 54 BP 141 EP 166 DI 10.1007/978-1-4939-3527-7_6 D2 10.1007/978-1-4939-3527-7 PG 26 WC Acoustics; Zoology SC Acoustics; Zoology GA BG4KZ UT WOS:000388941000009 ER PT S AU Carn, SA AF Carn, S. A. BE Harris, AJL DeGroeve, T Garel, F Carn, SA TI On the detection and monitoring of effusive eruptions using satellite SO2 measurements SO DETECTING, MODELLING AND RESPONDING TO EFFUSIVE ERUPTIONS SE Geological Society Special Publication LA English DT Article; Book Chapter ID SULFUR-DIOXIDE EMISSIONS; BASALTIC ERUPTIONS; VOLCANO; FLUX; RATES; NYAMURAGIRA; INSTRUMENT; MODIS; OMI AB Timely detection and quantification of lava effusion rates are crucial for volcanic hazard mitigation during effusive eruptions. Satellite-based detection methods typically exploit the exceptional radiant heat fluxes associated with lava effusion, but effusive eruptions can also emit prodigious amounts of sulphur dioxide (SO2). Measuring the magnitude and temporal evolution of SO2 emissions provides an additional means for monitoring effusive eruptions, complementing thermal monitoring. Examples of effusive eruptions detected since 1978 using ultraviolet (UV) satellite measurements of SO2 emissions by the Total Ozone Mapping Spectrometer (TOMS), Ozone Monitoring Instrument (OMI) and Ozone Mapping and Profiler Suite (OMPS) are reviewed. During many effusive eruptions, trends in SO2 production mimic the classic waxing-waning pattern characteristic of such events that is also seen in thermal infrared (TIR) hotspot data, suggesting a qualitative link between SO2 emissions and lava effusion rates. An example of lava effusion rate calculation based on TOMS SO2 measurements is presented for the 1998 eruption of Cerro Azul (Gala pagos Islands), for which detailed eruption observations and independent estimates of effusion rates are available. Combining TOMS-derived SO2 emission rates with estimates of sulphur content in Cerro Azul lavas yields lava effusion rates almost identical to independently derived values, demonstrating the utility of the technique. C1 [Carn, S. A.] Michigan Technol Univ, Dept Geol & Min Engn & Sci, Houghton, MI 49931 USA. [Carn, S. A.] Smithsonian Inst, Natl Museum Amer Hist, Dept Mineral Sci, Washington, DC 20560 USA. RP Carn, SA (reprint author), Michigan Technol Univ, Dept Geol & Min Engn & Sci, Houghton, MI 49931 USA.; Carn, SA (reprint author), Smithsonian Inst, Natl Museum Amer Hist, Dept Mineral Sci, Washington, DC 20560 USA. EM scarn@mtu.edu NR 73 TC 0 Z9 0 U1 0 U2 0 PU GEOLOGICAL SOC PUBLISHING HOUSE PI BATH PA UNIT 7, BRASSMILL ENTERPRISE CTR, BRASSMILL LANE, BATH BA1 3JN, AVON, ENGLAND SN 0305-8719 BN 978-1-86239-736-1 J9 GEOL SOC SPEC PUBL JI Geol. Soc. Spec. Publ. PY 2016 VL 426 BP 277 EP 292 PG 16 WC Geochemistry & Geophysics; Geology; Remote Sensing SC Geochemistry & Geophysics; Geology; Remote Sensing GA BG3YB UT WOS:000388378700014 ER PT S AU Myers, PC AF Myers, Philip C. BE Jablonka, P Andre, P VanDerTak, F TI Formation of star clusters: Models and simulations SO FROM INTERSTELLAR CLOUDS TO STAR-FORMING GALAXIES: UNIVERSAL PROCESSES? SE IAU Symposium Proceedings Series LA English DT Proceedings Paper CT 315th Symposium of the International-Astronomical-Union CY AUG 03-07, 2015 CL Honolulu, HI SP Int Astronom Union, Ecole Polythechnique Federale Lausanne, Netherlands Inst Space Res, Commissariat Lenergie Atomique & Aux Energies Alternat DE Molecular clouds; star formation; star clusters ID INITIAL MASS FUNCTION; MOLECULAR CLOUD; SUPERSONIC TURBULENCE; DARK CLOUDS; DENSE CORES; STELLAR; EVOLUTION; ACCRETION; RADIATION; DYNAMICS AB Recent progress is reviewed in describing the physical processes of star cluster formation, from the viewpoint of theoretical models and numerical simulations. In many studies, supersonic turbulent flows structure the gas into a network of clumps, filaments, and cores. Self-gravity drives star formation, moderated by turbulence, magnetic fields, and stellar feedback. Recent models and simulations describe the core mass function, the protostar mass function, and the star-formation rate. Several simulations indicate similar protostar birthrates, a mass advantage for firstborn protostars, and accretion rates that are superthermal and nearly constant. Recently observed core-filament systems with sonic line widths and parsec lengths present challenges for turbulent models. C1 [Myers, Philip C.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Myers, PC (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM pmyers@cfa.harvard.edu NR 52 TC 0 Z9 0 U1 0 U2 0 PU CAMBRIDGE UNIV PRESS PI CAMBRIDGE PA THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND SN 1743-9213 BN 978-1-107-13520-8 J9 IAU SYMP P SERIES JI IAU Symposium Proc. Series PY 2016 VL 315 BP 130 EP 137 DI 10.1017/S1743921316007390 PG 8 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BG2ZL UT WOS:000387795900108 ER PT S AU Saito, T Iono, D Ueda, J Yun, MS Nakanishi, K Sugai, H Imanishi, M Hagiwara, Y Kaneko, H Motohara, K Espada, D Yamashita, T Lee, M Michiyama, T Kawabe, R AF Saito, Toshiki Iono, Daisuke Ueda, Junko Yun, Min S. Nakanishi, Kouichiro Sugai, Hajime Imanishi, Masatoshi Hagiwara, Yoshiaki Kaneko, Hiroyuki Motohara, Kentaro Espada, Daniel Yamashita, Takuji Lee, Minju Michiyama, Tomonari Kawabe, Ryohei BE Jablonka, P Andre, P VanDerTak, F TI Molecular Gas Excitation and Chemistry in VV 114 and NGC 1614 with ALMA SO FROM INTERSTELLAR CLOUDS TO STAR-FORMING GALAXIES: UNIVERSAL PROCESSES? SE IAU Symposium Proceedings Series LA English DT Proceedings Paper CT 315th Symposium of the International-Astronomical-Union CY AUG 03-07, 2015 CL Honolulu, HI SP Int Astronom Union, Ecole Polythechnique Federale Lausanne, Netherlands Inst Space Res, Commissariat Lenergie Atomique & Aux Energies Alternat DE Galaxies: interaction; Galaxies: starburst; ISM: molecules ID CENTRAL KILOPARSEC; EMISSION; VV-114 AB We present high resolution molecular line observations of dusty AGN and star burst in nearby luminous infrared galaxies (LIRGs), VV 114 (band 3/4/7) and NGC 1614 (band 3/6/7/9), with ALMA. Multi-frequency imaging from 4.8 GHz to 691 GHz of NGC 1614 allows us to study spatial properties of the radio-to-FIR continuum and multiple CO transitions, and we find the CO excitation up to J(upp) = 6 can be explained by a single ISM model powered by nuclear starbursts. Our processing line imaging survey for VV 114 detected at least 30 molecular lines which show different chemical composition from region to region. Multi-molecule imaging helps us to diagnose the chemical differences of dusty ISM, while multi-transition imaging allows us to investigate gas physical conditions affected by nuclear activities directly. C1 [Saito, Toshiki; Lee, Minju; Kawabe, Ryohei] Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1330033, Japan. [Saito, Toshiki; Iono, Daisuke; Ueda, Junko; Nakanishi, Kouichiro; Imanishi, Masatoshi; Kaneko, Hiroyuki; Lee, Minju; Michiyama, Tomonari; Kawabe, Ryohei] Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan. [Iono, Daisuke; Nakanishi, Kouichiro; Imanishi, Masatoshi; Michiyama, Tomonari; Kawabe, Ryohei] SOKENDAI, Dept Astron Sci, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan. [Ueda, Junko] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Yun, Min S.] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA. [Sugai, Hajime] Univ Tokyo, Kavli Inst Phys & Math Universe WPI, 5-1-5 Kashiwanoha, Kashiwa, Chiba 2778583, Japan. [Imanishi, Masatoshi] Subaru Telescope, 650 North Aohoku Pl, Hilo, HI 96720 USA. [Hagiwara, Yoshiaki] Toyo Univ, Nat Sci Lab, Bunkyo Ku, 5-28-20 Hakusan, Tokyo 1128606, Japan. [Kaneko, Hiroyuki] NAOJ, Nobeyama Radio Observ, Minamisa Ku, 462-2 Minamimaki, Minamimaki, Nagano 3841305, Japan. [Motohara, Kentaro] Univ Tokyo, Inst Astron, 2-21-1 Osawa, Mitaka, Tokyo 1810015, Japan. [Espada, Daniel] Joint ALMA Observ, Alonso Cordova 3107,Casilla 19001, Santiago 19, Chile. [Yamashita, Takuji] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2298510, Japan. RP Saito, T (reprint author), Univ Tokyo, Grad Sch Sci, Dept Astron, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1330033, Japan.; Saito, T (reprint author), Natl Astron Observ Japan, 2-21-1 Osawa, Mitaka, Tokyo 1818588, Japan. EM toshiki.saito@nao.ac.jp NR 10 TC 0 Z9 0 U1 0 U2 0 PU CAMBRIDGE UNIV PRESS PI CAMBRIDGE PA THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND SN 1743-9213 BN 978-1-107-13520-8 J9 IAU SYMP P SERIES JI IAU Symposium Proc. Series PY 2016 VL 315 DI 10.1017/S1743921316008334 PG 2 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BG2ZL UT WOS:000387795900071 ER PT B AU Staaterman, E AF Staaterman, Erica BE Au, WWL Lammers, MO TI Passive Acoustic Monitoring in Benthic Marine Crustaceans: A New Research Frontier SO LISTENING IN THE OCEAN: NEW DISCOVERIES AND INSIGHTS ON MARINE LIFE FROM AUTONOMOUS PASSIVE ACOUSTIC RECORDERS SE Modern Acoustics and Signal Processing LA English DT Article; Book Chapter ID SOUND PRODUCTION; HEMISQUILLA-CALIFORNIENSIS; HABITATS; BEHAVIOR; LOBSTER; COMMUNITIES; DECAPODA; NOISE; REEF AB Passive acoustic monitoring has been used to study the soundscapes of some shallow-water coastal environments. These studies have revealed distinct patterns that depend upon the physical structure of the environment as well as the species living within it. One underrepresented group in marine bioacoustics is the benthic crustaceans, yet these animals are known to produce and detect sounds. Snapping shrimp are the most ubiquitous benthic crustacean, and their "snaps" can substantially elevate sound levels in the range of 2-15 kHz in a variety of habitats in the mid-latitudes. Clawed and spiny lobsters produce tonal vibrations and broadband "rasps," respectively, but these sounds occur more intermittently than the snapping shrimp choruses. Finally, burrow-dwelling mantis shrimp produce low-frequency rhythmic "rumbles" which tend to occur as dawn and dusk choruses. Passive acoustic monitoring of these taxa can be useful for revealing broad ecological patterns, by using some species (e. g., snapping shrimp) as ecological indicators. Acoustic measurements can reveal temporal patterns in crustacean sounds and detect species' occupancy of particular habitats. Finally, acoustic monitoring can demonstrate the temporal and frequency overlap between anthropogenic sounds and natural crustacean sounds, which can help refine research questions on potential impacts. C1 [Staaterman, Erica] Smithsonian Inst, Smithsonian Environm Res Ctr, 647 Contees Wharf Rd, Edgewater, MD 21037 USA. [Staaterman, Erica] Waves Inc, Syracuse, NY USA. RP Staaterman, E (reprint author), Smithsonian Inst, Smithsonian Environm Res Ctr, 647 Contees Wharf Rd, Edgewater, MD 21037 USA. EM e.staaterman@gmail.com NR 39 TC 0 Z9 0 U1 0 U2 0 PU SPRINGER-VERLAG BERLIN PI BERLIN PA HEIDELBERGER PLATZ 3, D-14197 BERLIN, GERMANY BN 978-1-4939-3176-7; 978-1-4939-3175-0 J9 MOD ACOUST SIGN PROC PY 2016 BP 325 EP 333 DI 10.1007/978-1-4939-3176-7_13 D2 10.1007/978-1-4939-3176-7 PG 9 WC Acoustics; Engineering, Electrical & Electronic; Marine & Freshwater Biology SC Acoustics; Engineering; Marine & Freshwater Biology GA BG4HX UT WOS:000388838600015 ER PT J AU Pellegrini, MOD Faden, RB de Almeida, RF AF de Oliveira Pellegrini, Marco Octavio Faden, Robert B. de Almeida, Rafael Felipe TI Taxonomic revision of Neotropical Murdannia Royle (Commelinaceae) SO PHYTOKEYS LA English DT Article DE Aquatic plants; Brazil; Commelinales; Commelineae; dewflower; Neotropical flora; spiderwort ID SEQUENCES AB This study provides a taxonomic revision for the Neotropical species of the genus Murdannia. Six species are recognized as native, including a new species and a new combination, while two Asian species are recognized as invasive. We present an identification key, a table summarizing the morphologic differences among the species, a new synonym, six lectotypifications, a distribution map, and descriptions, comments and photographic plates for each species. We also provide comments on the morphology of the Neotropical species of Murdannia, comparing them with the Paleotropical species, and a discussion of inflorescence architecture in the genus as a whole. C1 [de Oliveira Pellegrini, Marco Octavio] Univ Sao Paulo, Dept Bot, Rua Matao 277, BR-05508900 Sao Paulo, SP, Brazil. [de Oliveira Pellegrini, Marco Octavio] Inst Pesquisas Jardim Bot Rio de Janeiro, Rua Pacheco Leao 915, BR-22460030 Rio De Janeiro, RJ, Brazil. [de Oliveira Pellegrini, Marco Octavio; Faden, Robert B.] NMNH, Smithsonian Inst, Dept Bot, MRC 166,POB 37012, Washington, DC 20013 USA. [de Almeida, Rafael Felipe] Univ Estadual Feira de Santana, Programa Posgrad Bot, Ave Transnordestina S-N, BR-44036900 Feira De Santana, BA, Brazil. RP Pellegrini, MOD (reprint author), Univ Sao Paulo, Dept Bot, Rua Matao 277, BR-05508900 Sao Paulo, SP, Brazil.; Pellegrini, MOD (reprint author), Inst Pesquisas Jardim Bot Rio de Janeiro, Rua Pacheco Leao 915, BR-22460030 Rio De Janeiro, RJ, Brazil.; Pellegrini, MOD (reprint author), NMNH, Smithsonian Inst, Dept Bot, MRC 166,POB 37012, Washington, DC 20013 USA. EM marcooctavio.pellegrini@gmail.com OI de Almeida, Rafael Felipe/0000-0002-9562-9287 FU FAPESB [DEB BOL0584/2013]; CAPES; Fundacao Flora de Apoio a Botanica and Smithsonian Institution FX We would like to thank Mathias Erich Engels for all his support on field collections, spirits samples and photographs of Commelinaceae from Central-Western Brazil. We would also like to thank Mark T. Strong for revising the English and making suggestions for the improvement of this manuscript; Luana Silva Braucks Calazans for suggestions on an early version of the manuscript; and Isa Lucia de Morais Resende, Mateo Fernandez, Suzana Neves Moreira, William Milliken, William Vargas, and Vinicius Castro Souza for the beautiful field photos. Finally, the authors would like to thank all the curators and staff from the cited herbaria, especially Ranee Prakash and Sandra Knapp (Natural History Museum of London), Martin Xanthos (Royal Botanical Gardens, Kew), and Subir Bandyopadhyay and Parigi Prasanna (Botanical Survey of India) for all the help finding the needed specimens. RFA thanks FAPESB (DEB BOL0584/2013) for his Ph.D. scholarship. MOOP thanks CAPES for his Master scholarship granted from 2013-2015 (UFRJ) and for his current Ph.D. scholarship (USP), besides Fundacao Flora de Apoio a Botanica and Smithsonian Institution for his REFLORA grant. This study was carried out as part of the first author's Ph.D. degree in Botany at Programa de Pos-Graduacao em Botanica, Instituto de Biociencias, Universidade de Sao Paulo - USP. NR 52 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 74 BP 35 EP 78 DI 10.3897/phytokeys.74.9835 PG 44 WC Plant Sciences SC Plant Sciences GA ED3EA UT WOS:000388731000003 ER PT S AU Batista-Navarro, R Hammock, J Ulate, W Ananiadou, S AF Batista-Navarro, Riza Hammock, Jennifer Ulate, William Ananiadou, Sophia BE Fuhr, N Kovacs, L Risse, T Nejdl, W TI A Text Mining Framework for Accelerating the Semantic Curation of Literature SO RESEARCH AND ADVANCED TECHNOLOGY FOR DIGITAL LIBRARIES, TPDL 2016 SE Lecture Notes in Computer Science LA English DT Proceedings Paper CT 20th International Conference on Theory and Practice of Digital Libraries (TPDL) CY SEP 05-09, 2016 CL Hannover, GERMANY SP Elsevier B V, Ex Libris, L3S Res Ctr, German Natl Lib Sci & Technol AB The Biodiversity Heritage Library is the world's largest digital library of biodiversity literature. Currently containing almost 40 million pages, the library can be explored with a search interface employing keyword-matching, which unfortunately fails to address issues brought about by ambiguity. Helping alleviate these issues are tools that automatically attach semantic metadata to documents, e.g., biodiversity concept recognisers. However, gold standard, semantically annotated textual corpora are critical for the development of these advanced tools. In the biodiversity domain, such corpora are almost non-existent especially since the construction of semantically annotated resources is typically a time-consuming and laborious process. Aiming to accelerate the development of a corpus of biodiversity documents, we propose a text mining framework that hastens curation through an iterative feedback-loop process of (1) manual annotation, and (2) training and application of statistical concept recognition models. Even after only a few iterations, our curators were observed to have spent less time and effort on annotation. C1 [Batista-Navarro, Riza; Ananiadou, Sophia] Univ Manchester, Sch Comp Sci, Manchester M13 9PL, Lancs, England. [Hammock, Jennifer] Smithsonian Inst, Washington, DC 20560 USA. [Ulate, William] Missouri Bot Garden, St Louis, MO USA. RP Batista-Navarro, R (reprint author), Univ Manchester, Sch Comp Sci, Manchester M13 9PL, Lancs, England. EM riza.batista@manchester.ac.uk OI Hammock, Jennifer/0000-0002-9943-2342 NR 3 TC 0 Z9 0 U1 0 U2 0 PU SPRINGER INT PUBLISHING AG PI CHAM PA GEWERBESTRASSE 11, CHAM, CH-6330, SWITZERLAND SN 0302-9743 BN 978-3-319-43997-6; 978-3-319-43996-9 J9 LECT NOTES COMPUT SC PY 2016 VL 9819 BP 459 EP 462 DI 10.1007/978-3-319-43997-6_44 PG 4 WC Computer Science, Information Systems; Computer Science, Theory & Methods; Information Science & Library Science SC Computer Science; Information Science & Library Science GA BG4OK UT WOS:000389021000044 ER PT S AU Evans, IN Budynkiewicz, JA Evans, JD Miller, JB Onyuksel, C Paxson, C Plummer, DA AF Evans, Ian N. Budynkiewicz, Jamie A. Evans, Janet DePonte Miller, Joseph B. Onyuksel, Cem Paxson, Charles Plummer, David A. BE Chiozzi, G Guzman, JC TI Software requirements flow-down and preliminary software design for the G-CLEF spectrograph SO SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Software and Cyberinfrastructure for Astronomy IV CY JUN 26-30, 2016 CL Edinburgh, SCOTLAND SP SPIE DE G-CLEF; GMT; instrument control software; data reduction pipelines; requirements analysis; software design process ID SPECTROSCOPY; EXTRACTION AB The Giant Magellan Telescope (GMT)-Consortium Large Earth Finder (G-CLEF) is a fiber-fed, precision radial velocity (PRV) optical echelle spectrograph that will be the first light instrument on the GMT. The G-CLEF instrument device control subsystem (IDCS) provides software control of the instrument hardware, including the active feedback loops that are required to meet the G-CLEF PRV stability requirements. The IDCS is also tasked with providing operational support packages that include data reduction pipelines and proposal preparation tools. A formal, but ultimately pragmatic approach is being used to establish a complete and correct set of requirements for both the G-CLEF device control and operational support packages. The device control packages must integrate tightly with the state-machine driven software and controls reference architecture designed by the GMT Organization. A model-based systems engineering methodology is being used to develop a preliminary design that meets these requirements. Through this process we have identified some lessons that have general applicability to the development of software for ground-based instrumentation. For example, tasking an individual with overall responsibility for science/software/hardware integration is a key step to ensuring effective integration between these elements. An operational concept document that includes detailed routine and non routine operational sequences should be prepared in parallel with the hardware design process to tie together these elements and identify any gaps. Appropriate time-phasing of the hardware and software design phases is important, but revisions to driving requirements that impact software requirements and preliminary design are inevitable. Such revisions must be carefully managed to ensure efficient use of resources. C1 [Evans, Ian N.; Budynkiewicz, Jamie A.; Evans, Janet DePonte; Miller, Joseph B.; Onyuksel, Cem; Paxson, Charles; Plummer, David A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St,MS-81, Cambridge, MA 02138 USA. RP Evans, IN (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St,MS-81, Cambridge, MA 02138 USA. EM ievans@cfa.harvard.edu NR 21 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0205-2; 978-1-5106-0206-9 J9 PROC SPIE PY 2016 VL 9913 AR UNSP 99131Q DI 10.1117/12.2232163 PG 17 WC Astronomy & Astrophysics; Engineering, Electrical & Electronic; Optics SC Astronomy & Astrophysics; Engineering; Optics GA BG4GJ UT WOS:000388804600059 ER PT S AU Jenkins, JM Twicken, JD McCauliff, S Campbell, J Sanderfer, D Lung, D Mansouri-Samani, M Girouard, F Tenenbaum, P Klaus, T Smith, JC Caldwell, DA Chacon, AD Henze, C Heiges, C Latham, DW Morgan, E Swade, D Rinehart, S Vanderspek, R AF Jenkins, Jon M. Twicken, Joseph D. McCauliff, Sean Campbell, Jennifer Sanderfer, Dwight Lung, David Mansouri-Samani, Masoud Girouard, Forrest Tenenbaum, Peter Klaus, Todd Smith, Jeffrey C. Caldwell, Douglas A. Chacon, A. Dean Henze, Christopher Heiges, Cory Latham, David W. Morgan, Edward Swade, Daryl Rinehart, Stephen Vanderspek, Roland BE Chiozzi, G Guzman, JC TI The TESS Science Processing Operations Center SO SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Software and Cyberinfrastructure for Astronomy IV CY JUN 26-30, 2016 CL Edinburgh, SCOTLAND SP SPIE DE transit photometry; science pipelines; TESS mission; exoplanets; high performance computing AB The Transiting Exoplanet Survey Satellite (TESS) will conduct a search for Earth's closest cousins starting in early 2018 and is expected to discover similar to 1,000 small planets with R-p < 4 R circle plus and measure the masses of at least 50 of these small worlds. The Science Processing Operations Center (SPOC) is being developed at NASA Ames Research Center based on the Kepler science pipeline and will generate calibrated pixels and light curves on the NASA Advanced Supercomputing Division's Pleiades supercomputer. The SPOC will also search for periodic transit events and generate validation products for the transit-like features in the light curves. All TESS SPOC data products will be archived to the Mikulski Archive for Space Telescopes (MAST). C1 [Jenkins, Jon M.; Sanderfer, Dwight; Henze, Christopher] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA. [Twicken, Joseph D.; Tenenbaum, Peter; Smith, Jeffrey C.; Caldwell, Douglas A.] NASA, Ames Res Ctr, SETI Inst, Moffett Field, CA 94035 USA. [McCauliff, Sean; Campbell, Jennifer] NASA, Ames Res Ctr, Wyle Labs, Moffett Field, CA 94035 USA. [Lung, David; Chacon, A. Dean] NASA, Ames Res Ctr, Millenium Engn, Moffett Field, CA 94035 USA. [Mansouri-Samani, Masoud; Klaus, Todd] SGT Inc, NASA, Ames Res Ctr, Moffett Field, CA USA. [Girouard, Forrest] Logyx LLC, NASA, Ames Res Ctr, Moffett Field, CA USA. [Heiges, Cory] NASA, Goddard Space Flight Ctr, Gen Dynam, Greenbelt, MD USA. [Latham, David W.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Morgan, Edward; Vanderspek, Roland] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Swade, Daryl] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA. [Rinehart, Stephen] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA. RP Jenkins, JM (reprint author), NASA, Ames Res Ctr, Moffett Field, CA 94035 USA. EM jon.m.jenkins@nasa.gov NR 7 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0205-2; 978-1-5106-0206-9 J9 PROC SPIE PY 2016 VL 9913 AR UNSP 99133E DI 10.1117/12.2233418 PG 20 WC Astronomy & Astrophysics; Engineering, Electrical & Electronic; Optics SC Astronomy & Astrophysics; Engineering; Optics GA BG4GJ UT WOS:000388804600111 ER PT S AU Patel, NA Nishioka, H Huang, CWL AF Patel, Nimesh A. Nishioka, Hiroaki Huang, Chih-Wei Locutus BE Chiozzi, G Guzman, JC TI Control and monitoring software for the Greenland Telescope SO SOFTWARE AND CYBERINFRASTRUCTURE FOR ASTRONOMY IV SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Software and Cyberinfrastructure for Astronomy IV CY JUN 26-30, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Radio telescopes; Control software; Pointing calibration ID PROJECT AB The Greenland Telescope (GLT) is a 12m diameter antenna that is being developed from the ALMA North America prototype antenna, for VLBI observations and single-dish science approaching THz, at the Summit station in Greenland. The GLT is a collaboration between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics. We describe the control and monitoring software that is being developed for GLT. The present version of the software is ready for the initial tests of the antenna at Thule, including optical and radio pointing calibration, holography, and VLBI observations at 230 GHz. C1 [Patel, Nimesh A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Nishioka, Hiroaki; Huang, Chih-Wei Locutus] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei, Taiwan. RP Patel, NA (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM npatel@cfa.harvard.edu NR 16 TC 1 Z9 1 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0205-2; 978-1-5106-0206-9 J9 PROC SPIE PY 2016 VL 9913 AR UNSP 991308 DI 10.1117/12.2232409 PG 8 WC Astronomy & Astrophysics; Engineering, Electrical & Electronic; Optics SC Astronomy & Astrophysics; Engineering; Optics GA BG4GJ UT WOS:000388804600007 ER PT J AU Schwartz, GE Redfern, LK Ikuma, K Gunsch, CK Ruhl, LS Vengosh, A Hsu-Kim, H AF Schwartz, Grace E. Redfern, Lauren K. Ikuma, Kaoru Gunsch, Claudia K. Ruhl, Laura S. Vengosh, Avner Hsu-Kim, Heileen TI Impacts of coal ash on methylmercury production and the methylating microbial community in anaerobic sediment slurries SO ENVIRONMENTAL SCIENCE-PROCESSES & IMPACTS LA English DT Article ID FRESH-WATER SEDIMENTS; MERCURY METHYLATION; FLORIDA EVERGLADES; ORGANIC-MATTER; POWER-PLANTS; GENE HGCA; SULFIDE; BIOAVAILABILITY; MICROORGANISMS; MECHANISMS AB Mercury (Hg) associated with coal ash is an environmental concern, particularly if the release of coal ash to the environment is associated with the conversion of inorganic Hg to methylmercury (MeHg), a bioaccumulative form of Hg that is produced by anaerobic microorganisms. In this study, sediment slurry microcosm experiments were performed to understand how spilled coal ash might influence MeHg production in anaerobic sediments of an aquatic ecosystem. Two coal ash types were used: (1) a weathered coal ash; and (2) a freshly collected, unweathered fly ash that was relatively enriched in sulfate and Hg compared to the weathered ash. These ash samples were added to anaerobic sediment slurries constructed with a relatively pristine sediment (containing 0.03 mg kg(-1) Hg) and a Hg-contaminated sediment (containing 0.29 mg kg(-1) Hg). The results of these experiments showed negligible net production of MeHg in microcosms with no ash and in microcosms amended with the low sulfate/low Hg ash. In contrast, slurry microcosms amended with high sulfate/high Hg ash showed increases in total MeHg content that was 2 to 3 times greater than control microcosms without ash (p < 0.001). 16S amplicon sequencing of microbial communities in the slurries indicated that the coal ash addition generally increased the relative abundance of the methylating microbial community, including sulfate-reducing bacteria and iron-reducing bacteria species that are known to be efficient methylators of Hg. The stimulation of these microorganisms was likely caused by the release of substrates (sulfate and Fe) originating from the ash. Overall, the results highlight the need to incorporate both environmental parameters and coal ash characteristics into risk assessments that guide coal ash management and disposal. C1 [Schwartz, Grace E.; Redfern, Lauren K.; Gunsch, Claudia K.; Hsu-Kim, Heileen] Duke Univ, Dept Civil & Environm Engn, 121 Hudson Hall, Durham, NC 27708 USA. [Ikuma, Kaoru] Iowa State Univ, Dept Civil Construct & Environm Engn, Ames, IA 50011 USA. [Ruhl, Laura S.] Univ Arkansas Little Rock, Dept Earth Sci, Little Rock, Little Rock, AR 72204 USA. [Vengosh, Avner] Duke Univ, Nicholas Sch Environm, Div Earth & Ocean Sci, Durham, NC 27708 USA. [Schwartz, Grace E.] Smithsonian Environm Res Ctr, 647 Contees Wharf Rd, Edgewater, MD 21037 USA. RP Hsu-Kim, H (reprint author), Duke Univ, Dept Civil & Environm Engn, 121 Hudson Hall, Durham, NC 27708 USA. EM hsukim@duke.edu RI Hsu-Kim, Heileen/A-5409-2008; OI Hsu-Kim, Heileen/0000-0003-0675-4308; Ikuma, Kaoru/0000-0003-3715-7821; Gunsch, Claudia/0000-0002-8555-0313 FU Oak Ridge Associated Universities; National Science Foundation [CBET-1235661, OISE-1243433]; Environmental Research and Education Foundation FX We thank the Tennessee Valley Authority, Restoration Services Inc., and Environmental Standards Inc. for their assistance with field sampling. We thank Wenjie Sun and Morton Barlaz for the total sulfate measurements in coal ash. We also thank Neil Carriker, Rock Vitale, Kaitlyn Porter, and Tong Zhang for their assistance. This work was supported with grants from the Oak Ridge Associated Universities and the National Science Foundation (CBET-1235661 and OISE-1243433). G. Schwartz was also supported by a doctoral scholarship from the Environmental Research and Education Foundation. NR 57 TC 0 Z9 0 U1 4 U2 4 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2050-7887 EI 2050-7895 J9 ENVIRON SCI-PROC IMP JI Environ. Sci.-Process Impacts PY 2016 VL 18 IS 11 BP 1427 EP 1439 DI 10.1039/c6em00458j PG 13 WC Chemistry, Analytical; Environmental Sciences SC Chemistry; Environmental Sciences & Ecology GA EC9MV UT WOS:000388469600006 PM 27722355 ER PT B AU Ubelaker, DH AF Ubelaker, Douglas H. BE Siegel, JA TI Forensic Chemistry Series preface SO FORENSIC CHEMISTRY: FUNDAMENTALS AND APPLICATIONS SE Forensic Science in Focus LA English DT Editorial Material; Book Chapter C1 [Ubelaker, Douglas H.] Smithsonian Inst, Washington, DC 20560 USA. RP Ubelaker, DH (reprint author), Smithsonian Inst, Washington, DC 20560 USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU JOHN WILEY & SONS LTD PI CHICHESTER PA THE ATRIUM, SOUTHERN GATE, CHICHESTER PO19 8SQ, WEST SUSSEX, ENGLAND BN 978-1-118-89773-7; 978-1-118-89772-0 J9 FORENSIC SCI FOC PY 2016 BP XV EP XV PG 1 WC Chemistry, Analytical; Medicine, Legal SC Chemistry; Legal Medicine GA BF8UG UT WOS:000385233400001 ER PT J AU Mossbrucker, AM Fleming, CH Imron, MA Pudyatmoko, S Sumardi AF Mossbrucker, Alexander Markus Fleming, Christen H. Imron, Muhammad Ali Pudyatmoko, Satyawan Sumardi TI AKDE(C) home range size and habitat selection of Sumatran elephants SO WILDLIFE RESEARCH LA English DT Article DE area-corrected autocorrelated kernel density estimation; Asian elephant; Bukit Tigapuluh; elephant conservation; Elephas maximus sumatranus; habitat preference; movement behaviour; ranging behaviour; resource selection ID FRAGMENTED RAIN-FOREST; ASIAN ELEPHANT; RESOURCE USE; CONSERVATION; MOVEMENT; MAXIMUS; POPULATION; DISPERSAL; LANDSCAPE; TELEMETRY AB Context. Understanding ranging behaviour and habitat selection of threatened species is crucial for the development of conservation strategies and the design of conservation areas. Our understanding of the actual needs of the critically endangered Sumatran elephant in this context is insufficient. Aims. Provide reliable subspecies-specific information on home range size and habitat selection of Sumatran elephants. Methods. Using both the new area-corrected autocorrelated kernel density estimation (AKDE(C)) and two commonly applied conventional methods, the home range sizes of nine Sumatran elephants were estimated. Elephant habitat selection was studied using Manly's selection ratios. Key results. AKDE(C) home ranges of adults ranged from 275 km(2) to 1352 km(2). Estimates obtained using conventional KDE and minimum convex polygon (MCP) ranged between 156 km(2) and 997 km(2). Overall habitat selection was significant for both slope and land-cover type, whereas individual preferences varied to some extent. On the basis of global selection ratios, we found natural forest, pulpwood plantations and gentle slopes (<= 4 degrees) to be significantly selected, whereas most areas affected by human activities and steeper slopes were avoided by the majority of animals included in the study. Conclusions. As expected, AKDE(C) estimates were much larger than those obtained using conventional methods because conventional methods have a tendency to underestimate home range size when confronted with autocorrelated movement data and produce estimates that refer to the limited study period only, whereas AKDE(C) estimates include the predicted animal's long-term space use. The extremely large AKDE(C) estimate obtained for a subadult male most likely represents a combination of population dispersal range and temporary home range rather than its final adult home range. Regardless, it appears that Sumatran elephants roam over much larger areas than previously assumed. Natural forests and relatively flat areas are of great importance for Sumatran elephants. The observed intensive use of pulpwood plantations by one individual is likely because of limited availability of alternative suitable habitats. Implications. Alandscape-wide approach to elephant conservation that takes large home ranges into account, is required, and should include forest protection and restoration and elephant friendly management of existing pulpwood concessions, with special focus on areas with relatively gentle slopes. C1 [Mossbrucker, Alexander Markus; Imron, Muhammad Ali; Pudyatmoko, Satyawan; Sumardi] UGM, Fac Forestry, Jl Agro 1 Bulaksumur, Yogyakarta 55281, Indonesia. [Mossbrucker, Alexander Markus] Frankfurt Zool Soc, Bernhard Grzimek Allee 1, D-60316 Frankfurt, Germany. [Fleming, Christen H.] Natl Zool Pk, Smithsonian Conservat Biol Inst, Conservat Ecol Ctr, 1500 Remount Rd, Front Royal, VA 22630 USA. [Fleming, Christen H.] Univ Maryland, Dept Biol, College Pk, MD 20742 USA. RP Mossbrucker, AM (reprint author), UGM, Fac Forestry, Jl Agro 1 Bulaksumur, Yogyakarta 55281, Indonesia.; Mossbrucker, AM (reprint author), Frankfurt Zool Soc, Bernhard Grzimek Allee 1, D-60316 Frankfurt, Germany. EM islandelephants@gmail.com FU USA Fish & Wildlife Service (USFWS); International Elephant Project (IEP); Perth Zoo (Western Australia); Disney Conservation Fund FX We thank the USA Fish & Wildlife Service (USFWS), the International Elephant Project (IEP), Perth Zoo (Western Australia), and the Disney Conservation Fund for financial support, the Veterinary Society for Sumatran Wildlife Conservation (VESSWIC) for partial support of veterinary drugs and consumables, Setiabudi and the World Wide Fund for Nature (WWF) Indonesia for providing land-cover data, and Dr Martin Wikelski (Max Planck Institute for Ornithology) for donating a GPS collar. We are grateful to the Indonesian State Ministry of Research and Technology (RISTEK) and the Ministry of Environment and Forestry for granting permits for our research and to the department of Conservation of Natural Resources and Ecosystem (Konservasi Sumber Daya Alam dan Ekosistem (KSDAE), formerly BKSDA) for their kind support of field work. We are very thankful to Christopher Stremme, Nazaruddin and Hidayat for their invaluable support of elephant collaring and to Dr Kamran Safi for valuable advice concerning movement-data analysis. Further, the authors thank Dr Amanda Fernie for carefully reviewing of the English and two anonymous reviewers and the editor team of Wildlife Research for their valuable comments and suggestions on the manuscript. Special thanks go to Leif Cocks and Kylie Bullo (The Orangutan Project, TOP, and IEP) and to Dr Peter-Hinrich Pratje and the entire team of Frankfurt Zoological Society (FZS) for their enthusiastic and wide-ranging support. NR 65 TC 0 Z9 0 U1 11 U2 11 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1035-3712 EI 1448-5494 J9 WILDLIFE RES JI Wildl. Res. PY 2016 VL 43 IS 7 BP 566 EP 575 DI 10.1071/WR16069 PG 10 WC Ecology; Zoology SC Environmental Sciences & Ecology; Zoology GA EC9CG UT WOS:000388440700004 ER PT J AU Ashworth, AC Erwin, TL AF Ashworth, Allan C. Erwin, Terry L. TI Antarctotrechus balli sp n. (Carabidae, Trechini): the first ground beetle from Antarctica SO ZOOKEYS LA English DT Article DE Trechini; Carabidae; Antarctica; Miocene ID PLIOCENE SIRIUS GROUP; TRANSANTARCTIC MOUNTAINS; MIDDLE MIOCENE; COLEOPTERA; MARINE; LEAVES; RANGE AB Fossil elytra of a small trechine carabid are reported from the Oliver Bluffs on the Beardmore Glacier at lat. 85 degrees S. They were compared with counterparts from the extant genera Trechisibus, Tasmanorites, Oxytrechus and Pseudocnides. The fossils share some characters but are sufficiently different to be described as a new genus and species. We named the new species Antarctotrechus balli in honour of George E. Ball who made major contributions to the study of carabids through his own research and the training of students while at the University of Alberta, Edmonton, Alberta, Canada. The closest extant relatives to the extinct A. balli are species of Trechisibus, which inhabit South America, the Falkland Islands and South Georgia, and Tasmanorites, which inhabit Tasmania, Australia. Plant fossils associated with A. balli included Nothofagus (southern beech), Ranunculus (buttercup), moss mats and cushion plants that were part of a tundra biome. Collectively, the stratigraphic relationships and the growth characteristics of the fossil plants indicate that A. balli inhabited the sparsely-vegetated banks of a stream that was part of an outwash plain at the head of a fjord in the Transantarctic Mountains. Other insects represented by fossils in the tundra biome include a listroderine weevil and a cyclorrhaphan fly. The age of the fossils, based on comparison of associated pollen with Ar-40/Ar-39 dated pollen assemblages from the McMurdo Dry Valleys, is probably Early to Mid-Miocene in the range 14-20 Ma. The tundra biome, including A. balli, became extinct in the interior of Antarctica about 14 Ma and on the margins of the continent by 10-13 Ma. A. balli confirms that trechines were once widely distributed in Gondwana. For A. balli and other elements of the tundra biome it appears they continued to inhabit a warmer Antarctica for many millions of years after rifting of Tasmania (45 Ma) and southern South America (31 Ma). C1 [Ashworth, Allan C.] North Dakota State Univ, Dept Geosci, Quaternary Entomol Lab, Fargo, ND 58108 USA. [Erwin, Terry L.] Natl Museum Nat Hist, Smithsonian Inst, Hyper Divers Grp, Dept Entomol, MRC 187,POB 37012, Washington, DC 20013 USA. RP Ashworth, AC (reprint author), North Dakota State Univ, Dept Geosci, Quaternary Entomol Lab, Fargo, ND 58108 USA. EM allan.ashworth@ndsu.edu FU NSF [9615252, 0947821] FX We extend hearty thanks to Karolyn Darrow of the Department of Entomology at the Smithsonian Institution for elytron images and outline drawings of adults of extant three species of Trechisibus. We also warmly thank David Maddison for assistance in understanding the southern trechine complexity. ACA acknowledges the logistics support of the US Antarctic program for the field study on the Beardmore Glacier and colleagues who assisted in the field study: David Cantrill, Jane Francis, Forrest McCarthy, Marty Reed and Steve Roof. The research was supported by NSF grants 9615252 and 0947821. NR 33 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 635 BP 109 EP 122 DI 10.3897/zookeys.635.10535 PG 14 WC Zoology SC Zoology GA ED0BV UT WOS:000388508900006 PM 27917060 ER PT S AU Zych, M Pikovski, I Costa, F Brukner, C AF Zych, M. Pikovski, I. Costa, F. Brukner, C. BE Riehle, F TI General relativistic effects in quantum interference of "clocks" SO 8TH SYMPOSIUM ON FREQUENCY STANDARDS AND METROLOGY 2015 SE Journal of Physics Conference Series LA English DT Proceedings Paper CT 8th Symposium on Frequency Standards and Metrology CY OCT 12-16, 2015 CL Potsdam, GERMANY SP Physikalisch Technische Bundesanstalt, Helmholtz Fonds e V, Natl Inst Standards & Technol, First TF, Observ Paris, Ctr Natl Rech Sci, Lab Natl Metrologie & Dessais, Deutsche Forschungsgemeinschaft ID WORLD ATOMIC CLOCKS; NEUTRON INTERFEROMETER; TIME GAINS; 4TH TEST; WAVE; DECOHERENCE; MOLECULES; EVOLUTION; GRAVITY; WITNESS AB Quantum mechanics and general relativity have been each successfully tested in numerous experiments. However, the regime where both theories are jointly required to explain physical phenomena remains untested by laboratory experiments, and is also not fully understood by theory. This contribution reviews recent ideas for a new type of experiments: quantum interference of "clocks", which aim to test novel quantum effects that arise from time dilation. "Clock" interference experiments could be realised with atoms or photons in near future laboratory experiments. C1 [Zych, M.; Costa, F.] Univ Queensland, Ctr Engn Quantum Syst, Sch Math & Phys, St Lucia, Qld 4072, Australia. [Pikovski, I.] Harvard Smithsonian Ctr Astrophys, ITAMP, Cambridge, MA 02138 USA. [Pikovski, I.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Brukner, C.] Austrian Acad Sci, Inst Quantum Opt & Quantum Informat, Boltzmanngasse 3, A-1090 Vienna, Austria. [Brukner, C.] Univ Vienna, Fac Phys, Boltzmanngasse 5, A-1090 Vienna, Austria. RP Zych, M (reprint author), Univ Queensland, Ctr Engn Quantum Syst, Sch Math & Phys, St Lucia, Qld 4072, Australia. EM m.zych@uq.edu.au RI Costa, Fabio/G-3746-2014; Zych, Magdalena/G-4007-2014; OI Costa, Fabio/0000-0002-6547-6005; Zych, Magdalena/0000-0002-8356-7613; Pikovski, Igor/0000-0002-9441-2553 NR 51 TC 0 Z9 0 U1 0 U2 0 PU IOP PUBLISHING LTD PI BRISTOL PA DIRAC HOUSE, TEMPLE BACK, BRISTOL BS1 6BE, ENGLAND SN 1742-6588 J9 J PHYS CONF SER PY 2016 VL 723 AR UNSP 012044 DI 10.1088/1742-6596/723/1/012044 PG 13 WC Instruments & Instrumentation; Physics, Multidisciplinary SC Instruments & Instrumentation; Physics GA BG2YF UT WOS:000387774800044 ER PT S AU Baldwin, D Szentgyorgyi, A Barnes, S Bean, J Ben-Ami, S Brennan, P Budynkiewicz, J Chun, MY Conroy, C Crane, JD Epps, H Evans, I Evans, J Foster, J Frebel, A Gauron, T Guzman, D Hare, T Jang, BH Jang, JG Jordan, A Kim, J Kim, KM de Oliveira, CM Lopez-Morales, M McCracken, K McMuldroch, S Miller, J Mueller, M Oh, JS Ordway, M Park, BG Park, C Park, SJ Paxson, C Phillips, D Plummer, D Podgorski, W Seifahrt, A Stark, D Steiner, J Uomoto, A Walsworth, R Yu, YS AF Baldwin, Dan Szentgyorgyi, Andrew Barnes, Stuart Bean, Jacob Ben-Ami, Sagi Brennan, Patricia Budynkiewicz, Jamie Chun, Moo-Young Conroy, Charlie Crane, Jeffrey D. Epps, Harland Evans, Ian Evans, Janet Foster, Jeff Frebel, Anna Gauron, Thomas Guzman, Dani Hare, Tyson Jang, Bi-Ho Jang, Jeong-Gyun Jordan, Andres Kim, Jihun Kim, Kang-Min de Oliveira, Claudia Mendes Lopez-Morales, Mercedes McCracken, Kenneth McMuldroch, Stuart Miller, Joseph Mueller, Mark Oh, Jae Sok Ordway, Mark Park, Byeong-Gon Park, Chan Park, Sung-Joon Paxson, Charles Phillips, David Plummer, David Podgorski, William Seifahrt, Andreas Stark, Daniel Steiner, Joao Uomoto, Alan Walsworth, Ronald Yu, Young-Sam BE Navarro, R Burge, JH TI Advanced Structural Design for Precision Radial Velocity Instruments SO ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION II SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II CY JUN 26-JUL 01, 2016 CL Edinburgh, UNITED KINGDOM SP SPIE DE Echelle spectrograph; precision radial velocity; G -CLEF; GMT; composite optical bench; thermal stability; mechanical stability; low CIE AB The GMT-Consortium Large Earth Finder (G-CLEF) is an echelle spectrograph with precision radial velocity (PRV) capability that will be a first light instrument for the Giant Magellan Telescope (GMT). G-CLEF has a PRV precision goal of 40 cm/sec (10 cm/s for multiple measurements) to enable detection of Earth-like exoplanets in the habitable zones of sun-like stars'. This precision is a primary driver of G-CLEF's structural design. Extreme stability is necessary to minimize image motions at the CCD detectors. Minute changes in temperature, pressure, and acceleration environments cause structural deformations, inducing image motions which degrade PRV precision. The instrument's structural design will ensure that the PRV goal is achieved under the environments G-CLEF will be subjected to as installed on the GMT azimuth platform, including: Millikelvin (0.001 K) thermal soaks and gradients 10 millibar changes in ambient pressure Changes in acceleration due to instrument tip/tilt and telescope slewing Carbon fiber/cyanate composite was selected for the optical bench structure in order to meet performance goals. Low coefficient of thermal expansion (C 1E) and high stiffness-to-weight are key features of the composite optical bench design. Manufacturability and serviceability of the instrument are also drivers of the design. In this paper, we discuss analyses leading to technical choices made to minimize G-CLEF's sensitivity to changing environments. Finite element analysis (FEA) and image motion sensitivity studies were conducted to determine PRV performance under operational environments. We discuss the design of the optical bench structure to optimize stiffness to -weight and minimize deformations due to inertial and pressure effects. We also discuss quasi-kinematic mounting of optical elements and assemblies, and optimization of these to ensure minimal image motion under thermal, pressure, and inertial loads expected during PRV observations. C1 [Baldwin, Dan; Szentgyorgyi, Andrew; Barnes, Stuart; Ben-Ami, Sagi; Brennan, Patricia; Budynkiewicz, Jamie; Conroy, Charlie; Evans, Ian; Evans, Janet; Foster, Jeff; Gauron, Thomas; Lopez-Morales, Mercedes; McCracken, Kenneth; McMuldroch, Stuart; Miller, Joseph; Mueller, Mark; Ordway, Mark; Paxson, Charles; Phillips, David; Plummer, David; Podgorski, William; Walsworth, Ronald] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02140 USA. [Stark, Daniel] Univ Arizona, Steward Observ, 933 North Cherry St, Tucson, AZ 85721 USA. [Crane, Jeffrey D.; Hare, Tyson; Uomoto, Alan] Carnegie Inst Sci, 813 Santa Barbara St, Pasadena, CA 91101 USA. [Guzman, Dani; Jordan, Andres] Pontificia Univ Catolica Chile, Vicuna Mackenna 4860, Santiago, Chile. [Bean, Jacob] Univ Chicago, 640 S Ellis Ave, Chicago, IL 60637 USA. [Chun, Moo-Young; Jang, Bi-Ho; Jang, Jeong-Gyun; Kim, Jihun; Kim, Kang-Min; Oh, Jae Sok; Park, Byeong-Gon; Park, Chan; Park, Sung-Joon; Yu, Young-Sam] Korea Astron & Space Sci Inst KASI, 776 Daedeokdae Ro, Daejeon, South Korea. [Frebel, Anna] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Epps, Harland] Univ Calif Santa Cruz, Univ Calif Observ, Lick Observ, Santa Cruz, CA 95064 USA. [de Oliveira, Claudia Mendes; Steiner, Joao] Univ Sao Paolo, Rua Matao 1226, BR-05508900 Sao Paulo, Brazil. RP Baldwin, D (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02140 USA. NR 8 TC 0 Z9 0 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0203-8; 978-1-5106-0204-5 J9 PROC SPIE PY 2016 VL 9912 AR UNSP 99123I DI 10.1117/12.2235250 PN 1 PG 16 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BG2XH UT WOS:000387747900106 ER PT S AU Goble, W Ortiz, R AF Goble, William Ortiz, Ricardo BE Navarro, R Burge, JH TI Characterization of an integrally wound tungsten and aluminum filament for physical vapor deposition SO ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION II SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II CY JUN 26-JUL 01, 2016 CL Edinburgh, UNITED KINGDOM SP SPIE DE physical vapor deposition; aluminization; tungsten filament; MMT Observatory AB As part of the effort to increase the reliability of the MMT Observatory (MMTO) 6.5m Primary Mirror Coating System, the specified filament has changed from a configuration in which the aluminum charge is hand wound around a tungsten filament to a configuration in which the aluminum is integrally wound with the tungsten at the time of filament manufacture. In the MMTO configuration, this filament consists of the three strands of tungsten wire and one strand of aluminum wire. In preparation of a full system test utilizing two hundred filaments fired simultaneously, an extensive testing program was undertaken to characterize these filaments using a four filament configuration in the MMTO small coating chamber (0.5m) and then a forty filament configuration in the University of Arizona Steward Observatory coating chamber (2m). The testing using the smaller coating chambers has shown these filaments provide very predicable coatings from test to test, and with the proper heating profile, these filaments greatly reduce the likelihood of aluminum drips. The initial filament design was modified during the course of testing by shortening the unwound filament length to closer match the aluminum load required in the MMTO coating chamber. This change increased the aluminum deposition rates without increasing the power delivered of the filament power supplies (commercial welders). Filament power levels measured at the vacuum chamber feedthroughs, currents, and deposition rates from multiple coating tests, including a full system test, are presented. C1 [Goble, William; Ortiz, Ricardo] Univ Arizona, MMT Observ, Tucson, AZ 85721 USA. [Goble, William; Ortiz, Ricardo] Smithsonian Inst, MMT Observ, Washington, DC 20560 USA. [Goble, William; Ortiz, Ricardo] Univ Arizona, Tucson, AZ 85721 USA. RP Goble, W (reprint author), Univ Arizona, MMT Observ, Tucson, AZ 85721 USA.; Goble, W (reprint author), Smithsonian Inst, MMT Observ, Washington, DC 20560 USA.; Goble, W (reprint author), Univ Arizona, Tucson, AZ 85721 USA. EM wgoble@mmto.org NR 3 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0203-8; 978-1-5106-0204-5 J9 PROC SPIE PY 2016 VL 9912 AR UNSP 991238 DI 10.1117/12.2233637 PN 1 PG 8 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BG2XH UT WOS:000387747900097 ER PT S AU Phillips, DF Glenday, AG Dumusque, X Buchschacher, N Cameron, AC Cecconi, M Charbonneau, D Cosentino, R Ghedina, A Haywood, R Latham, DW Li, CH Lodi, M Lovis, C Molinari, E Pepe, F Sasselov, D Szentgyorgyi, A Udry, S Walsworth, RL AF Phillips, David F. Glenday, Alex G. Dumusque, Xavier Buchschacher, Nicolas Cameron, Andrew Collier Cecconi, Massimo Charbonneau, David Cosentino, Rosario Ghedina, Adriano Haywood, Raphaelle Latham, David W. Li, Chih-Hao Lodi, Marcello Lovis, Christophe Molinari, Emilio Pepe, Francesco Sasselov, Dimitar Szentgyorgyi, Andrew Udry, Stephane Walsworth, Ronald L. BE Navarro, R Burge, JH TI An astro-comb calibrated solar telescope to search for the radial velocity signature of Venus SO ADVANCES IN OPTICAL AND MECHANICAL TECHNOLOGIES FOR TELESCOPES AND INSTRUMENTATION II SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Advances in Optical and Mechanical Technologies for Telescopes and Instrumentation II CY JUN 26-JUL 01, 2016 CL Edinburgh, UNITED KINGDOM SP SPIE ID LASER FREQUENCY COMB; HARPS-N; ASTROPHYSICAL SPECTROGRAPH; SUN; PLANET; SYSTEM; STAR; SDO AB We recently demonstrated sub-m/s sensitivity in measuring the radial velocity (RV) between the Earth and Sun using a simple solar telescope feeding the HARPS-N spectrograph at the Italian National Telescope, which is calibrated with a green astro-comb. We are using the solar telescope to characterize the effects of stellar (solar) RV jitter due to activity on the solar surface with the goal of detecting the solar RV signal from Venus, thereby demonstrating the sensitivity of these instruments to detect true Earth-twin exoplanets. C1 [Phillips, David F.; Charbonneau, David; Haywood, Raphaelle; Latham, David W.; Sasselov, Dimitar; Szentgyorgyi, Andrew; Walsworth, Ronald L.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Glenday, Alex G.] Komodo Hlth Inc, New York, NY USA. [Dumusque, Xavier; Buchschacher, Nicolas; Lovis, Christophe; Pepe, Francesco; Udry, Stephane] Observ Geneva, 51 Ch Maillettes, CH-1290 Sauverny, Switzerland. [Cameron, Andrew Collier] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland. [Cecconi, Massimo; Cosentino, Rosario; Ghedina, Adriano; Lodi, Marcello; Molinari, Emilio] INAF Fdn Galileo Galilei, Rambla Jose Ana Fernandez Perez 7, E-38712 Brena Baja, Spain. [Li, Chih-Hao] AOSense Inc, Sunnyvale, CA 94085 USA. [Molinari, Emilio] INAF IASF Milano, Via Bassini 15, I-20133 Milan, Italy. RP Phillips, DF (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM dphil@cfa.harvard.edu NR 24 TC 0 Z9 0 U1 2 U2 2 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0203-8; 978-1-5106-0204-5 J9 PROC SPIE PY 2016 VL 9912 AR UNSP 99126Z PN 1 PG 8 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BG2XH UT WOS:000387747900208 ER PT B AU Wulff, J AF Wulff, Janie BE Hubbard, DK Rogers, CS Lipps, JH Stanley, GD TI Sponge Contributions to the Geology and Biology of Reefs: Past, Present, and Future SO CORAL REEFS AT THE CROSSROADS SE Coral Reefs of the World LA English DT Article; Book Chapter DE Sponges; Reef-building; Reef restoration and repair; Water column filtering; Positive ecosystem roles of sponges on coral reefs ID DEMOSPONGE CLIONA-ORIENTALIS; CARIBBEAN CORAL-REEF; TERPIOS-HOSHINOTA SUBERITIDAE; GIANT BARREL SPONGE; MARINE SPONGES; EXCAVATING SPONGE; MORPHOLOGICAL STRATEGIES; ECOLOGICAL INTERACTIONS; BIODIVERSITY HOTSPOTS; XESTOSPONGIA-MUTA AB Histories of sponges and reefs have been intertwined from the beginning. Paleozoic and Mesozoic sponges generated solid building blocks, and constructed reefs in collaboration with microbes and other encrusting organisms. During the Cenozoic, sponges on reefs have assumed various accessory geological roles, including adhering living corals to the reef frame, protecting solid biogenic carbonate from bioeroders, generating sediment and weakening corals by eroding solid substrate, and consolidating loose rubble to facilitate coral recruitment and reef recovery after physical disturbance. These many influences of sponges on substratum stability, and on coral survival and recruitment, blur distinctions between geological vs. biological roles. Biological roles of sponges on modern reefs include highly efficient filtering of bacteria-sized plankton from the water column, harboring of hundreds of species of animal and plant symbionts, influencing seawater chemistry in conjunction with their diverse microbial symbionts, and serving as food for charismatic megafauna. Sponges may have been playing these roles for hundreds of millions of years, but the meager fossil record of soft-bodied sponges impedes historical analysis. Sponges are masters of intrigue. They play roles that cannot be observed directly and then vanish without a trace, thereby thwarting understanding of their roles in the absence of carefully controlled manipulative experiments and time-series observations. Sponges are more heterogeneous than corals in their ecological requirements and vulnerabilities. Serious misinterpretations have resulted from over-generalizing from a few conspicuous species to the thousands of coral-reef sponge species, representing over twenty orders in three classes, and a great variety of body plans and relationships to corals and solid carbonate substrata. Dynamics of living sponges are difficult to document because most sponges heal after partial mortality and vanish quickly after death. Thus observations of localized increases or overgrowths of corals by a few unusual sponge species have led to recent assertions that sponges are in the process of overwhelming coral reefs. However, a consistent pattern of high mortality in the few long-term census studies done on full assemblages suggests that, perhaps for the first time in their long history, sponges may actually be unable to keep up with changes in the sea. Diminished sponge populations could have profound consequences, many of them negative, for corals and coral reefs. C1 [Wulff, Janie] Florida State Univ, Dept Biol Sci, Tallahassee, FL 32303 USA. [Wulff, Janie] Smithsonian Trop Res Inst, Panama City, Panama. RP Wulff, J (reprint author), Florida State Univ, Dept Biol Sci, Tallahassee, FL 32303 USA.; Wulff, J (reprint author), Smithsonian Trop Res Inst, Panama City, Panama. EM wulff@bio.fsu.edu NR 197 TC 0 Z9 0 U1 1 U2 1 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS BN 978-94-017-7567-0; 978-94-017-7565-6 J9 CORAL REEFS WORLD PY 2016 VL 6 BP 103 EP 126 DI 10.1007/978-94-017-7567-0_5 D2 10.1007/978-94-017-7567-0 PG 24 WC Marine & Freshwater Biology; Zoology SC Marine & Freshwater Biology; Zoology GA BG3NC UT WOS:000388077200006 ER PT J AU Mirbach, CE Brandl, SJ AF Mirbach, Christopher E. Brandl, Simon J. TI Ontogenetic shifts in the social behaviour of pairing coral reef rabbitfishes (Siganidae) SO MARINE BIOLOGY RESEARCH LA English DT Article DE Herbivory; juvenile reef fish; mixed-species pair; pair formation; rabbitfish; schooling; Siganus ID JUVENILE PARROTFISH; COORDINATED VIGILANCE; HERBIVOROUS FISHES; HABITAT COMPLEXITY; CONTINGENCY-TABLES; COLOR PATTERNS; MARINE FISHES; RECRUITMENT; COMPETITORS; POPULATION AB Adult rabbitfishes (Siganidae) differ from most other herbivorous coral reef fishes by forming stable pair bonds throughout their adult lives. However, little is known about the early life stages of rabbitfishes, and no quantitative evidence regarding the ontogeny of pairing behaviour exists to date. This study describes the abundance, distribution and ontogeny of social associations in juvenile rabbitfishes on the mid-shelf reefs around Lizard Island, Great Barrier Reef, Australia. Using underwater visual censuses, we surveyed an area of 5728 m(2) across three distinct habitat types, revealing that the abundance of juveniles varies significantly among species, size class and exposure level. Furthermore, we demonstrate a pronounced ontogenetic shift in the social associations of juveniles of Siganus doliatus and Siganus corallinus, changing from primarily solitary individuals in the smallest size class (<50 mm) to predominantly paired individuals in the larger size classes (50-100 mm and 100-150 mm). In this context, we report the presence of several mixed-species pairs of rabbitfishes, providing the first evidence for this behaviour within the family. This supports previous research, which posits that there are strong ecological drivers, rather than a solely reproductive basis, for pairing behaviour in rabbitfishes. Based on our results, we suggest that further exploration of the ecology of early life stages of herbivorous reef fishes will increase our knowledge about ecological processes on coral reefs. C1 [Mirbach, Christopher E.; Brandl, Simon J.] James Cook Univ, Coll Marine & Environm Sci, Townsville, Qld 4811, Australia. [Brandl, Simon J.] James Cook Univ, ARC Ctr Excellence Coral Reef Studies, Townsville, Qld, Australia. [Brandl, Simon J.] Smithsonian Environm Res Ctr, Tennenbaum Marine Observ Network, Edgewater, MD USA. RP Brandl, SJ (reprint author), James Cook Univ, Coll Marine & Environm Sci, Townsville, Qld 4811, Australia. EM simon.brandl@my.jcu.edu.au FU Great Barrier Reef Foundation FX This research was supported by the Great Barrier Reef Foundation (SJB). NR 46 TC 0 Z9 0 U1 4 U2 4 PU TAYLOR & FRANCIS AS PI OSLO PA KARL JOHANS GATE 5, NO-0154 OSLO, NORWAY SN 1745-1000 EI 1745-1019 J9 MAR BIOL RES JI Mar. Biol. Res. PY 2016 VL 12 IS 8 BP 874 EP 880 DI 10.1080/17451000.2016.1203952 PG 7 WC Ecology; Marine & Freshwater Biology SC Environmental Sciences & Ecology; Marine & Freshwater Biology GA EB8QI UT WOS:000387655500009 ER PT S AU Conan, R Bouchez, A Quiros-Pacheco, F McLeod, B Ashby, D AF Conan, R. Bouchez, A. Quiros-Pacheco, F. McLeod, B. Ashby, D. BE Marchetti, E Close, LM Veran, JP TI The GMT active optics control strategies SO ADAPTIVE OPTICS SYSTEMS V SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Adaptive Optics Systems V CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE AB The Giant Magellan Telescope (GMT) has a Gregorian 25.4-meter diameter primary mirror composed of seven 8.4-meter diameter segments. The secondary mirror consists of seven 1.1-meter diameter segments. In the active and adaptive operation modes of the GMT, around a dozen wavefront sensors are selectively used to monitor the optical aberrations across the focal plane. A dedicated wavefront control system drives slow and fast corrections at the M1 and M2 mirrors to deliver image quality optimized for the field of view of the scientific instrument in use. This paper describes the control strategies for the active optics mode of the GMT. Different wavefront estimation algorithm are compared and the performance of the GMT is evaluated using the Dynamic Optical Simulation package. C1 [Conan, R.; Bouchez, A.; Quiros-Pacheco, F.; Ashby, D.] GMTO, 465 N Halstead Ave, Pasadena, CA 91107 USA. [McLeod, B.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Conan, R (reprint author), GMTO, 465 N Halstead Ave, Pasadena, CA 91107 USA. EM rconan@gmto.org NR 8 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0198-7 J9 PROC SPIE PY 2016 VL 9909 AR UNSP 99091T DI 10.1117/12.2231578 PG 11 WC Optics; Physics, Applied SC Optics; Physics GA BG2JZ UT WOS:000387429700056 ER PT S AU Kopon, D McLeod, B van Dam, MA Bouchez, A McCracken, K Catropa, D Podgorski, W McMuldroch, S Conder, A Close, L Males, J Morzinski, K Norton, T AF Kopon, Derek McLeod, Brian van Dam, Marcos A. Bouchez, Antonin McCracken, Ken Catropa, Daniel Podgorski, William McMuldroch, Stuart Conder, Alan Close, Laird Males, Jared Morzinski, Katie Norton, Timothy BE Marchetti, E Close, LM Veran, JP TI On-sky demonstration of the GMT dispersed fringe phasing sensor prototype on the Magellan telescope SO ADAPTIVE OPTICS SYSTEMS V SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Adaptive Optics Systems V CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Active optics; adaptive optics; Giant Magellan Telescope; phasing; dispersed fringe sensor AB The GMT is an aplanatic Gregorian telescope consisting of 7 primary and secondary mirror segments that must be phased to within a fraction of an imaging wavelength to allow the 25.4 meter telescope to reach its diffraction limit. When operating in Laser Tomographic Adaptive Optics (LTAO) mode, on-axis guide stars will not be available for segment phasing. In this mode, the GMT's Acquisition, Guiding, and Wavefront Sensing system (AGWS) will deploy four pickoff probes to acquire natural guide stars in a 6-10 arcmin annular FOV for guiding, active optics, and segment phasing. The phasing sensor will be able to measure piston phase differences between the seven primary/secondary pairs of up to 50 microns with an accuracy of 50 nm using a J-band dispersed fringe sensor. To test the dispersed fringe sensor design and validate the performance models, SAO has built and commissioned a prototype phasing sensor on the Magellan Clay 6.5 meter telescope. This prototype uses an aperture mask to overlay 6 GMT-sized segment gap patterns on the Magellan 6.5 meter primary mirror reimaged pupil. The six diffraction patterns created by these subaperture pairs are then imaged with a lenslet array and dispersed with a grism. An on-board phase shifter has the ability to simulate an arbitrary phase shift within subaperture pairs. The prototype operates both on-axis and 6 arcmin off-axis either with AO correction from the Magellan adaptive secondary MagAO system on or off in order to replicate as closely as possible the conditions expected at the GMT. C1 [Kopon, Derek; McLeod, Brian; McCracken, Ken; Catropa, Daniel; Podgorski, William; McMuldroch, Stuart; Norton, Timothy] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [van Dam, Marcos A.] Flat Wavefronts, 21 Lascelles St, Christchurch 8022, New Zealand. [Bouchez, Antonin; Conder, Alan] GMTO Corp, 251 S Lake Ave,Suite 300, Pasadena, CA 91101 USA. [Close, Laird; Males, Jared; Morzinski, Katie] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA. RP Kopon, D (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM derek.kopon@cfa.harvard.edu NR 14 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0198-7 J9 PROC SPIE PY 2016 VL 9909 AR UNSP 990946 DI 10.1117/12.2232942 PG 11 WC Optics; Physics, Applied SC Optics; Physics GA BG2JZ UT WOS:000387429700121 ER PT J AU Lin, HW Chen, YT Holman, MJ Ip, WH Payne, MJ Lacerda, P Fraser, WC Gerdes, DW Bieryla, A Sie, ZF Chen, WP Burgett, WS Denneau, L Jedicke, R Kaiser, N Magnier, EA Tonry, JL Wainscoat, RJ Waters, C AF Lin, Hsing Wen Chen, Ying-Tung Holman, Matthew J. Ip, Wing-Huen Payne, M. J. Lacerda, P. Fraser, W. C. Gerdes, D. W. Bieryla, A. Sie, Z. -F. Chen, W. -P. Burgett, W. S. Denneau, L. Jedicke, R. Kaiser, N. Magnier, E. A. Tonry, J. L. Wainscoat, R. J. Waters, C. TI THE PAN-STARRS 1 DISCOVERIES OF FIVE NEW NEPTUNE TROJANS SO ASTRONOMICAL JOURNAL LA English DT Article DE Kuiper belt: general; minor planets, asteroids: general; surveys ID KUIPER-BELT OBJECTS; DARK ENERGY SURVEY; SOLAR-SYSTEM; SIZE DISTRIBUTION; PLANET MIGRATION; CHAOTIC CAPTURE; 2001 QR322; INCLINATION; SEARCH; ORIGIN AB In this work, we report the detection of seven Neptune Trojans (NTs) in the Pan-STARRS 1 (PS1) survey. Five of these are new discoveries, consisting of four L4 Trojans and one L5 Trojan. Our orbital simulations show that the L5 Trojan stably librates for only several million years. This suggests that the L5 Trojan must be of recent capture origin. On the other hand, all four new L4 Trojans stably occupy the 1: 1 resonance with Neptune for more than 1 Gyr. They can, therefore, be of primordial origin. Our survey simulation results show that the inclination width of the NT population should be between 7 degrees and 27 degrees at > 95% confidence, and most likely similar to 11 degrees. In this paper, we describe the PS1 survey, the Outer Solar System pipeline, the confirming observations, and the orbital/physical properties of the new NTs. C1 [Lin, Hsing Wen; Ip, Wing-Huen; Sie, Z. -F.; Chen, W. -P.] Natl Cent Univ, Inst Astron, Taoyuan 32001, Taiwan. [Chen, Ying-Tung] Acad Sinica, Inst Astron & Astrophys, POB 23-141, Taipei 106, Taiwan. [Holman, Matthew J.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Holman, Matthew J.; Payne, M. J.; Bieryla, A.] Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Ip, Wing-Huen] Macau Univ Sci & Technol, Space Sci Inst, Macau, Peoples R China. [Lacerda, P.; Fraser, W. C.] Queens Univ Belfast, Astrophys Res Ctr, Belfast BT7 1NN, Antrim, North Ireland. [Gerdes, D. W.] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Burgett, W. S.; Denneau, L.; Jedicke, R.; Kaiser, N.; Magnier, E. A.; Tonry, J. L.; Wainscoat, R. J.; Waters, C.] Univ Hawaii Manoa, Inst Astron, Honolulu, HI 96822 USA. RP Lin, HW (reprint author), Natl Cent Univ, Inst Astron, Taoyuan 32001, Taiwan. EM edlin@gm.astro.ncu.edu.tw OI Lin, Hsing Wen/0000-0001-7737-6784; Gerdes, David/0000-0001-6942-2736 FU MOST [MOST 104-2119-008-024, MOST 105-2112-M-008-024-MY3]; MOE under the Aim for Top University Program NCU; Macau Technical Fund [017/2014/A1, 039/2013/A2]; CAS Fellowship for Taiwan-Youth-Visiting-Scholars [2015TW2JB0001]; National Aeronautics and Space Administration [NNX08AR22G]; National Science Foundation [AST-1238877] FX This work was supported in part by MOST Grant MOST 104-2119-008-024 (TANGO II), MOST Grant MOST 105-2112-M-008-024-MY3, MOE under the Aim for Top University Program NCU, and the Macau Technical Fund: 017/2014/A1 and 039/2013/A2. H.W.L. acknowledges the support of the CAS Fellowship for Taiwan-Youth-Visiting-Scholars under grant no. 2015TW2JB0001.; The Pan-STARRS 1 Surveys (PS1) have been made possible through contributions from the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, Johns Hopkins University, Durham University, the University of Edinburgh, Queen's University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under grant no. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under grant no. AST-1238877, and the University of Maryland. NR 39 TC 0 Z9 0 U1 1 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-6256 EI 1538-3881 J9 ASTRON J JI Astron. J. PY 2016 VL 152 IS 6 AR 147 DI 10.3847/0004-6256/152/5/147 PG 8 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA EB7HJ UT WOS:000387557200001 ER PT J AU Breedy, O Guzman, HM AF Breedy, Odalisca Guzman, Hector M. TI A new Muricea species (Cnidaria, Anthozoa, Octocorallia) from the eastern tropical Pacific SO ZOOKEYS LA English DT Article DE Alcyonacea; Cnidaria; eastern Pacific; mesophotic zone; Muricea subtilis; new species; plexaurid; soft corals; taxonomy AB The genus Muricea is considered abundant and widely distributed along the eastern Pacific. Its occurrence in shallow waters has been recognised; however species from deeper than 30 m have been rarely recorded. During the 2005 R/V Urraca expedition along the north and central Pacific coast of Costa Rica several octo-coral specimens were collected by bottom trawling from 30 to 150 m yielding new species and new records. Herein we describe a new species of Muricea from deeper than 30 m. The morphological characters of the species were analysed and illustrated by optic and scanning electron microscopy. Muricea subtilis sp. n. can be distinguished from the other species in the genus by its thin spiny branches, non-imbricate calyces, white colony and sclerites, and the size and composition of sclerites. Comparative character tables are provided for the closest Muricea species-group. This new species increases the number in the genus to 26, and contributes to the knowledge on the diversity and distribution of mesophotic soft corals in the eastern Pacific. C1 [Breedy, Odalisca] Univ Costa Rica, Escuela Biol, Ctr Invest Ciencias Mar & Limnol, Ctr Invest Estruct Microscop, POB 11501-2060, San Jose, Costa Rica. [Breedy, Odalisca; Guzman, Hector M.] Smithsonian Trop Res Inst, POB 0843-03092, Panama City, Panama. RP Breedy, O (reprint author), Univ Costa Rica, Escuela Biol, Ctr Invest Ciencias Mar & Limnol, Ctr Invest Estruct Microscop, POB 11501-2060, San Jose, Costa Rica.; Breedy, O (reprint author), Smithsonian Trop Res Inst, POB 0843-03092, Panama City, Panama. EM odaliscab@gmail.com FU Vicerrectoria de Investigacion de la Universidad de Costa Rica [808-B5172]; Smithsonian Tropical Research Institute FX We thank Leen van Ofwegen (Netherlands Centre for Biodiversity Naturalis), Stephen Cairns (Museum of Natural History, Smithsonian Institution) and Gary Williams (California Academy of Science) for their time and suggestions to improve this publication. Also, Yolanda Camacho and Rita Vargas (UCR) for collecting the material for this study and the Smithsonian Tropical Research Institute researchers Rachel Collins and Ross Robertson who were in charge of the R/V Urraca-STRI 2005 expedition. We appreciate Jorge Ceballos (Smithsonian Tropical Research Institute), Alexander Rodriguez and Cristian Mora (UCR) for their valuable contribution in this research. Finally, we acknowledge Jorge Brenes and Annette Calvo-Shadid (UCR) who kindly helped us with the species etymology. The project was partially sponsored by the Vicerrectoria de Investigacion de la Universidad de Costa Rica, project 808-B5172, and the Smithsonian Tropical Research Institute. NR 37 TC 0 Z9 0 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 629 BP 1 EP 10 DI 10.3897/zookeys.629.10828 PG 10 WC Zoology SC Zoology GA EB7PD UT WOS:000387580000001 ER PT J AU Costa, DNR Mathis, WN Marinoni, L AF Costa, Daniel N. R. Mathis, Wayne N. Marinoni, Luciane TI A revision of the shore-fly genus Lamproclasiopa Hendel (Diptera, Ephydridae) SO ZOOKEYS LA English DT Article DE Diptera; Ephydridae; New World tropics; Indian Subcontinent; taxonomic changes; Lamproclasiopa AB The species of the genus Lamproclasiopa Hendel are revised, including 13 new species (type locality in parenthesis): L. aliceae (United States. New Mexico. Grant: Silver City (Big Ditch; 32 degrees 46.4'N, 108 degrees 16.5'W; 1790 m)), L. argentipicta (Costa Rica. San Jose. Zurqui de Moravia (10 degrees 2.8'N, 84 degrees 0.6'W)), L. auritunica (Bolivia. Oruro: Pazna (S. of the town; 18 degrees 36.2'S, 66 degrees 54.7'W, 3750 m).), L. brunnea (Costa Rica. San Jose. Zurqu de Moravia (10 degrees 2.8'N, 84 degrees 0.6'W)), L. caligosa (Chile. Osorno: Anticura (1 km W; 40 degrees 39'S, 72 degrees 10'W; 430 m)), L. curva (Chile. Los Lagos: Chiloe Island, Chepu (on seashore; 42 degrees 5'S, 73 degrees 59.65'W)), L. ecuadoriensis (Ecuador. Orellana: Rio Tiputini Biodiversity Station (0 degrees 38.2'S, 76 degrees 8.9'W)), L. furvitibia (Costa Rica. San Jose. Zurqu de Moravia (10 degrees 2.8'N, 84 degrees 0.6'W)), L. lapaz (Bolivia. La Paz: La Paz (6 km NE; 16 degrees 25.7'S, 68 degrees 04.3'W; 4130m)), L. mancha (Brazil. Parana: Curitiba, Universidade Federal do Parana, Reserva Biologica (25 degrees 26.9'S, 49 degrees 14'W; 915 m)), L. triangularis (Peru. Madre de Dios: Rio Manu, Pakitza (11 degrees 56.6'S, 71 degrees 16.9'W; 250 m)), L. xanthocera (Brazil. Parana. Curitiba, Universidade Federal do Parana, Reserva Biologica (25 degrees 26.9'S, 49 degrees 14'W; 915 m)), L. zerafael (Brazil. Amazonas: Reserva Ducke (02 degrees 55.8'S, 59 degrees 58.5'W; 40 m)). All known species are described with an emphasis on structures of the male terminalia, which are fully illustrated. Detailed locality data and distribution maps for all species are provided. For perspective and to facilitate genus-group and species-group recognition, the tribe Discocerinini is diagnosed and a key to genera in the New World is provided. C1 [Costa, Daniel N. R.; Marinoni, Luciane] Univ Fed Parana, Dept Zool, BR-81531980 Curitiba, Parana, Brazil. [Mathis, Wayne N.] Smithsonian Inst, Dept Entomol, POB 37012,MRC 169, Washington, DC 20013 USA. RP Costa, DNR (reprint author), Univ Fed Parana, Dept Zool, BR-81531980 Curitiba, Parana, Brazil. EM negosekidan@ufpr.br RI Marinoni, Luciane /C-5720-2013 FU CNPq, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico - Brazil [234167/2014-9]; CAPES (Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brazil); CNPq [401609/2009-0]; U.S. National Science Foundation [DEB 1145890] FX We thank the curators and collections managers who loaned collections or facilitated work in their museums: David A. Grimaldi (AMNH), Jon K. Gelhaus and Jason D. Weintraub (ANSP), Jose Albertino Rafael and Rosaly Ale-Rocha (INPA), and Carlos Jose Einicker Lamas (MZUSP). This study was supported by grants from CNPq, Conselho Nacional de Desenvolvimento Cientifico e Tecnologico - Brazil (Process number 234167/2014-9) and CAPES (Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brazil), including a recent field work in Brazil (December 2009-June 2010) that resulted in the vast majority of specimens from Brazil that were studied in this paper (CNPq, Visiting Researcher/Process number 401609/2009-0), which we gratefully acknowledge. The ZADBI project was funded by U.S. National Science Foundation grant DEB 1145890 to B. Brown and A. Borkent. We thank Dianne Mathis for helping with all aspects of the production of this paper, especially the field work in Brazil. We also thank A. Bernardo Carvalho and his lab (Elisa Carvalho, Monica Carvalho, Susana Vaz) for hosting us while conducting field work along the coast of Sao Paulo, and Jose Albertino Rafael and Rosaly Ale-Rocha (INPA) for hosting us while working at INPA and conducting field work in the general environs of Manaus. NR 37 TC 0 Z9 0 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 631 SI SI BP 1 EP 99 DI 10.3897/zookeys.631.10718 PG 99 WC Zoology SC Zoology GA EB7PQ UT WOS:000387581600001 PM 27917044 ER PT J AU van Nieukerken, EJ Doorenweerd, C Hoare, RJB Davis, DR AF van Nieukerken, Erik J. Doorenweerd, Camiel Hoare, Robert J. B. Davis, Donald R. TI Revised classification and catalogue of global Nepticulidae and Opostegidae (Lepidoptera, Nepticuloidea) SO ZOOKEYS LA English DT Article DE Taxonomy; leaf miners; checklist; history; new synonyms; new combinations ID ACADEMY-OF-SCIENCES; LEAF-MINING MOTHS; FAMILY NEPTICULIDAE; SPECIES-GROUP; HOST-PLANT; MINERS LEPIDOPTERA; EUROPE LEPIDOPTERA; SOUTH-AMERICA; 1ST DISCOVERY; GENUS AB A catalogue of all named Nepticulidae and Opostegidae is presented, including fossil species. The catalogue is simultaneously published online in the scratchpad http://nepticuloidea.info/ and in Catalogue of Life (http://www.catalogueoflife.org/col/details/database/id/172). We provide a historical overview of taxonomic research on Nepticuloidea and a brief 'state of the art'. A DNA barcode dataset with 3205 barcodes is made public at the same time, providing DNA barcodes of ca. 779 species, of which 2563 are identified as belonging to 444 validly published species. We recognise 862 extant and 18 fossil species of Nepticulidae in 22 extant genera and the fossil form genus Stigmellites. We count 192 valid Opostegidae species in 7 genera, without fossils. We also list seven dubious Nepticulidae names that cannot be placed due to absent type material and poor descriptions, 18 unavailable names in Nepticulidae that cannot be placed and we also list the 33 names (including four fossils) that once were placed as Nepticulidae or Opostegidae but are now excluded. All synonyms and previous combinations are listed. The generic classification follows the Molecular phylogeny that is published almost simultaneously. Subfamilies and tribes are not recognised, Trifurculinae Scoble, 1983 is synonymised with Nepticulidae Stainton, 1854 and Opostegoidinae Kozlov, 1987 is synonymised with Opostegidae Meyrick, 1893. The status of Casanovula Hoare, 2013, Etainia Beirne, 1945, Fomoria Beirne, 1945, Glaucolepis Braun, 1917, Menurella Hoare, 2013, Muhabbetana Kocak & Kemal, 2007 and Zimmermannia Hering, 1940 is changed from subgenus to full genus, whereas two genera are considered synonyms again: Manoneura Davis, 1979, a synonym of Enteucha Meyrick, 1915 and Levarchama Beirne, 1945, a synonym of Trifurcula Zeller, 1848. We propose 87 new combinations in Nepticulidae and 10 in Opostegidae, largely due to the new classification, and re-examination of some species. We propose the following 37 new synonymies for species (35 in Nepticulidae, 2 in Opostegidae): Stigmella acerifoliella Dovnar-Zapolski, 1969 (unavailable, = S. acerna Puplesis, 1988), Stigmella nakamurai Kemperman & Wilkinson, 1985 (= S. palionisi Puplesis, 1984), Nepticula amseli Skala, 1941 (unavailable = S. birgittae Gustafsson, 1985), Stigmella cathepostis Kemperman & Wilkinson, 1985 (= S. microtheriella (Stainton, 1854)), Stigmella populnea Kemperman & Wilkinson, 1985 (= S. nivenburgensis (Preissecker, 1942)), Nepticula obscurella Braun, 1912 (revised synonymy, = S. myricafoliella (Busck, 1900)), Nepticula mandingella Gustafsson, 1972 (= S. wollofella (Gustafsson, 1972)), Stigmella rosaefoliella pectocatena Wilkinson & Scoble, 1979 (= S. centifoliella (Zeller, 1848)), Micropteryx pomivorella Packard, 1870 (= S. oxyacanthella (Stainton, 1854)), Stigmella crataegivora Puplesis, 1985 (= S. micromelis Puplesis, 1985), Stigmella scinanella Wilkinson & Scoble, 1979 (= S. purpuratella (Braun, 1917)), Stigmella palmatae Puplesis, 1984 (= S. filipendulae (Wocke, 1871)), Stigmella sesplicata Kemperman & Wilkinson, 1985 (= S. lediella (Schleich, 1867)), Stigmella rhododendrifolia Dovnar-Zapolski & Tomilova, 1978 (unavailable, = S. lediella (Schleich, 1867)), Stigmella oa Kemperman & Wilkinson, 1985 (= S. spiculifera Kemperman & Wilkinson, 1985), Stigmella gracilipae Hirano, 2014 (= S. monticulella Puplesis, 1984), Nepticula chaoniella Herrich-Schaffer, 1863 (= S. samiatella (Zeller, 1839)), Bohemannia piotra Puplesis, 1984 (= B. pulverosella (Stainton, 1849)), Bohemannia nipponicella Hirano, 2010 (= B. manschurella Puplesis, 1984), Sinopticula sinica Yang, 1989 (= Glaucolepis oishiella (Matsumura, 1931)), Trifurcula collinella Nel, 2012 (= Glaucolepis magna (A. Lastuvka & Z. Lastuvka, 1997)), Obrussa tigrinella Puplesis, 1985 (= Etainia trifasciata (Matsumura, 1931)), Microcalyptris vittatus Puplesis, 1984 and M. arenosus Falkovitsh, 1986 (both = Acalyptris falkovitshi (Puplesis, 1984)), Ectoedemia castaneae Busck, 1913, E. heinrichi Busck, 1914 and E. helenella Wilkinson, 1981 (all three = Zimmermannia bosquella (Chambers, 1878)), Ectoedemia chloranthis Meyrick, 1928 and E. acanthella Wilkinson & Newton, 1981 (both = Zimmermannia grandisella (Chambers, 1880)), Ectoedemia coruscella Wilkinson, 1981 (= Zimmermannia mesoloba (Davis, 1978)), Ectoedemia piperella Wilkinson & Newton, 1981 and E. reneella Wilkinson, 1981 (both = Zimmermannia obrutella (Zeller, 1873)), Ectoedemia similigena Puplesis, 1994 (= E. turbidella (Zeller, 1848)), Ectoedemia andrella Wilkinson, 1981 (= E. ulmella (Braun, 1912)), Nepticula canadensis Braun, 1917 (= E. minimella (Zetterstedt, 1839)), Opostega rezniki Kozlov, 1985 (= O. cretatella Chretien, 1915), Pseudopostega cyrneochalcopepla Nel & Varenne, 2012 (= P. chalcopepla (Walsingham, 1908)). Stigmella caryaefoliella (Clemens, 1861) and Zimmermannia bosquella (Chambers, 1878) are taken out of synonymy and re-instated as full species. Lectotypes are designated for Trifurcula obrutella Zeller, 1873 and Nepticula grandisella Chambers, 1880. C1 [van Nieukerken, Erik J.; Doorenweerd, Camiel] Naturalis Biodivers Ctr, POB 9517, NL-2300 RA Leiden, Netherlands. [Hoare, Robert J. B.] Landcare Res Ltd, Private Bag 92-170, Auckland, New Zealand. [Davis, Donald R.] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, MRC 105,POB 37012, Washington, DC 20013 USA. RP van Nieukerken, EJ (reprint author), Naturalis Biodivers Ctr, POB 9517, NL-2300 RA Leiden, Netherlands. EM nieukerken@naturalis.nl NR 723 TC 1 Z9 1 U1 5 U2 5 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 628 BP 65 EP 246 DI 10.3897/zookeys.628.9799 PG 182 WC Zoology SC Zoology GA EA2MK UT WOS:000386426900002 PM 27917038 ER PT S AU Babb, JF Hussein, MS AF Babb, James F. Hussein, Mahir S. BE Elster, C Phillips, DR Roberts, CD TI van der Weals and Casimir-Polder interactions between neutrons SO 21ST INTERNATIONAL CONFERENCE ON FEW-BODY PROBLEMS IN PHYSICS SE EPJ Web of Conferences LA English DT Proceedings Paper CT 21st International Conference on Few-Body Problems in Physics (FB21) CY MAY 18-22, 2015 CL Chicago, IL SP Ohio Univ, Argonne Natl Lab ID ENERGY COMPTON-SCATTERING; ELECTROMAGNETIC POLARIZABILITIES; NUCLEON AB We investigate the van der Waals interaction between neutrons using the theory of Casimir and Polder, wherein the potential for asymptotically large separations falls off as the inverse seventh power, and compare it to the similar interaction between a neutron and a proton, for which the asymptotic interaction falls off as the inverse fourth power. Modifications of the formalism to extend the validity to smaller separations using dynamic electric and magnetic dipole polarizability data are discussed. C1 [Babb, James F.; Hussein, Mahir S.] Harvard Smithsonian Ctr Astrophys, ITAMP, MS 14,60 Garden St, Cambridge, MA 02138 USA. [Hussein, Mahir S.] Univ Sao Paulo, Inst Estudos Avancados, CP 72012, BR-05508970 Sao Paulo, SP, Brazil. [Hussein, Mahir S.] Univ Sao Paulo, Inst Fis, CP 66318, BR-05314970 Sao Paulo, Brazil. [Hussein, Mahir S.] CTA, Inst Tecnol Aeronaut, Dept Fis, Sao Jose Dos Campos, SP, Brazil. RP Babb, JF (reprint author), Harvard Smithsonian Ctr Astrophys, ITAMP, MS 14,60 Garden St, Cambridge, MA 02138 USA. EM jbabb@cfa.harvard.edu; hussein@if.usp.br NR 13 TC 0 Z9 0 U1 1 U2 1 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 2100-014X J9 EPJ WEB CONF PY 2016 VL 113 AR 08001 DI 10.1051/epjconf/201611308001 PG 2 WC Physics, Nuclear; Physics, Particles & Fields SC Physics GA BG0KL UT WOS:000386310200126 ER PT J AU Ng, K AF Ng, Konrad BE Srikanth, R Song, MH TI Asian American New Media as Literature for the Digital Age SO CAMBRIDGE HISTORY OF ASIAN AMERICAN LITERATURE LA English DT Article; Book Chapter C1 [Ng, Konrad] Smithsonian Inst, Asian Pacific Amer Ctr, Washington, DC 20560 USA. [Ng, Konrad] Univ Hawaii Manoa, Creat Media, Honolulu, HI 96822 USA. RP Ng, K (reprint author), Smithsonian Inst, Asian Pacific Amer Ctr, Washington, DC 20560 USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU CAMBRIDGE UNIV PRESS PI CAMBRIDGE PA THE PITT BUILDING, TRUMPINGTON ST, CAMBRIDGE CB2 1RP, CAMBS, ENGLAND BN 978-1-107-05395-3 PY 2016 BP 551 EP 566 D2 10.1017/CHO9781107284289 PG 16 WC Literature, American SC Literature GA BF9FA UT WOS:000385516100033 ER PT J AU Taylor, PM AF Taylor, Paul Michael TI Smithsonian Naturalist William Louis Abbott's Turkestan Expedition of 1893 and 1894 SO CENTRAL ASIATIC JOURNAL LA English DT Article AB This paper introduces an important body of ethnographic, biological, and unpublished archival materials deriving from a collecting expedition to Turkestan undertaken from April 1893 to November 1894 by American naturalist William Louis Abbott (1860-1936). Beyond summarising the localities he visited in Turkestan, and the current organization and usefulness of his collections for research, the paper attempts to interpret Abbott's unpublished archival correspondence to assess his collecting focus, biases, and purposes, as well as his perspectives on contemporaneous events in Turkestan and in the neighboring Russian-controlled border areas (today's Tajikistan and Kyrgyzstan) into which he also briefly traveled without permission. The results of Abbott's work are having a positive impact on the anthropology, museums, and regional studies right into the 21st century C1 [Taylor, Paul Michael] Smithsonian Inst, Washington, DC 20560 USA. RP Taylor, PM (reprint author), Smithsonian Inst, Washington, DC 20560 USA. NR 22 TC 0 Z9 0 U1 0 U2 0 PU VERLAG OTTO HARRASSOWITZ PI WIESBADEN PA TAUMUSSTR 14,, 65183 WIESBADEN, GERMANY SN 0008-9192 J9 CENT ASIATIC J JI Cent. Asiat. J. PY 2016 VL 59 IS 1-2 BP 255 EP + PG 22 WC Asian Studies SC Asian Studies GA DZ6RI UT WOS:000385989200009 ER PT J AU Krause, GH Winter, K Krause, B Virgo, A AF Krause, G. Heinrich Winter, Klaus Krause, Barbara Virgo, Aurelio TI Protection by light against heat stress in leaves of tropical crassulacean acid metabolism plants containing high acid levels SO FUNCTIONAL PLANT BIOLOGY LA English DT Article DE Agave angustifolia; Clusia rosea; Clusia pratensis; facultative CAM; obligate CAM; tonoplast ID HIGH-TEMPERATURE TOLERANCE; CHLOROPHYLL FLUORESCENCE; FICUS-INSIPIDA; PHOTOSYNTHETIC APPARATUS; THERMAL TOLERANCE; CAM PLANTS; ACCLIMATION; KALANCHOE; OPUNTIA; ALPINE AB Heat tolerance of plants exhibiting crassulacean acid metabolism (CAM) was determined by exposing leaf sections to a range of temperatures both in the dark and the light, followed by measuring chlorophyll a fluorescence (F-v/F-m and F-0) and assessing visible tissue damage. Three CAM species, Clusia rosea Jacq., Clusia pratensis Seem. and Agave angustifolia Haw., were studied. In acidified tissues sampled at the end of the night and exposed to elevated temperatures in the dark, the temperature that caused a 50% decline of F-v/F-m (T-50), was remarkably low (40-43 degrees C in leaves of C. rosea). Conversion of chlorophyll to pheophytin indicated irreversible tissue damage caused by malic acid released from the vacuoles. By contrast, when acidified leaves were illuminated during heat treatments, T-50 was up to 50-51 degrees C. In de-acidified samples taken at the end of the light period, T-50 reached approximate to 54 degrees C, irrespective of whether temperature treatments were done in the dark or light. Acclimation of A. angustifolia to elevated daytime temperatures resulted in a rise of T-50 from approximate to 54 degrees to approximate to 57 degrees C. In the field, high tissue temperatures always occur during sun exposure. Measurements of the heat tolerance of CAM plants that use heat treatments of acidified tissue in the dark do not provide relevant information on heat tolerance in an ecological context. However, in the physiological context, such studies may provide important clues on vacuolar properties during the CAM cycle (i.e. on the temperature relationships of malic acid storage and malic acid release). C1 [Krause, G. Heinrich; Winter, Klaus; Krause, Barbara; Virgo, Aurelio] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Balboa, Ancon, Panama. [Krause, G. Heinrich] Univ Dusseldorf, Inst Plant Biochem, Univ Str 1, D-40225 Dusseldorf, Germany. RP Krause, GH (reprint author), Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Balboa, Ancon, Panama.; Krause, GH (reprint author), Univ Dusseldorf, Inst Plant Biochem, Univ Str 1, D-40225 Dusseldorf, Germany. EM ghkrause@uni-duesseldorf.de FU Smithsonian Tropical Research Institute FX The study was supported by the Smithsonian Tropical Research Institute. We thank Milton Garcia for technical assistance and George Angehr for critically reading a previous version of the manuscript. NR 39 TC 0 Z9 0 U1 1 U2 1 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1445-4408 EI 1445-4416 J9 FUNCT PLANT BIOL JI Funct. Plant Biol. PY 2016 VL 43 IS 11 BP 1061 EP 1069 DI 10.1071/FP16093 PG 9 WC Plant Sciences SC Plant Sciences GA EA1RJ UT WOS:000386369300005 ER PT J AU Ubelaker, DH AF Ubelaker, Douglas H. TI The Dynamic Interface of Bioarchaeology and Forensic Anthropology SO INTERSECCIONES EN ANTROPOLOGIA LA English DT Article DE Bioarchaeology; Forensic Anthropology; Trauma ID RADIOCARBON; SKELETAL; TISSUE; DEATH AB The disciplines of bioarchaeology and forensic anthropology pursue somewhat different goals but they share considerable methodology and basic scientific information. Experience and research in each of these endeavors enhances the practice of the other. The symbiotic and dynamic relationship of these academic areas greatly improves the quality of the applications of each. The shared information impacts in positive ways all areas of both fields, but is especially important in several key components. Within bioarchaeology, information from forensic practice is vital to the proper interpretation of traumatic and other alterations, especially in the assessment of the timing (antemortem, perimortem, postmortem) of the event producing the alteration. Within forensic anthropology, data gleaned from the practice of bioarchaeology augment techniques of detection, recovery and assessment of the postmortem interval and taphonomic factors that may be involved. Currently, both fields are experiencing a surge in professional activity and student interest, as well as a rapid increase in published research, casework and technology. While the volume of available information presents challenges, practitioners in each field need to remain cognizant of professional activity and research results in the other. C1 [Ubelaker, Douglas H.] Smithsonian Inst, Dept Anthropol, 10th & Constitut Ave NW MRC 112, Washington, DC 20013 USA. RP Ubelaker, DH (reprint author), Smithsonian Inst, Dept Anthropol, 10th & Constitut Ave NW MRC 112, Washington, DC 20013 USA. EM ubelaked@si.edu NR 28 TC 0 Z9 0 U1 0 U2 0 PU UNIV NAC CENTRO PROVINCIA BUENOS AIRES PI BUENOS AIRES PA FAC CIENCIAS SOCIALES, AVE ARISTOBULO DEL VALLE 5737, BUENOS AIRES, OLAVARIA 7400, ARGENTINA SN 1850-373X J9 INTERSECCIONES ANTRO JI Intersecciones Antropol. PY 2016 VL 17 IS 2 BP 137 EP 143 PG 7 WC Anthropology; Archaeology SC Anthropology; Archaeology GA EA1GX UT WOS:000386341600001 ER PT J AU Mawdsley, J Harrison, J Sithole, H AF Mawdsley, Jonathan Harrison, James Sithole, Hendrik TI Natural history of a South African insect pollinator assemblage (Insecta: Coleoptera, Diptera, Hymenoptera, Lepidoptera): diagnostic notes, food web analysis and conservation recommendations SO JOURNAL OF NATURAL HISTORY LA English DT Article DE Pollination; pollinator; insect; Savannah; Africa; tree; shrub ID KRUGER-NATIONAL-PARK; ACACIA-NIGRESCENS; SCARABAEIDAE; SAVANNA; POLLEN; BEES AB We describe activity patterns, relative abundances and pollen transport by insect floral visitors in the Skukuza Ranger District, Kruger National Park, Republic of South Africa, based on field surveys conducted during the early rainy seasons of years 2006 to 2012 (inclusive). Diagnostic notes, illustrations and natural history observations are provided for species in the families Buprestidae, Cerambycidae, Cleridae, Lycidae and Scarabaeidae (Coleoptera), Muscidae, Platystomatidae and Tabanidae (Diptera), Apidae, Halictidae, Megachilidae, Sphecidae and Vespidae (Hymenoptera), and Pieridae and Thyrididae (Lepidoptera) that transported pollen of tree or shrub species. Observations on floral phenology and pollination syndrome are presented for 27 flowering tree or shrub species. To provide a foundation for studies of the effects of drought and climate change on pollination services in the Kruger National Park, we applied methods of food web analysis to characterise this plant-pollinator assemblage. The food web analysis shows moderate levels of redundancy in plant-pollinator interactions (with connectance values averaging 0.19 for plant species and 0.20 for pollinator species), suggesting that pollination services in this system may exhibit some resilience to environmental perturbations. Possible conservation strategies for maintaining pollination services in this ecological system are discussed, including habitat management to conserve larval or nesting areas for social and solitary bees and scarab beetles, as well as further inventories and long-term monitoring of pollinator species. C1 [Mawdsley, Jonathan] Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, MRC 187, NHB 169, Washington, DC 20560 USA. [Harrison, James] Univ Witwatersrand, Sch Anim Plant & Environm Sci, Johannesburg, South Africa. [Harrison, James] Ditsong Natl Museum Nat Hist, Dept Entomol, Pretoria, South Africa. [Sithole, Hendrik] South African Natl Pk, Sci Serv Dept, Invertebrates, Kimberley, South Africa. RP Mawdsley, J (reprint author), Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, MRC 187, NHB 169, Washington, DC 20560 USA. EM MawdsleyJ@si.edu FU Ditsong: National Museum of Natural History; University of the Witwatersrand FX We gratefully acknowledge F. Venter and the South African National Parks (SANParks) for granting permission to conduct this study in the Kruger National Park. For assistance with fieldwork, we thank R. and A. Mawdsley from Cleveland State University and J. Mawdsley from Stark State University, as well as V. Ndlovu, O. Sithole, J. Baloyi, M. Mambane, M. Sarela, P. Khoza, T. Khoza and A. Manganyi from the SANParks. For field and laboratory research support, we thank the Ditsong: National Museum of Natural History (formerly Transvaal Museum) as well as the University of the Witwatersrand. We also thank G. Zambatis from SANParks for her assistance with plant identifications. For providing us with photographic assistance and the images of specimens of Cetoniinae, we thank A. P. Marias. For access to museum collections for voucher specimen identification, we thank S. Brady and T. Erwin of the National Museum of Natural History, Smithsonian Institution, and N. Vandenberg and S. Lingafelter of the United States Department of Agriculture Systematic Entomology Laboratory. For editorial comments on earlier drafts of the manuscript, we thank C. Carter, M. Surridge, K. Wallace and three anonymous reviewers whose comments greatly improved the manuscript. In-kind support for this project was provided by the H. John Heinz III Center for Science, Economics and the Environment (USA), by the Transvaal Museum, by the University of the Witwatersrand and by South African National Parks (RSA). NR 39 TC 0 Z9 0 U1 6 U2 6 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OR14 4RN, OXON, ENGLAND SN 0022-2933 EI 1464-5262 J9 J NAT HIST JI J. Nat. Hist. PY 2016 VL 50 IS 45-46 BP 2849 EP 2879 DI 10.1080/00222933.2016.1216194 PG 31 WC Biodiversity Conservation; Ecology SC Biodiversity & Conservation; Environmental Sciences & Ecology GA EA1DA UT WOS:000386331500004 ER PT S AU McGlynn, T Fabbiano, G Accomazzi, A Smale, A White, RL Donaldson, T Aloisi, A Dower, T Mazzerella, JM Ebert, R Pevunova, O Imel, D Berriman, GB Teplitz, HI Groom, SL Desai, VR Landry, W AF McGlynn, Thomas Fabbiano, Guiseppina Accomazzi, Alberto Smale, Alan White, Richard L. Donaldson, Thomas Aloisi, Alessandra Dower, Theresa Mazzerella, Joseph M. Ebert, Rick Pevunova, Olga Imel, David Berriman, Graham B. Teplitz, Harry I. Groom, Steve L. Desai, Vandana R. Landry, Walter BE Peck, AB Seaman, RL Benn, CR TI Providing comprehensive and consistent access to astronomical observatory archive data: the NASA archive model SO OBSERVATORY OPERATIONS: STRATEGIES, PROCESSES, AND SYSTEMS VI SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Observatory Operations - Strategies, Processes, and Systems VI CY JUN 27-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Virtual observatory; data archives; standards; IVOA; NASA AB Since the turn of the millennium a constant concern of astronomical archives have begun providing data to the public through standardized protocols unifying data from disparate physical sources and wavebands across the electromagnetic spectrum into an astronomical virtual observatory (VO). In October 2014, NASA began support for the NASA Astronomical Virtual Observatories (NAVO) program to coordinate the efforts of NASA astronomy archives in providing data to users through implementation of protocols agreed within the International Virtual Observatory Alliance (IVOA). A major goal of the NAVO collaboration has been to step back from a piecemeal implementation of IVOA standards and define what the appropriate presence for the US and NASA astronomy archives in the VO should be. This includes evaluating what optional capabilities in the standards need to be supported, the specific versions of standards that should be used, and returning feedback to the IVOA, to support modifications as needed. We discuss a standard archive model developed by the NAVO for data archive presence in the virtual observatory built upon a consistent framework of standards defined by the IVOA. Our standard model provides for discovery of resources through the VO registries, access to observation and object data, downloads of image and spectral data and general access to archival datasets. It defines specific protocol versions, minimum capabilities, and all dependencies. The model will evolve as the capabilities of the virtual observatory and needs of the community change. C1 [McGlynn, Thomas; Smale, Alan] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. [Fabbiano, Guiseppina; Accomazzi, Alberto] Smithsonian Astrophys Observ, Cambridge, MA USA. [White, Richard L.; Donaldson, Thomas; Aloisi, Alessandra; Dower, Theresa] Space Telescope Sci Inst, Baltimore, MD 21218 USA. [Mazzerella, Joseph M.; Ebert, Rick; Pevunova, Olga; Imel, David; Berriman, Graham B.; Teplitz, Harry I.; Groom, Steve L.; Desai, Vandana R.; Landry, Walter] Infrared Proc & Anal Ctr, Pasadena, CA USA. [Mazzerella, Joseph M.; Ebert, Rick; Pevunova, Olga; Imel, David; Berriman, Graham B.; Teplitz, Harry I.; Groom, Steve L.; Desai, Vandana R.; Landry, Walter] CALTECH, Pasadena, CA 91125 USA. RP McGlynn, T (reprint author), NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. OI Accomazzi, Alberto/0000-0002-4110-3511 NR 15 TC 0 Z9 0 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0199-4; 978-1-5106-0200-7 J9 PROC SPIE PY 2016 VL 9910 AR 99100A DI 10.1117/12.2231438 PG 11 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PO UT WOS:000385793600009 ER PT S AU Winkelman, S Rots, A AF Winkelman, Sherry Rots, Arnold BE Peck, AB Seaman, RL Benn, CR TI Usefulness and dangers of relying on grant acknowledgments in an observatory bibliography SO OBSERVATORY OPERATIONS: STRATEGIES, PROCESSES, AND SYSTEMS VI SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Observatory Operations - Strategies, Processes, and Systems VI CY JUN 27-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE bibliography; bibliometrics; grant citations; observatory acknowledgments AB The purpose of this paper is to present a quantitative assessment of how well grant and/or program acknowledgments reflect the science impact of Chandra observing, archive, and theory programs and to assess whether observatory acknowledgments alone are a good indicator for inclusion in an observatory bibliography. For grant citations we find that curators will often need to determine the correct grant being cited and they will need to assess relationship between the content of a paper and the grant proposal being cited for statistics to be meaningful. We also find a significant number of papers can be attributed to observing programs through grant links only and that performing full-text searches against the ADS for grant numbers can lead to additional articles for inclusion in the bibliography. When looking at acknowledgment sections as a whole, we find that using an observatory acknowledgment as the sole source for determining inclusion in a bibliography will greatly underestimate the number of science papers attributable to the observatory. C1 [Winkelman, Sherry; Rots, Arnold] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02168 USA. RP Winkelman, S (reprint author), Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02168 USA. EM swinkelman@cfa.harvard.edu NR 3 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0199-4; 978-1-5106-0200-7 J9 PROC SPIE PY 2016 VL 9910 AR 99101W DI 10.1117/12.2231668 PG 8 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PO UT WOS:000385793600061 ER PT S AU Winkelman, S Rots, A AF Winkelman, Sherry Rots, Arnold BE Peck, AB Seaman, RL Benn, CR TI Observatory Bibliographies: A Vital Resource in Operating an Observatory SO OBSERVATORY OPERATIONS: STRATEGIES, PROCESSES, AND SYSTEMS VI SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Observatory Operations - Strategies, Processes, and Systems VI CY JUN 27-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE bibliography; bibliometrics; data archive AB The Chandra Data Archive (CDA) maintains an extensive observatory bibliography. By linking the published articles with the individual datasets analyzed in the paper, we have the opportunity to join the bibliographic metadata (including keywords, subjects, objects, data references from other observatories, etc.) with the meta data associated with the observational datasets. This rich body of information is ripe for far more sophisticated data mining than the two repositories (publications and data) would afford individually. Throughout the course of the mission the CDA has investigated numerous questions regarding the impact of specific types of Chandra programs such as the relative science impact of GTO, GO, and DDT programs or observing, archive, and theory programs. Most recently the Chandra bibliography was used to assess the impact of programs based on the size of the program to examine whether the dividing line between standard and large projects should be changed and whether another round of X-ray Visionary Programs should be offered. Traditionally we have grouped observations by proposal when assessing the impact of programs. For this investigation we aggregated observations by pointing and instrument configuration such that objects observed multiple times in the mission were considered single observing programs. This change in perspective has given us new ideas for assessing the science impact of Chandra and for presenting data to our users. In this paper we present the methodologies used in the recent study, some of its results, and most importantly some unexpected insights into assessing the science impact of an observatory. C1 [Winkelman, Sherry; Rots, Arnold] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02168 USA. RP Winkelman, S (reprint author), Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02168 USA. EM swinkelman@cfa.harvard.edu NR 3 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0199-4; 978-1-5106-0200-7 J9 PROC SPIE PY 2016 VL 9910 AR 991006 DI 10.1117/12.2231730 PG 8 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PO UT WOS:000385793600005 ER PT J AU Castillo-Cardenas, MF Sanjur, O Toro-Perea, N AF Fernanda Castillo-Cardenas, Maria Sanjur, Oris Toro-Perea, Nelson TI Differences in sculpture and size of pollen grains: new morphological evidence of diversification in Pelliciera rhizophorae, an ancient Neotropical mangrove species SO PALYNOLOGY LA English DT Article DE pollen morphology; diversification; exine sculpture; Pelliciera rhizophorae; Neotropics; mangroves ID PALEOBOTANY; COMMUNITIES; EVOLUTION; PANAMA AB The present study shows new evidence of morphological traits that supports the hypothesis of diversification between two genetic variants of Pelliciera rhizophorae (Tetrameristaceae), the most ancient species in the Neotropical mangrove ecosystem. Previous studies using molecular markers identified two variants of this species. Our new study, using pollen grain morphology, revealed differences in pollen sculpture between the two variants; that is, in Variant A the exine is characterised as perforate-verrucose, while in Variant B, it is punctuate. Pollen size in Variant A is larger than in Variant B, whereas the exine is thicker in Variant B than in Variant A. The differences in pollen morphology between the two variants represent new evidence suggesting that a diversification process might be occurring within P. rhizophorae, possibly due to adaptive processes in response to environmental conditions or pollination vectors. C1 [Fernanda Castillo-Cardenas, Maria; Sanjur, Oris] Smithsonian Trop Res Inst, Balboa 084303092, Ancon, Panama. [Fernanda Castillo-Cardenas, Maria; Toro-Perea, Nelson] Univ Valle, Dept Biol, Apartado 25360,Edif 320, Cali, Colombia. RP Castillo-Cardenas, MF (reprint author), Smithsonian Trop Res Inst, Balboa 084303092, Ancon, Panama.; Castillo-Cardenas, MF (reprint author), Univ Valle, Dept Biol, Apartado 25360,Edif 320, Cali, Colombia. EM mfcastillo@gmail.com FU International Foundation for Science (IFS) [D/3832-3] FX We are grateful to the institutions that supported the development of this research: the International Foundation for Science (IFS) for funding this study (grant D/3832-3); logistical support provided by the Universidad del Valle (UNIVALLE) in Colombia, and the Smithsonian Tropical Research Institute (STRI) in Panama. We would also like to thank the STRI scientists who collaborated on this study: biologist Jorge Ceballos (support in SEM and LSCM), and Enrique Moreno (scientific expert in palynology). We are grateful to biologists Alonso Santos and Daniel Buitrago (fieldwork), as well as to Jose Alejandro Ramirez, an undergraduate student (Universidad de Panama), for his support in fieldwork and slide preparation. NR 21 TC 0 Z9 0 U1 2 U2 2 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 0191-6122 EI 1558-9188 J9 PALYNOLOGY JI Palynology PY 2016 VL 40 IS 3 BP 302 EP 307 DI 10.1080/01916122.2015.1045050 PG 6 WC Plant Sciences; Paleontology SC Plant Sciences; Paleontology GA DZ7LN UT WOS:000386047200004 ER PT J AU Duan, L Yang, X Liu, PL Johnson, G Wen, J Chang, ZY AF Duan, Lei Yang, Xue Liu, Peiliang Johnson, Gabriel Wen, Jun Chang, Zhaoyang TI A molecular phylogeny of Caraganeae (Leguminosae, Papilionoideae) reveals insights into new generic and infrageneric delimitations SO PHYTOKEYS LA English DT Article DE Caragana; Chesneya; Chesniella; chloroplast capture; generic delimitation; phylogeny ID REVISION AB Based on sequence data of nuclear ITS and plastid matK, trnL-F and psbA-trnH markers, the phylogeny of the subtribes Caraganinae and Chesneyinae in tribe Caraganeae was inferred. The results support the monophyly of each of the subtribes. Within subtribes Caraganinae, Calophaca and Halimodendron are herein transferred into Caragana to ensure its generic monophyly. The subtribe Chesneyinae is composed of four well-supported genera: Chesneya, Chesniella, Gueldenstaedtia and Tibetia. Based on phylogenetic, morphological, distributional and habitat type evidence, the genus Chesneya was divided into three monophyletic sections: C. sect. Chesneya, C. sect. Pulvinatae and C. sect. Spinosae. Chesneya macrantha is herein transferred into Chesniella. Spongiocarpella is polyphyletic and its generic rank is not maintained. The position of Chesneya was incongruent in the nuclear ITS and the plastid trees. A paternal chloroplast capture event via introgression is hypothesized for the origin of Chesneya, which is postulated to have involved the common ancestor of Chesniella (male) and that of the Gueldenstaedtia - Tibetia (GUT) clade (female) as the parents. C1 [Duan, Lei] Chinese Acad Sci, Key Lab Plant Resources Conservat & Sustainable U, South China Bot Garden, Guangzhou 510650, Guangdong, Peoples R China. [Yang, Xue] Kunming Univ, Sch Agr, Kunming 650204, Yunnan, Peoples R China. [Liu, Peiliang; Chang, Zhaoyang] Northwest A&F Univ, Coll Life Sci, Yangling 712100, Shaanxi, Peoples R China. [Johnson, Gabriel; Wen, Jun] Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, MRC 166, Washington, DC 20013 USA. RP Chang, ZY (reprint author), Northwest A&F Univ, Coll Life Sci, Yangling 712100, Shaanxi, Peoples R China.; Wen, J (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, MRC 166, Washington, DC 20013 USA. EM wenj@si.edu; czybbg@nwsuaf.edu.cn FU Laboratories of Analytical Biology of the National Museum of Natural History (Smithsonian Institution); Natural Science Foundation of China [30270106, 30870155]; China Scholarship Council FX We are grateful to the curators of the following herbaria for providing leaf samples, seeds or DNA samples: CS, F, K, TURP, US, WUK and XJBI. We thank Matthew Kweskin, Mingqin Zhou, and Jianqiang Zhang for lab assistance; Natasha Crump for Russian literature translation; Robin Everly for literature search; and Martin F. Wojciechowski, Ying Feng, Shimin Duan, Irina Illarionova and Roman Ufimov for checking voucher information. The Laboratories of Analytical Biology of the National Museum of Natural History (Smithsonian Institution), the Natural Science Foundation of China (Project no. 30270106, 30870155) and the China Scholarship Council are gratefully acknowledged for financial support of the study. NR 10 TC 1 Z9 1 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 70 BP 111 EP 137 DI 10.3897/phytokeys.70.9641 PG 27 WC Plant Sciences SC Plant Sciences GA EA2MN UT WOS:000386427500008 ER PT J AU Feuillet, C AF Feuillet, Christian TI Lectotypifications of six taxa in the Boraginales (Cordiaceae and Heliotropiaceae) SO PHYTOKEYS LA English DT Article DE Cordia; Cordiaceae; Heliotropiaceae; lectotype; Myriopus; Tournefortia; Varronia ID NAMES; TYPIFICATION AB A large number of specimens used as original material for the description of new species were destroyed in the bombing of the Berlin-Dahlem herbarium, B, in 1943. Six lectotypes are designated here for Cordia discolor Cham., Cordia multispicata Cham., Cordia tobagensis Urb. and its variety broadwayi Urb. in the Cordiaceae and for Tournefortia paniculata Cham. and Tournefortia ulei Vaupel in the Heliotropiaceae. C1 [Feuillet, Christian] Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, MRC 166, POB 37012, Washington, DC 20013 USA. [Feuillet, Christian] Oregon State Univ, Dept Bot & Plant Pathol, 2082 Cordley Hall, Corvallis, OR 97331 USA. RP Feuillet, C (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, MRC 166, POB 37012, Washington, DC 20013 USA.; Feuillet, C (reprint author), Oregon State Univ, Dept Bot & Plant Pathol, 2082 Cordley Hall, Corvallis, OR 97331 USA. EM feuillec@si.edu NR 20 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 62 BP 95 EP 100 DI 10.3897/phytokeys.62.6259 PG 6 WC Plant Sciences SC Plant Sciences GA DZ8RX UT WOS:000386140000002 ER PT J AU Stein, NM van Dyk, DA Kashyap, VL AF Stein, Nathan M. van Dyk, David A. Kashyap, Vinay L. TI Preprocessing solar images while preserving their latent structure SO STATISTICS AND ITS INTERFACE LA English DT Article; Proceedings Paper CT Banff Workshop on Statistical and Computational Theory and Methodology for Big Data Analysis CY FEB 09-14, 2014 CL Banff, CANADA DE Clustering; Decision theory; Dissimilarity measure; Hellinger distance; Image segmentation; Latent structure; Solar physics; Space weather ID EXTREME-ULTRAVIOLET SPECTRA; DENSITY STRUCTURE; QUIET-SUN; DATA SET; PLASMA; SEGMENTATION; TEMPERATURE; DIAGNOSTICS; CALIBRATION; STATISTICS AB Telescopes such as the Atmospheric Imaging Assembly aboard the Solar Dynamics Observatory, a NASA satellite, collect massive streams of high resolution images of the Sun through multiple wavelength filters. Reconstructing pixel-by-pixel thermal properties based on these images can be framed as an ill-posed inverse problem with Poisson noise, but this reconstruction is computationally expensive and there is disagreement among researchers about what regularization or prior assumptions are most appropriate. This article presents an image segmentation framework for preprocessing such images in order to reduce the data volume while preserving as much thermal information as possible for later downstream analyses. The resulting segmented images reflect thermal properties but do not depend on solving the ill-posed inverse problem. This allows users to avoid the Poisson inverse problem altogether or to tackle it on each of similar to 10 segments rather than on each of similar to 10(7) pixels, reducing computing time by a factor of similar to 10(6). We employ a parametric class of dissimilarities that can be expressed as cosine dissimilarity functions or Hellinger distances between non linearly transformed vectors of multi-passband observations in each pixel. We develop a decision theoretic framework for choosing the dissimilarity that minimizes the expected loss that arises when estimating identifiable thermal properties based on segmented images rather than on a pixel-by-pixel basis. We also examine the efficacy of different dissimilarities for recovering clusters in the underlying thermal properties. The expected losses are computed under scientifically motivated prior distributions. Two simulation studies guide our choices of dissimilarity function. We illustrate our method by segmenting images of a coronal hole observed on 26 February 2015. C1 [Stein, Nathan M.] Univ Penn, Dept Stat, Philadelphia, PA 19104 USA. [van Dyk, David A.] Imperial Coll London, Dept Math, Stat Sect, London, England. [Kashyap, Vinay L.] Harvard Smithsonian Ctr Astrophys, Div High Energy Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP van Dyk, DA (reprint author), Imperial Coll London, Dept Math, Stat Sect, London, England. EM natstein@wharton.upenn.edu; dvandyk@imperial.ac.uk; vkashyap@cfa.harvard.edu NR 47 TC 0 Z9 0 U1 1 U2 1 PU INT PRESS BOSTON, INC PI SOMERVILLE PA PO BOX 43502, SOMERVILLE, MA 02143 USA SN 1938-7989 EI 1938-7997 J9 STAT INTERFACE JI Stat. Interface PY 2016 VL 9 IS 4 BP 535 EP 551 PG 17 WC Mathematical & Computational Biology; Mathematics, Interdisciplinary Applications SC Mathematical & Computational Biology; Mathematics GA DZ8FM UT WOS:000386106300013 ER PT J AU Agnarsson, I LeQuier, SM Kuntner, M Cheng, RC Coddington, JA Binford, G AF Agnarsson, Ingi LeQuier, Stephanie M. Kuntner, Matjaz Cheng, Ren-Chung Coddington, Jonathan A. Binford, Greta TI Phylogeography of a good Caribbean disperser: Argiope argentata (Araneae, Araneidae) and a new 'cryptic' species from Cuba SO ZOOKEYS LA English DT Article DE Biogeography; CarBio; dispersal; diversification; GAARlandia; Intermediate dispersal model; Isolation by distance model ID SPIDERS; EVOLUTION; DIVERSIFICATION; BIOGEOGRAPHY; ISLANDS; PHYLOGENETICS; COLONIZATION; SYSTEMATICS; DIMORPHISM; HYPOTHESIS AB The Caribbean islands harbor rich biodiversity with high levels of single island endemism. Stretches of ocean between islands represent significant barriers to gene-flow. Yet some native species are widespread, indicating dispersal across oceans, even in wingless organisms like spiders. Argiope argentata (Fabricius, 1775) is a large, charismatic, and widespread species of orb-weaving spider ranging from the United States to Argentina and is well known to balloon. Here we explore the phylogeography of A. argentata in the Caribbean as a part of the multi-lineage CarBio project, through mtDNA haplotype and multi-locus phylogenetic analyses. The history of the Argiope argentata lineage in the Caribbean goes back 3-5 million years and is characterized by multiple dispersal events and isolation-by-distance. We find a highly genetically distinct lineage on Cuba which we describe as Argiope butchko sp. n. While the argentata lineage seems to readily balloon shorter distances, stretches of ocean still act as filters for among-island gene-flow as evidenced by distinct haplotypes on the more isolated islands, high FST values, and strong correlation between intraspecific (but not interspecific) genetic and geographic distances. The new species described here is clearly genetically diagnosable, but morphologically cryptic, at least with reference to the genitalia that typically diagnose spider species. Our results are consistent with the intermediate dispersal model suggesting that good dispersers, such as our study species, limit the effect of oceanic barriers and thus diversification and endemism. C1 [Agnarsson, Ingi; LeQuier, Stephanie M.] Univ Vermont, Dept Biol, Burlington, VT 05405 USA. [Agnarsson, Ingi; Kuntner, Matjaz; Coddington, Jonathan A.] Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, Washington, DC 20560 USA. [Kuntner, Matjaz; Cheng, Ren-Chung] ZRC SAZU, Inst Biol, Evolutionary Zool Lab, Ljubljana, Slovenia. [Binford, Greta] Lewis & Clark Coll, Dept Biol, Portland, OR 97219 USA. RP Agnarsson, I (reprint author), Univ Vermont, Dept Biol, Burlington, VT 05405 USA.; Agnarsson, I (reprint author), Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, Washington, DC 20560 USA. EM iagnarsson@gmail.com FU NSF [DEB-1050187-1050253-1314749]; Smithsonian Institution SI Barcode Network; Slovenian Research Agency [P1-10236, J1-6729] FX Many thanks to all the members of team CarBio and our collaborators for tireless effort in the field over the last four years. Special thanks to collaborators in Cuba (Alexander Sanchez, Giraldo Alayon, Franklyn Cala-Riquelme and others) and Hispaniola (Solanlly Carrero Jimenez, Gabriel de los Santos) for invaluable help with organization and execution of logistically complex expeditions and ongoing collaboration. We thank Matjaz Gregoric, Klemen Candek, and Gabriele Uhl for kind help with obtaining additional samples. Funding for this work came from NSF DEB-1050187-1050253-1314749 to IA and GB, and the Smithsonian Institution 2013 SI Barcode Network to JC and IA. MK and RCC were supported by the Slovenian Research Agency (grants P1-10236 and J1-6729 to MK). NR 62 TC 0 Z9 0 U1 3 U2 3 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 625 BP 25 EP 44 DI 10.3897/zookeys.625.8729 PG 20 WC Zoology SC Zoology GA DZ7PN UT WOS:000386058400003 PM 27833425 ER PT J AU Boyd, OF Erwin, TL AF Boyd, Olivia F. Erwin, Terry L. TI Taxonomic review of New World Tachyina (Coleoptera, Carabidae): descriptions of new genera, subgenera, and species, with an updated key to the subtribe in the Americas SO ZOOKEYS LA English DT Review DE Elaphropus; Meotachys; Nototachys; Polyderidius; Polyderis; Nothoderis; Stigmatachys; Tachyxysta; Amazon basin ID BEMBIDIINI; ERWIN; BEETLES AB The classification of the carabid subtribe Tachyina (Trechitae: Bembidiini) is reviewed in light of newly discovered diversity from Central and South America. Described herein are three new genera (Tachyxysta gen. n., Stigmatachys gen. n., Nothoderis gen. n.), two new subgenera of Meotachys (Scolistichus subgen. n., Hylotachys subgen. n.), and two new subgenera of Elaphropus (Ammotachys subgen. n., Idiotachys subgen. n.). Two names previously synonymized under Polyderis (Polyderidius Jeannel, 1962) and Elaphropus (Nototachys Alluaud, 1930) are elevated to generic and subgeneric status, respectively. Eight new species are recognized: Tachyxysta howdenorum (type locality: Mexico: Chiapas: El Aguacero, 680m); Elaphropus marchantarius (type locality: Brazil, Amazonas, Rio Solimoes, Ilha de Marchantaria), E. acutifrons (type locality: Brazil: Para, Santarem) and E. occidentalis (type locality: Peru: Loreto, Pithecia, 74 degrees 45'W 05 degrees 28'S); Stigmatachys uvea (type locality: Peru: Loreto: Campamento San Jacinto, 2 degrees 18.75'S, 75 degrees 51.77'W, 175-215m); and Meotachys riparius (type locality: Colombia: Amazonas: Leticia, 700 ft), M. ballorum (type locality: Brazil: Amazonas, Rio Negro Cucui), and M. rubrum (type locality: Peru: Madre de Dios: Rio Manu, Pakitza, 11 degrees 56 degrees 47'S 071 degrees 17 degrees 00'W, 356m). An updated key to the genera and subgenera of Tachyina occurring in the New World is provided, with accompanying illustrations. C1 [Boyd, Olivia F.] Oregon State Univ, Dept Integrat Biol, Corvallis, OR 97331 USA. [Erwin, Terry L.] Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, POB 37012, Washington, DC 20013 USA. RP Boyd, OF (reprint author), Oregon State Univ, Dept Integrat Biol, Corvallis, OR 97331 USA. EM boydo@oregonstate.edu FU Harold E. and Leona M. Rice Endowment Fund at Oregon State University; National Museum of Natural History, Smithsonian Institution, Department of Entomology FX In addition to the individuals mentioned under Material examined above, the authors thank all the collectors and curators who provided specimens for this work: George Ball (UASM), Yves Bousquet (CNC), Warren Steiner (NMNH), Brian Farrell (MCZ), R.C. Graves, and the late Henry Howden, as well as curators Thierry Deuve (MNHN) and Cleide Costa (MZUSP) for loaning critical specimens from the collections of the late J. Negre and Hans Reichardt, respectively. Charyn Micheli provided much support and assistance with the NMNH Tachyina collections during this project, including processing of large loans and acquisition of literature and specimen data. Thanks to D.H. Kavanaugh and G.E. Ball for their comments on the manuscript. We especially thank David Maddison for his many hours of advice and encouragement throughout the project and for his valuable comments on drafts of the manuscript. This work was funded in part from the Harold E. and Leona M. Rice Endowment Fund at Oregon State University, through David Maddison. Funding for article processing charges was provided by the National Museum of Natural History, Smithsonian Institution, Department of Entomology. NR 46 TC 0 Z9 0 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 626 BP 87 EP 123 DI 10.3897/zookeys.626.10033 PG 37 WC Zoology SC Zoology GA DZ7PV UT WOS:000386059200005 PM 27833435 ER PT J AU Frias-Torres, S Goehlich, H Reveret, C Montoya-Maya, PH AF Frias-Torres, S. Goehlich, H. Reveret, C. Montoya-Maya, P. H. TI Reef fishes recruited at midwater coral nurseries consume biofouling and reduce cleaning time in Seychelles, Indian Ocean SO AFRICAN JOURNAL OF MARINE SCIENCE LA English DT Article DE animal-assisted cleaning; coral gardening; coral reef restoration; endangered species; floating ecosystem ID DAMSELFISHES POMACENTRIDAE; RESTORATION; RESILIENCE; ECOSYSTEMS; MANAGEMENT AB In coral reef restoration, coral gardening involves rearing coral fragments in underwater nurseries prior to transplantation. These nurseries become fish-aggregating devices and attract biofouling. We hypothesised that: (1) the presence of corals at a nursery is critical to recruit fish assemblages and (2) the recruited fish assemblages control biofouling, reducing person-hours invested in nursery cleaning. Three midwater coral nurseries were deployed at 8 m depth for 27 months within the marine protected area of Cousin Island Special Reserve, Seychelles, Indian Ocean. Each nursery consisted of a 6 m x 6 m PVC pipe frame, layered with a recycled 5.5-cm-mesh tuna net. Human cleaning effort was calculated based on daily dive logs. Nursery-associated fish assemblages and behaviour were video-recorded prior to harvesting corals after a 20-month growth period and seven months post-coral harvesting. The density (ind. m(-2)) of blue-yellow damselfish Pomacentrus caeruleus was 12-16 times higher when corals were present than when corals were absent at the nurseries. Fish assemblages recruited into the nurseries included three trophic levels, from herbivores to omnivores, in six families: Ephippidae, Pomacentridae, Labridae (Scarinae), Gobiidae, Siganidae and Monacanthidae. Higher abundance of large fish (total number of individuals) resulted in 2.75 times less person-hours spent in nursery cleaning. These results have important implications for cost-effective coral reef restoration. C1 [Frias-Torres, S.; Goehlich, H.; Reveret, C.; Montoya-Maya, P. H.] Isl Conservat Ctr, Nat Seychelles, Amitie, Praslin, Seychelles. [Frias-Torres, S.] Smithsonian Marine Stn, Ft Pierce, FL 34949 USA. [Goehlich, H.] Univ Rostock, Inst Biol Sci, Rostock, Germany. [Reveret, C.] CREOCEAN, La Rochelle, France. RP Frias-Torres, S (reprint author), Isl Conservat Ctr, Nat Seychelles, Amitie, Praslin, Seychelles.; Frias-Torres, S (reprint author), Smithsonian Marine Stn, Ft Pierce, FL 34949 USA. EM sfriastorres@gmail.com FU United States Agency for International Development (USAID) Reef Rescuers Project [674-A-00-10-00123-00] FX We thank K Rowe, M Mullins, D Quinlan and D Soto for help during fieldwork and N Shah for commenting on an earlier draft of the manuscript. Funding to Nature Seychelles was received through the United States Agency for International Development (USAID) Reef Rescuers Project 674-A-00-10-00123-00. NR 22 TC 0 Z9 0 U1 1 U2 1 PU NATL INQUIRY SERVICES CENTRE PTY LTD PI GRAHAMSTOWN PA 19 WORCESTER STREET, PO BOX 377, GRAHAMSTOWN 6140, SOUTH AFRICA SN 1814-232X EI 1814-2338 J9 AFR J MAR SCI JI Afr. J. Mar. Sci. PY 2016 VL 38 IS 3 BP 421 EP 426 DI 10.2989/1814232X.2015.1078259 PG 6 WC Marine & Freshwater Biology SC Marine & Freshwater Biology GA DY8RF UT WOS:000385397200014 ER PT J AU Van Bocxlaer, B Strong, EE AF Van Bocxlaer, Bert Strong, Ellen E. TI Anatomy, functional morphology, evolutionary ecology and systematics of the invasive gastropod Cipangopaludina japonica (Viviparidae: Bellamyinae) SO CONTRIBUTIONS TO ZOOLOGY LA English DT Article DE basal Architaenioglossa; Bellamya; fecundity; geometric morphometrics; histology; reproductive anatomy; sexual dimorphism ID MALLEATUS REEVE GASTROPODA; FRESH-WATER; CAENOGASTROPODA VIVIPARIDAE; CAMPELOMA-RUFUM; NORTH-AMERICA; 3 POPULATIONS; PROSOBRANCHIA; PHYLOGENY; SNAILS; MONTREAL AB The anatomy, functional morphology and evolutionary ecology of the Viviparidae, and the subfamily Bellamyinae in particular, are incompletely known. Partly as a result, genealogical relationships within the family remain poorly understood. Because of this lack in knowledge, few informed hypotheses exist on ancestral states, how differences in body plans between the subfamilies evolved, and how the peculiar biogeographic distribution patterns of viviparids have arisen. Here we document the anatomy, morphology, life history and systematics of Cipango-paludina japonica, a Japanese species that has been introduced into North America, to resolve taxonomic confusion and to improve our understanding of how form and function are related in bellamyines. Anatomical and histological examinations demonstrate marked differences between C. japonica and other bellamyines in the radula, salivary gland, kidney, nerve ring and reproductive organs. Substantial differences also exist between male and female body organization, but conchological differences between sexes in semi-landmark morphometric analyses are limited. The volume of the brood pouch of females, and hence body and shell size, appear to be good predictors of reproductive success, and the species' ecological versatility may relate to high fecundity and the ability to alternate between feeding modes. Comparing our observations on C. japonica with other viviparids and basal Architaenioglossa, we identify several persistent misinterpretations in the literature on how form and function are related in viviparids, not in the least as to female reproductive anatomy. Our reinterpretations improve understanding of the evolution of Viviparidae and its subfamilies, and hopefully will allow future workers to isolate key traits that shaped the evolution of viviparids at the taxonomic levels of their interest for more detailed studies. C1 [Van Bocxlaer, Bert] Leibniz Inst Evolut & Biodivers Sci, Museum Nat Kunde, Invalidenstr 43, D-10115 Berlin, Germany. [Van Bocxlaer, Bert] Univ Giessen, Dept Anim Ecol & Systemat, Heinrich Buff Ring 26-32 IFZ, D-35392 Giessen, Germany. [Van Bocxlaer, Bert; Strong, Ellen E.] Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, POB 37012,MRC 163, Washington, DC 20013 USA. [Van Bocxlaer, Bert] Univ Ghent, Dept Biol, Limnol Unit, KL Ledeganckstr 35, B-9000 Ghent, Belgium. RP Van Bocxlaer, B (reprint author), Leibniz Inst Evolut & Biodivers Sci, Museum Nat Kunde, Invalidenstr 43, D-10115 Berlin, Germany.; Van Bocxlaer, B (reprint author), Univ Giessen, Dept Anim Ecol & Systemat, Heinrich Buff Ring 26-32 IFZ, D-35392 Giessen, Germany.; Van Bocxlaer, B (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, POB 37012,MRC 163, Washington, DC 20013 USA.; Van Bocxlaer, B (reprint author), Univ Ghent, Dept Biol, Limnol Unit, KL Ledeganckstr 35, B-9000 Ghent, Belgium. EM bert.vanbocxlaer@ugent.be FU Peter Buck Fellowship of the Smithsonian Institution; Alexander von Humboldt Fellowship; Fellowship of the Flanders Research Foundation FX We thank two anonymous referees for constructive comments that improved the manuscript significantly; Elizabeth Diamond (USNM) for assistance with histology; Paul Greenhall and Kristen Mercer (USNM) for shipping and cataloguing specimens. BVB was supported by a Peter Buck Fellowship of the Smithsonian Institution, an Alexander von Humboldt Fellowship and a Fellowship of the Flanders Research Foundation. NR 98 TC 0 Z9 0 U1 6 U2 6 PU NATURALIS BIODIVERSITY CENTER PI LEIDEN PA DARWINWEG 2, LEIDEN, 2333 CR, NETHERLANDS SN 1383-4517 EI 1875-9866 J9 CONTRIB ZOOL JI Contrib. Zool. PY 2016 VL 85 IS 2 BP 235 EP 263 PG 29 WC Zoology SC Zoology GA DZ6ZT UT WOS:000386013100002 ER PT S AU McLeod, BA Smith, R AF McLeod, Brian A. Smith, Roger BE Holland, AD Beletic, J TI Mitigation of H2RG persistence with image illumination SO HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY VII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on High Energy, Optical, and Infrared Detectors for Astronomy VII CY JUN 26-29, 2016 CL Edinburgh, SCOTLAND SP SPIE DE infrared detectors; persistence; HAWAII-2RG AB Residual charge generation, or image persistence, in infrared detectors is a problem that affects many low-light astronomical instruments. The HAWAII-2RG in the MMT & Magellan Infrared Spectrograph shows significant persistence when first powered up. We describe here how we reduce the persistence sensitivity of this detector by exposure to light. C1 [McLeod, Brian A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Smith, Roger] CALTECH, Caltech Opt Observ, MC105-24,1200 E Calif Blvd, Pasadena, CA 91125 USA. RP McLeod, BA (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM bmcleod@cfa.harvard.edu NR 6 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0209-0; 978-1-5106-0210-6 J9 PROC SPIE PY 2016 VL 9915 AR UNSP 99150G DI 10.1117/12.2233083 PN 1 PG 7 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PM UT WOS:000385793400014 ER PT S AU Launius, RD AF Launius, Roger D. BE Freeman, M TI The Railroad and the Space Program Revisited: Historical Analogues and the Stimulation of Commercial Space Operations SO HISTORY OF ROCKETRY AND ASTRONAUTICS: PROCEEDINGS OF THE FORTY-EIGHTH HISTORY SYMPOSIUM OF THE INTERNATIONAL ACADEMY OF ASTRONAUTICS, 2014 SE AAS History Series LA English DT Proceedings Paper CT 48th History Symposium of the International Academy of Astronautics CY SEP, 2014 CL Toronto, CANADA AB In 1965 historian Bruce Mazlish edited the NASA-sponsored study, The Railroad and the Space Program: An Exploration in Historical Analogy (MET Press), seeking to understand the historical record of government stimulation of private sector investment in infrastructure for the public good. The study team explored several specific episodes of American railroad history. It took as its mission: "In all of these studies an effort will be made to move from the impact of the railroad in the specific area under consideration to an analogy with the possible space impact today in similar areas." While the result was disappointing at the time there remain lessons to be gained in exploring the historical analogue of railroad building and operation in the nineteenth century and their application to an expansion of space exploitation. While many are familiar with the enticing of American transcontinental railroad construction through land grants, national, state, and local governments had engaged in a range of other stimulative efforts to facilitate railroad development. These included tax breaks, investment credits, and otherwise favorable decisions supporting these business interests. It also involved, in some instances, direct subsidies for a time, monopolies not only on railroad operations but also in ancillary and even tertiary industries, and changes to regulations to ease requirements for labor, safety, and other factors. This chapter revisits this analogue, drawing several key findings from the railroad experience. It suggests that there is a broad range of options that have been pursued in the past to stimulate investment in infrastructure in this case in railroads-that have application for future space operations. Not all of these options were successful some failed outright and others had detrimental unintended consequences and that will be discussed as well. C1 [Launius, Roger D.] Smithsonian Inst, Natl Air & Space Museum, Washington, DC 20560 USA. RP Launius, RD (reprint author), Smithsonian Inst, Natl Air & Space Museum, Washington, DC 20560 USA. NR 33 TC 0 Z9 0 U1 0 U2 0 PU AMER ASTRONAUTICAL SOC PI SAN DIEGO PA PUBLICATIONS OFFICE PO BOX 28130, SAN DIEGO, CA 92128 USA SN 0730-3564 BN 978-0-87703-628-9; 978-0-87703-627-2 J9 AAS HIST SER PY 2016 VL 46 BP 189 EP 205 PG 17 WC Engineering, Aerospace; History & Philosophy Of Science SC Engineering; History & Philosophy of Science GA BF8ZF UT WOS:000385321800010 ER PT J AU Tiiman, A Luo, JH Wallin, C Olsson, L Lindgren, J Jarvet, J Roose, P Sholts, SB Rahimipour, S Abrahams, JP Karlstrom, AE Graslund, A Warmlander, SKTS AF Tiiman, Ann Luo, Jinghui Wallin, Cecilia Olsson, Lisa Lindgren, Joel Jarvet, Juri Roose, Per Sholts, Sabrina B. Rahimipour, Shai Abrahams, Jan Pieter Karlstrom, Amelie Eriksson Graslund, Astrid Warmlander, Sebastian K. T. S. TI Specific Binding of Cu(II) Ions to Amyloid-Beta Peptides Bound to Aggregation-Inhibiting Molecules or SDS Micelles Creates Complexes that Generate Radical Oxygen Species SO JOURNAL OF ALZHEIMERS DISEASE LA English DT Article DE Alzheimer's disease; copper-binding protein; hydrogen peroxide; membrane chemistry; neurodegeneration; protein aggregation ID AMYOTROPHIC-LATERAL-SCLEROSIS; SYNTHETIC MODEL PROTEINS; HELICAL COILED-COILS; ALZHEIMERS-DISEASE; OXIDATIVE STRESS; METAL-IONS; CASCADE HYPOTHESIS; SERUM COPPER; HYDROGEN-PEROXIDE; NMR-SPECTROSCOPY AB Aggregation of the amyloid-beta (A beta) peptide into insoluble plaques is a major factor in Alzheimer's disease (AD) pathology. Another major factor in AD is arguably metal ions, as metal dyshomeostasis is observed in AD patients, metal ions modulate A beta aggregation, and AD plaques contain numerous metals including redox-active Cu and Fe ions. In vivo, A beta is found in various cellular locations including membranes. So far, Cu(II)/A beta interactions and ROS generation have not been investigated in a membrane environment. Here, we study Cu(II) and Zn(II) interactions with A beta bound to SDS micelles or to engineered aggregation-inhibiting molecules (the cyclic peptide CP-2 and the Z(A beta 3)(12-58) Y18L Affibody molecule). In all studied systems the A beta N-terminal segment was found to be unbound, unstructured, and free to bind metal ions. In SDS micelles, A beta was found to bind Cu(II) and Zn(II) with the same ligands and the same K-D as in aqueous solution. ROS was generated in all Cu(II)/A beta complexes. These results indicate that binding of A beta to membranes, drugs, and other entities that do not interact with the A beta N-terminal part, appears not to compromise the N-terminal segment's ability to bind metal ions, nor impede the capacity of N-terminally bound Cu(II) to generate ROS. C1 [Tiiman, Ann; Luo, Jinghui; Wallin, Cecilia; Olsson, Lisa; Jarvet, Juri; Sholts, Sabrina B.; Graslund, Astrid; Warmlander, Sebastian K. T. S.] Stockholm Univ, Arrhenius Labs, Dept Biochem & Biophys, Stockholm, Sweden. [Luo, Jinghui] Univ Oxford, Chem Res Lab, Oxford OX1 2JD, England. [Lindgren, Joel] Affibody AB, Solna, Sweden. [Jarvet, Juri] NICPB, Tallinn, Estonia. [Roose, Per] Karolinska Inst, Inst Environm Med, Stockholm, Sweden. [Roose, Per] Capio St Goran Hosp, Dept Clin Physiol, Stockholm, Sweden. [Sholts, Sabrina B.] Smithsonian Inst, Natl Museum Nat Hist, Dept Anthropol, Washington, DC 20560 USA. [Rahimipour, Shai] Bar Ilan Univ, Dept Chem, Ramat Gan, Israel. [Abrahams, Jan Pieter] Univ Basel, Biozentrum, CH-4003 Basel, Switzerland. [Abrahams, Jan Pieter] Paul Scherrer Inst, Lab Biomol Res, Villigen, Switzerland. [Karlstrom, Amelie Eriksson] KTH Royal Inst Technol, Sch Biotechnol, Stockholm, Sweden. RP Warmlander, SKTS (reprint author), Stockholm Univ, Arrhenius Labs, Dept Biochem & Biophys, Stockholm, Sweden. EM seb@dbb.su.se FU Magnus Bergvall foundation; Swedish Research Council; Brain Foundation FX The work was funded by grants from the Magnus Bergvall foundation to SW, and from the Swedish Research Council and the Brain Foundation to AG. The discussion of the results was greatly improved by the insightful and constructive comments by the anonymous reviewers. NR 80 TC 0 Z9 0 U1 9 U2 9 PU IOS PRESS PI AMSTERDAM PA NIEUWE HEMWEG 6B, 1013 BG AMSTERDAM, NETHERLANDS SN 1387-2877 EI 1875-8908 J9 J ALZHEIMERS DIS JI J. Alzheimers Dis. PY 2016 VL 54 IS 3 BP 971 EP 982 DI 10.3233/JAD-160427 PG 12 WC Neurosciences SC Neurosciences & Neurology GA DZ2DF UT WOS:000385651800012 PM 27567855 ER PT J AU Zarina, G Sholts, SB Tichinin, A Rudovica, V Viksna, A Engizere, A Muiznieks, V Bartelink, EJ Warmlander, SKTS AF Zarina, Gunita Sholts, Sabrina B. Tichinin, Alina Rudovica, Vita Viksna, Arturs Engizere, Austra Muiznieks, Vitolds Bartelink, Eric J. Warmlander, Sebastian K. T. S. TI Cribra orbitalia as a potential indicator of childhood stress: Evidence from paleopathology, stable C, N, and O isotopes, and trace element concentrations in children from a 17th-18th century cemetery in Jekabpils, Latvia SO JOURNAL OF TRACE ELEMENTS IN MEDICINE AND BIOLOGY LA English DT Article DE Epidemiology; Bioarchaeology; Nutrition; Physical anthropology; Trace elements; Cribra orbitalia ID IRON-DEFICIENCY-ANEMIA; POROTIC HYPEROSTOSIS; COPPER DEFICIENCY; BONE; DIET; SAMPLES; RATIOS; CHICK; LEAD AB Cribra orbitalia (CO), or porotic hyperostosis (PH) of the orbital roof, is one of the most common pathological conditions found in archaeological subadult skeletal remains. Reaching frequencies higher than 50% in many prehistoric samples, CO has been generally attributed to a variety of factors including malnutrition (e.g., megaloblastic anemia) and parasitism. In this study, we tested the relationship between CO, trace element concentrations, and stable isotope values (delta C-13, delta N-15, delta O-18) in subadult skeletons from a 17th to 18th century cemetery in the historic town of Jekabpils, Latvia. A total of 28 subadults were examined, seven of which (25%) showed evidence of CO. Bioarchaeological evidence indicated high mortality for children in this cemetery: half of the burials were subadults under the age of 14, while a third were under the age of four. Life expectancy at birth was estimated to have been only 21.6 years. Trace element concentrations measured by Inductively Coupled Plasma - Mass Spectrometry (ICP-MS) showed no relationship between presence or absence of CO and levels of manganese, zinc, strontium, barium, copper, cadmium, or lead in the bones (p>0.05). However, a significant correlation (p<0.05) was found between the presence of CO and decreased levels of iron. The correlations between CO and decreased levels of copper and lead approached significance (p=0.056 for both elements). Individuals with CO furthermore displayed significantly lower delta N-15 isotope values, suggesting greater consumption of lower trophic level food resources than those unaffected by CO; delta C-13 and delta O-18 values, in contrast, showed no significant differences. These results suggest that the prevalence of CO may be related to dietary deficiencies. In this case, low iron levels may also signify a diet low in other key vitamins (e.g., B-g and B-12), which are known to cause megaloblastic anemia. (C) 2016 Elsevier GmbH. All rights reserved. C1 [Zarina, Gunita] Univ Latvia, Inst Latvian Hist, Riga, Latvia. [Sholts, Sabrina B.] Smithsonian Inst, Natl Museum Nat Hist, Dept Anthropol, Washington, DC 20560 USA. [Tichinin, Alina; Bartelink, Eric J.] Calif State Univ Chico, Dept Anthropol, Chico, CA 95929 USA. [Rudovica, Vita; Viksna, Arturs] Univ Latvia, Dept Analyt Chem, Riga, Latvia. [Engizere, Austra; Muiznieks, Vitolds] Latvian Natl Museum Hist, Riga, Latvia. [Warmlander, Sebastian K. T. S.] Univ Stockholm, Div Biophys, S-10691 Stockholm, Sweden. [Warmlander, Sebastian K. T. S.] Univ Calif Los Angeles, Cotsen Inst Archaeol, Getty Conservat Programme, Los Angeles, CA USA. RP Warmlander, SKTS (reprint author), Univ Stockholm, Div Biophys, S-10691 Stockholm, Sweden. EM seb@dbb.su.se NR 42 TC 0 Z9 0 U1 5 U2 5 PU ELSEVIER GMBH, URBAN & FISCHER VERLAG PI JENA PA OFFICE JENA, P O BOX 100537, 07705 JENA, GERMANY SN 0946-672X J9 J TRACE ELEM MED BIO JI J. Trace Elem. Med. Biol. PY 2016 VL 38 SI SI BP 131 EP 137 DI 10.1016/j.jtemb.2016.05.008 PG 7 WC Biochemistry & Molecular Biology; Endocrinology & Metabolism SC Biochemistry & Molecular Biology; Endocrinology & Metabolism GA DY9RU UT WOS:000385473600016 PM 27289401 ER PT J AU Wallin, C Kulkarni, YS Abelein, A Jarvet, J Liao, QH Strodel, B Olsson, L Luo, JH Abrahams, JP Sholts, SB Roos, PM Kamerlin, SCL Graslund, A Warmlander, SKTS AF Wallin, Cecilia Kulkarni, Yashraj S. Abelein, Axel Jarvet, Juri Liao, Qinghua Strodel, Birgit Olsson, Lisa Luo, Jinghui Abrahams, Jan Pieter Sholts, Sabrina B. Roos, Per M. Kamerlin, Shina C. L. Graslund, Astrid Warmlander, Sebastian K. T. S. TI Characterization of Mn(II) ion binding to the amyloid-beta peptide in Alzheimer's disease SO JOURNAL OF TRACE ELEMENTS IN MEDICINE AND BIOLOGY LA English DT Article DE Manganese; Neurodegeneration; Metal-protein binding; Spectroscopy; Molecular dynamics ID AMYOTROPHIC-LATERAL-SCLEROSIS; LINEAR CONSTRAINT SOLVER; PARTICLE MESH EWALD; CEREBROSPINAL-FLUID; METAL-IONS; A-BETA; FORCE-FIELD; MOLECULAR SIMULATION; COPPER-BINDING; BLOOD-PLASMA AB Growing evidence links neurodegenerative diseases to metal exposure. Aberrant metal ion concentrations have been noted in Alzheimer's disease (AD) brains, yet the role of metals in AD pathogenesis remains unresolved. A major factor in AD pathogenesis is considered to be aggregation of and amyloid formation by amyloid-beta (A beta) peptides. Previous studies have shown that A beta displays specific binding to Cu(II) and Zn(II) ions, and such binding has been shown to modulate A beta aggregation. Here, we use nuclear magnetic resonance (NMR) spectroscopy to show that Mn(II) ions also bind to the N-terminal part of the A beta(1-40) peptide, with a weak binding affinity in the milli- to micromolar range. Circular dichroism (CD) spectroscopy, solid state atomic force microscopy (AFM), fluorescence spectroscopy, and molecular modeling suggest that the weak binding of Mn(II) to A beta may not have a large effect on the peptide's aggregation into amyloid fibrils. However, identification of an additional metal ion displaying A beta binding reveals more complex AD metal chemistry than has been previously considered in the literature. (C) 2016 Elsevier GmbH. All rights reserved. C1 [Wallin, Cecilia; Abelein, Axel; Jarvet, Juri; Olsson, Lisa; Luo, Jinghui; Sholts, Sabrina B.; Graslund, Astrid; Warmlander, Sebastian K. T. S.] Stockholm Univ, Dept Biochem & Biophys, Svante Arrhenius Vag 16C, S-10691 Stockholm, Sweden. [Kulkarni, Yashraj S.; Kamerlin, Shina C. L.] Uppsala Univ, Dept Cell & Mol Biol, Husargatan 3, S-75124 Uppsala, Sweden. [Abelein, Axel] Karolinska Inst, Div Neurogeriatr, Dept Neurobiol Care Sci & Soc NVS, H1,Novum Pl 5, S-14157 Stockholm, Sweden. [Jarvet, Juri] NICPB, Akad Tee 23, EE-12618 Tallinn, Estonia. [Liao, Qinghua; Strodel, Birgit] Forschungszentrum Julich, Inst Complex Syst Struct Biochem, D-52425 Julich, Germany. [Strodel, Birgit] Univ Dusseldorf, Inst Theoret & Computat Chem, Univ Str 1, D-40225 Dusseldorf, Germany. [Luo, Jinghui] Univ Oxford, Chem Res Lab, 12 Mansfield Rd, Oxford OX1 3TA, England. [Abrahams, Jan Pieter] Univ Basel, Biozentrum, Klingelbergstr 70, CH-4056 Basel, Switzerland. [Abrahams, Jan Pieter] Paul Scherrer Inst, Dept Biol & Chem, Lab Biomol Res, OFLC 102, CH-5232 Villigen, Switzerland. [Sholts, Sabrina B.] Smithsonian Inst, Natl Museum Nat Hist, Dept Anthropol, 10th & Constitut Ave NW, Washington, DC 20013 USA. [Roos, Per M.] Karolinska Inst, Inst Environm Med, Nobels Vag 13, S-17177 Stockholm, Sweden. [Roos, Per M.] Capio St Goran Hosp, Dept Clin Physiol, St Goransplan 1, S-11219 Stockholm, Sweden. RP Warmlander, SKTS (reprint author), Stockholm Univ, Dept Biochem & Biophys, Svante Arrhenius Vag 16C, S-10691 Stockholm, Sweden. EM seb@dbb.su.se RI Abrahams, Jan Pieter/G-7287-2016 OI Abrahams, Jan Pieter/0000-0001-8216-1868 NR 84 TC 2 Z9 2 U1 9 U2 9 PU ELSEVIER GMBH, URBAN & FISCHER VERLAG PI JENA PA OFFICE JENA, P O BOX 100537, 07705 JENA, GERMANY SN 0946-672X J9 J TRACE ELEM MED BIO JI J. Trace Elem. Med. Biol. PY 2016 VL 38 SI SI BP 183 EP 193 DI 10.1016/j.jtemb.2016.03.009 PG 11 WC Biochemistry & Molecular Biology; Endocrinology & Metabolism SC Biochemistry & Molecular Biology; Endocrinology & Metabolism GA DY9RU UT WOS:000385473600023 PM 27085215 ER PT S AU Bender, AN Ade, PAR Andersond, AJ Avva, J Ahmed, Z Arnold, K Austermann, JE Thakur, RB Benson, BA Bleem, LE Byrum, K Carlstrom, JE Carter, FW Chang, CL Cho, HM Cliche, JF Crawford, TM Cukierman, A Czaplewski, D Ding, J Divan, R de Haan, T Dobbs, MA Dutcher, D Everett, W Gilbert, A Groh, JC Guyser, R Halverson, NW Harke-Hosemann, A Harrington, NL Hattori, K Henning, JW Hilton, GC Holzapfel, WL Huang, N Irwin, KD Jeong, O Khaire, T Korman, M Kubik, D Kuo, CL Lee, AT Leitch, EM Lendinez, S Meyer, SS Miller, CS Montgomery, J Nadolski, A Natoli, T Nguyen, H Noyosad, V Padin, S Pan, Z Pearson, J Posada, CM Rahlin, A Reichardt, CL Ruhl, JE Saliwanchik, BR Sayre, JT Shariff, JA Shirley, I Shirokoff, E Smecher, G Sobrin, J Stan, L Stark, AA Story, K Suzuki, A Tang, QY Thompson, KL Tucker, C Vanderlinde, K Vieira, JD Wang, G Whitehorn, N Yefremenko, V Yoon, KW AF Bender, A. N. Ade, P. A. R. Andersond, A. J. Avva, J. Ahmed, Z. Arnold, K. Austermann, J. E. Thakur, R. Basu Benson, B. A. Bleem, L. E. Byrum, K. Carlstrom, J. E. Carter, F. W. Chang, C. L. Cho, H. M. Cliche, J. F. Crawford, T. M. Cukierman, A. Czaplewski, D. Ding, J. Divan, R. de Haan, T. Dobbs, M. A. Dutcher, D. Everett, W. Gilbert, A. Groh, J. C. Guyser, R. Halverson, N. W. Harke-Hosemann, A. Harrington, N. L. Hattori, K. Henning, J. W. Hilton, G. C. Holzapfel, W. L. Huang, N. Irwin, K. D. Jeong, O. Khaire, T. Korman, M. Kubik, D. Kuo, C. L. Lee, A. T. Leitch, E. M. Lendinez, S. Meyer, S. S. Miller, C. S. Montgomery, J. Nadolski, A. Natoli, T. Nguyen, H. Noyosad, V. Padin, S. Pan, Z. Pearson, J. Posada, C. M. Rahlin, A. Reichardt, C. L. Ruhl, J. E. Saliwanchik, B. R. Sayre, J. T. Shariff, J. A. Shirley, I. Shirokoff, E. Smecher, G. Sobrin, J. Stan, L. Stark, A. A. Story, K. Suzuki, A. Tang, Q. Y. Thompson, K. L. Tucker, C. Vanderlinde, K. Vieira, J. D. Wang, G. Whitehorn, N. Yefremenko, V. Yoon, K. W. BE Holland, WS Zmuidzinas, J TI Integrated Performance of a Frequency Domain Multiplexing Readout in the SPT-3G Receiver SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE ID QUANTUM INTERFERENCE DEVICE; ARRAYS AB The third generation receiver for the South Pole Telescope, SPT-3G, will make extremely deep, arcminute-resolution maps of the temperature and polarization of the cosmic microwave background. The SPT-3G maps will enable studies of the B-mode polarization signature, constraining primordial gravitational waves as well as the effect of massive neutrinos on structure formation in the late universe. The SPT-3G receiver will achieve exceptional sensitivity through a focal plane of similar to 16,000 transition-edge sensor bolometers, an order of magnitude more than the current SPTpol receiver. SPT-3G uses a frequency domain multiplexing (fMux) scheme to read out the focal plane, combining the signals from 64 bolometers onto a single pair of wires. The fMux readout facilitates the large number of detectors in the SPT-3G focal plane by limiting the thermal load due to readout wiring on the 250 millikelvin cryogenic stage. A second advantage of the fMux system is that the operation of each bolometer can be optimized. In addition to these benefits, the fMux readout introduces new challenges into the design and operation of the receiver. The bolometers are operated at a range of frequencies up to 5 MHz, requiring control of stray reactances over a large bandwidth. Additionally, crosstalk between multiplexed detectors will inject large false signals into the data if not adequately mitigated. SPT-3G is scheduled to deploy to the South Pole Telescope in late 2016. Here, we present the pre-deployment performance of the fMux readout system with the SPT-3G focal plane. C1 [Bender, A. N.; Bleem, L. E.; Byrum, K.; Carlstrom, J. E.; Carter, F. W.; Chang, C. L.; Yefremenko, V.] Argonne Natl Lab, Div High Energy Phys, 9700 S Cass Ave, Argonne, IL 60439 USA. [Bender, A. N.; Andersond, A. J.; Thakur, R. Basu; Benson, B. A.; Bleem, L. E.; Carter, F. W.; Chang, C. L.; Crawford, T. M.; Dutcher, D.; Henning, J. W.; Meyer, S. S.; Padin, S.; Pan, Z.; Shirokoff, E.; Sobrin, J.; Tang, Q. Y.] Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA. [Ade, P. A. R.; Tucker, C.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3YB, S Glam, Wales. [Andersond, A. J.; Benson, B. A.; Nguyen, H.; Rahlin, A.] Fermilab Natl Accelerator Lab, MS209,POB 500, Batavia, IL 60510 USA. [Avva, J.; Cukierman, A.; de Haan, T.; Groh, J. C.; Harrington, N. L.; Holzapfel, W. L.; Huang, N.; Jeong, O.; Lee, A. T.; Shirley, I.; Suzuki, A.; Whitehorn, N.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Ahmed, Z.; Irwin, K. D.; Kuo, C. L.; Story, K.; Thompson, K. L.; Yoon, K. W.] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, 452 Lomita Mall, Stanford, CA 94305 USA. [Ahmed, Z.; Irwin, K. D.; Kuo, C. L.; Story, K.; Thompson, K. L.; Yoon, K. W.] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA. [Ahmed, Z.; Irwin, K. D.; Kuo, C. L.; Thompson, K. L.; Yoon, K. W.] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA. [Arnold, K.] Univ Wisconsin, Dept Phys, 1150 Univ Ave, Madison, WI 53706 USA. [Austermann, J. E.; Hilton, G. C.] NIST Quantum Devices Grp, 325 Broadway Mailcode 817-03, Boulder, CO 80305 USA. [Benson, B. A.; Carlstrom, J. E.; Chang, C. L.; Crawford, T. M.; Leitch, E. M.; Meyer, S. S.; Shirokoff, E.; Tang, Q. Y.] Univ Chicago, Dept Astron & Astrophys, 5640 South Ellis Ave, Chicago, IL 60637 USA. [Carlstrom, J. E.; Meyer, S. S.] Univ Chicago, Enrico Fermi Inst, 5640 South Ellis Ave, Chicago, IL 60637 USA. [Carlstrom, J. E.; Dutcher, D.; Meyer, S. S.; Sobrin, J.] Univ Chicago, Dept Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA. [Cliche, J. F.; Dobbs, M. A.; Gilbert, A.; Montgomery, J.] McGill Univ, Dept Phys, 3600 Rue Univ, Montreal, PQ H3A 2T8, Canada. [Czaplewski, D.; Divan, R.; Miller, C. S.; Stan, L.] Argonne Natl Lab, Ctr Nanoscale Mat, 9700 S Cass Ave, Argonne, IL 60439 USA. [Ding, J.; Lendinez, S.; Noyosad, V.; Pearson, J.; Posada, C. M.] Argonne Natl Lab, Div Mat Sci, 9700 S Cass Ave, Argonne, IL 60439 USA. [Dobbs, M. A.] Canadian Inst Adv Res, CIFAR Program Cosmol & Grav, Toronto, ON M5G 1Z8, Canada. [Everett, W.; Halverson, N. W.] Univ Colorado, Dept Astrophys & Planetary Sci, CASA, Boulder, CO 80309 USA. [Guyser, R.; Harke-Hosemann, A.; Nadolski, A.; Vieira, J. D.] Univ Illinois, Astron Dept, 1002 W Green St, Urbana, IL 61801 USA. [Halverson, N. W.] Univ Colorado, Dept Phys, Boulder, CO 80309 USA. [Hattori, K.] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan. [Korman, M.; Ruhl, J. E.; Saliwanchik, B. R.; Shariff, J. A.] Univ Calif Davis, Dept Phys, One Shields Ave, Davis, CA 95616 USA. [Lee, A. T.] Lawrence Berkeley Natl Lab, Phys Div, Berkeley, CA 94720 USA. [Vanderlinde, K.] Univ Toronto, Dept Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada. [Reichardt, C. L.] Univ Melbourne, Sch Phys, Parkville, Vic 3010, Australia. [Smecher, G.] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA. [Stark, A. A.] Three Speed Log Inc, Vancouver, BC V6A 2J8, Canada. [Natoli, T.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Vieira, J. D.] Univ Toronto, Dunlap Inst Astron & Astrophys, 50 St George St, Toronto, ON M5S 3H4, Canada. Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA. RP Bender, AN (reprint author), Argonne Natl Lab, Div High Energy Phys, 9700 S Cass Ave, Argonne, IL 60439 USA.; Bender, AN (reprint author), Univ Chicago, Kavli Inst Cosmol Phys, 5640 South Ellis Ave, Chicago, IL 60637 USA. EM abender@anl.gov RI Novosad, V /J-4843-2015; DING, Junjia/K-2277-2013; OI DING, Junjia/0000-0002-9917-9156; Stark, Antony/0000-0002-2718-9996 NR 13 TC 1 Z9 1 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 99141D DI 10.1117/12.2232146 PN 1 PG 11 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800032 ER PT S AU Grayson, JA Ade, PAR Ahmed, Z Alexander, KD Amiri, M Barkats, D Benton, SJ Bischoff, CA Bock, JJ Boenish, H Bowens-Rubin, R Buder, I Bullock, E Buza, V Connors, J Filippini, JP Fliescher, S Halpern, M Harrison, S Hilton, GC Hristov, VV Hui, H Irwin, KD Kang, J Karkare, KS Karpel, E Kefeli, S Kernasovskiy, SA Kovac, JM Kuo, CL Leitch, EM Lueker, M Megerian, KG Monticue, V Namikawa, T Netterfield, CB Nguyen, HT O'Brient, R Ogburn, RW Pryke, C Reintsema, CD Richter, S Schwarz, R Sorensen, C Sheehy, CD Staniszewski, ZK Steinbach, B Teply, GP Thompson, KL Tolan, JE Tucker, C Turner, AD Vieregg, AG Wandui, A Weber, AC Wiebe, DV Willmert, J Wu, WLK Yoon, KW AF Grayson, J. A. Ade, P. A. R. Ahmed, Z. Alexander, K. D. Amiri, M. Barkats, D. Benton, S. J. Bischoff, C. A. Bock, J. J. Boenish, H. Bowens-Rubin, R. Buder, I. Bullock, E. Buza, V. Connors, J. Filippini, J. P. Fliescher, S. Halpern, M. Harrison, S. Hilton, G. C. Hristov, V. V. Hui, H. Irwin, K. D. Kang, J. Karkare, K. S. Karpel, E. Kefeli, S. Kernasovskiy, S. A. Kovac, J. M. Kuo, C. L. Leitch, E. M. Lueker, M. Megerian, K. G. Monticue, V. Namikawa, T. Netterfield, C. B. Nguyen, H. T. O'Brient, R. Ogburn, R. W. Pryke, C. Reintsema, C. D. Richter, S. Schwarz, R. Sorensen, C. Sheehy, C. D. Staniszewski, Z. K. Steinbach, B. Teply, G. P. Thompson, K. L. Tolan, J. E. Tucker, C. Turner, A. D. Vieregg, A. G. Wandui, A. Weber, A. C. Wiebe, D. V. Willmert, J. Wu, W. L. K. Yoon, K. W. BE Holland, WS Zmuidzinas, J TI BICEP3 performance overview and planned Keck Array upgrade SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Cosmic Microwave Background; Inflation; Gravitational Waves; Polarization; BICEP; Keck Array ID B-MODE POLARIZATION; BOLOMETERS AB BICEP3 is a 520mm aperture, compact two-lens refractor designed to observe the polarization of the cosmic microwave background (CMB) at 95 GHz. Its focal plane consists of modularized tiles of antenna-coupled transition edge sensors (TESs), similar to those used in BICEP2 and the Keck Array. The increased per-receiver optical throughput compared to BICEP2/Keck Array, due to both its faster f/1.7 optics and the larger aperture, more than doubles the combined mapping speed of the BICEP/Keck program. The BICEP3 receiver was recently upgraded to a full complement of 20 tiles of detectors (2560 TESs) and is now beginning its second year of observation (and first science season) at the South Pole. We report on its current performance and observing plans. Given its high per-receiver throughput while maintaining the advantages of a compact design, BICEP3-class receivers are ideally suited as building blocks for a 3rd-generation CMB experiment, consisting of multiple receivers spanning 35 GHz to 270 GHz with total detector count in the tens of thousands. We present plans for such an array, the new "BICEP Array" that will replace the Keck Array at the South Pole, including design optimization, frequency coverage, and deployment/observing strategies. C1 [Grayson, J. A.; Ahmed, Z.; Irwin, K. D.; Kang, J.; Karpel, E.; Kernasovskiy, S. A.; Kuo, C. L.; Monticue, V.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Grayson, J. A.; Ahmed, Z.; Irwin, K. D.; Kang, J.; Karpel, E.; Kernasovskiy, S. A.; Kuo, C. L.; Monticue, V.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] SLAC Natl Accelerator Lab, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA. [Ade, P. A. R.; Halpern, M.; Tucker, C.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Alexander, K. D.; Barkats, D.; Bischoff, C. A.; Boenish, H.; Bowens-Rubin, R.; Buder, I.; Buza, V.; Connors, J.; Harrison, S.; Karkare, K. S.; Kovac, J. M.; Richter, S.; Sorensen, C.; Vieregg, A. G.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Amiri, M.; Wiebe, D. V.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada. [Benton, S. J.; Netterfield, C. B.] Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada. [Benton, S. J.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Bock, J. J.; Filippini, J. P.; Hristov, V. V.; Hui, H.; Kefeli, S.; Lueker, M.; O'Brient, R.; Staniszewski, Z. K.; Steinbach, B.; Teply, G. P.] CALTECH, Dept Phys, Pasadena, CA 91125 USA. [Bock, J. J.; Megerian, K. G.; Nguyen, H. T.; O'Brient, R.; Staniszewski, Z. K.; Turner, A. D.; Weber, A. C.] Jet Prop Lab, Pasadena, CA 91109 USA. [Bullock, E.; Pryke, C.] Univ Minnesota, Minnesota Inst Astrophys, Minneapolis, MN 55455 USA. [Buza, V.; Kovac, J. M.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Filippini, J. P.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Filippini, J. P.] Univ Illinois, Dept Astron, Urbana, IL 61801 USA. [Fliescher, S.; Pryke, C.; Schwarz, R.; Sheehy, C. D.; Willmert, J.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA. [Hilton, G. C.; Irwin, K. D.; Reintsema, C. D.] NIST, Boulder, CO 80305 USA. [Leitch, E. M.; Sheehy, C. D.; Vieregg, A. G.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA. [Netterfield, C. B.] Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada. [Teply, G. P.] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA. [Vieregg, A. G.] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 USA. [Wu, W. L. K.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Grayson, JA (reprint author), Stanford Univ, Dept Phys, Stanford, CA 94305 USA.; Grayson, JA (reprint author), SLAC Natl Accelerator Lab, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA. EM jgrayson@stanford.edu OI Karkare, Kirit/0000-0002-5215-6993; Namikawa, Toshiya/0000-0003-3070-9240 NR 19 TC 1 Z9 1 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 99140S DI 10.1117/12.2233894 PN 1 PG 17 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800017 ER PT S AU Grimes, P Blundell, R Paine, S Tong, CYE Zeng, LZ AF Grimes, Paul Blundell, Ray Paine, Scott Tong, C. -Y. Edward Zeng, Lingzhen BE Holland, WS Zmuidzinas, J TI Next Generation Receivers for the Submillimeter Array SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Millimeter interferometry; Submillimeter interferometry; Millimeter receivers; Submillimeter receivers; Radio telescopes AB The Submillimeter Array (SMA) is an 8-element mm/sub-mm interferometer on the summit of Maunakea, Hawaii that is operated jointly by the Smithsonian Astrophysical Observatory (SAO) and the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA). After nearly 13 years of operation, we are undertaking a major upgrade of the array's cryogenics, receivers and other systems that will enhance the science capabilities of the array and replace components reaching end-of-life. Here we describe the new receivers, containing dual-polarization, ultra-wideband SIS mixers operating at 230 and 345 GHz, the new ultra-wideband IF signal transport and correlator system, and the enhanced observing capabilities that will be enabled by this upgrade. C1 [Grimes, Paul; Blundell, Ray; Paine, Scott; Tong, C. -Y. Edward; Zeng, Lingzhen] Harvard Smithsonian Ctr Astrophys, Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA. RP Grimes, P (reprint author), Harvard Smithsonian Ctr Astrophys, Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA. EM pgrimes@cfa.harvard.edu NR 13 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 991424 DI 10.1117/12.2232790 PN 1 PG 9 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800052 ER PT S AU Harrington, K Marriage, T Ali, A Appel, JW Bennett, CL Boone, F Brewer, M Chan, MW Chuss, DT Colazo, F Dahal, S Denis, K Dunner, R Eimer, J Essinger-Hileman, T Fluxa, P Halpern, M Hilton, G Hinshaw, GF Hubmayr, J Iuliano, J Karakla, J McMahon, J Miller, NT Moseley, SH Palma, G Parker, L Petroff, M Pradenas, B Rostem, K Sagliocca, M Valle, D Watts, D Wollack, E Xu, ZL Zeng, LZ AF Harrington, Kathleen Marriage, Tobias Ali, Aamir Appel, John W. Bennett, Charles L. Boone, Fletcher Brewer, Michael Chan, Manwei Chuss, David T. Colazo, Felipe Dahal, Sumit Denis, Kevin Dunner, Rolando Eimer, Joseph Essinger-Hileman, Thomas Fluxa, Pedro Halpern, Mark Hilton, Gene Hinshaw, Gary F. Hubmayr, Johannes Iuliano, Jeffery Karakla, John McMahon, Jeff Miller, Nathan T. Moseley, Samuel H. Palma, Gonzalo Parker, Lucas Petroff, Matthew Pradenas, Bastian Rostem, Karwan Sagliocca, Marco Valle, Deniz Watts, Duncan Wollack, Edward Xu, Zhilei Zeng, Lingzhen BE Holland, WS Zmuidzinas, J TI The Cosmology Large Angular Scale Surveyor SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE ID PROBE WMAP OBSERVATIONS; B-MODE POLARIZATION; MICROWAVE BACKGROUND POLARIMETRY; INFLATIONARY UNIVERSE; FLATNESS; HORIZON AB The Cosmology Large Angular Scale Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from inflation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular scales. The frequencies of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145/217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower frequencies and dust emission at higher frequencies. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular scales. Using this combination of a broad frequency range, large sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.). C1 [Harrington, Kathleen; Marriage, Tobias; Ali, Aamir; Appel, John W.; Bennett, Charles L.; Brewer, Michael; Chan, Manwei; Dahal, Sumit; Eimer, Joseph; Essinger-Hileman, Thomas; Iuliano, Jeffery; Karakla, John; Miller, Nathan T.; Parker, Lucas; Petroff, Matthew; Rostem, Karwan; Valle, Deniz; Watts, Duncan; Xu, Zhilei] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA. [Halpern, Mark; Hinshaw, Gary F.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z4, Canada. [Colazo, Felipe; Denis, Kevin; Miller, Nathan T.; Moseley, Samuel H.; Rostem, Karwan; Wollack, Edward] NASA, Goddard Space Flight Ctr, Code 660, Greenbelt, MD 20771 USA. [Chuss, David T.; Sagliocca, Marco] Villanova Univ, Dept Phys, Villanova, PA 19085 USA. [Boone, Fletcher; McMahon, Jeff] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA. [Dunner, Rolando; Fluxa, Pedro] Pontificia Univ Catolica Chile, Inst Astrofis, Fac Fis, Ave Vicuna Mackenna 4860, Santiago 7820436, Chile. [Dunner, Rolando; Fluxa, Pedro] Pontificia Univ Catolica Chile, Ctr Astroingn, Fac Fis, Ave Vicuna Mackenna 4860, Santiago 7820436, Chile. [Hilton, Gene; Hubmayr, Johannes] Natl Inst Stand & Technol, 325 Broadway, Boulder, CO 80305 USA. [Zeng, Lingzhen] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Palma, Gonzalo; Pradenas, Bastian] Univ Chile, Dept Phys, FCFM, Blanco Encalada 2008, Santiago, Chile. RP Harrington, K (reprint author), Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA. EM kharrington@jhu.edu RI Wollack, Edward/D-4467-2012 OI Wollack, Edward/0000-0002-7567-4451 NR 40 TC 1 Z9 1 U1 2 U2 2 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 99141K DI 10.1117/12.2233125 PN 1 PG 21 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800038 ER PT S AU Hui, H Ade, PAR Ahmed, Z Alexander, KD Amiri, M Barkats, D Benton, SJ Bischoff, CA Bock, JJ Boenish, H Bowens-Rubin, R Buder, I Bullock, E Buza, V Connors, J Filippini, JP Fliescher, S Grayson, JA Halpern, M Harrison, S Hilton, GC Hristov, VV Irwin, KD Kang, J Karkare, KS Karpel, E Kefeli, S Kernasovskiy, SA Kovac, JM Kuo, CL Leitch, EM Lueker, M Megerian, KG Monticue, V Namikawa, T Netterfield, CB Nguyen, T O'Brient, R Ogburn, RW Pryke, C Reintsema, CD Richter, S Schwarz, R Sorensen, C Sheehy, CD Staniszewski, ZK Steinbach, B Teply, GP Thompson, KL Tolan, JE Tucker, C Turner, AD Vieregg, AG Wandui, A Weber, AC Wiebe, DV Willmert, J Wu, WLK Yoon, KW AF Hui, H. Ade, P. A. R. Ahmed, Z. Alexander, K. D. Amiri, M. Barkats, D. Benton, S. J. Bischoff, C. A. Bock, J. J. Boenish, H. Bowens-Rubin, R. Buder, I. Bullock, E. Buza, V. Connors, J. Filippini, J. P. Fliescher, S. Grayson, J. A. Halpern, M. Harrison, S. Hilton, G. C. Hristov, V. V. Irwin, K. D. Kang, J. Karkare, K. S. Karpel, E. Kefeli, S. Kernasovskiy, S. A. Kovac, J. M. Kuo, C. L. Leitch, E. M. Lueker, M. Megerian, K. G. Monticue, V. Namikawa, T. Netterfield, C. B. Nguyen, T. O'Brient, R. Ogburn, R. W. Pryke, C. Reintsema, C. D. Richter, S. Schwarz, R. Sorensen, C. Sheehy, C. D. Staniszewski, Z. K. Steinbach, B. Teply, G. P. Thompson, K. L. Tolan, J. E. Tucker, C. Turner, A. D. Vieregg, A. G. Wandui, A. Weber, A. C. Wiebe, D. V. Willmert, J. Wu, W. L. K. Yoon, K. W. BE Holland, WS Zmuidzinas, J TI BICEP3 focal plane design and detector performance SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Cosmic Microwave Background; BICEP; Keck Array; Polarization ID BOLOMETERS AB BICEP3, the latest telescope in the BICEP/Keck program, started science observations in March 2016. It is a 550mm aperture refractive telescope observing the polarization of the cosmic microwave background at 95 GHz. We show the focal plane design and detector performance, including spectral response, optical efficiency and preliminary sensitivity of the upgraded BICEP3. We demonstrate 9.72 mu K-CMB root s noise performance of the BICEP3 receiver. C1 [Hui, H.; Bock, J. J.; Filippini, J. P.; Hristov, V. V.; Kefeli, S.; Lueker, M.; O'Brient, R.; Staniszewski, Z. K.; Steinbach, B.; Teply, G. P.] CALTECH, Dept Phys, Pasadena, CA 91125 USA. [Ade, P. A. R.; Tucker, C.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Ahmed, Z.; Grayson, J. A.; Irwin, K. D.; Kang, J.; Karpel, E.; Kernasovskiy, S. A.; Kuo, C. L.; Monticue, V.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] SLAC Natl Accelerator Lab, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA. [Ahmed, Z.; Grayson, J. A.; Irwin, K. D.; Kang, J.; Karpel, E.; Kernasovskiy, S. A.; Kuo, C. L.; Monticue, V.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Alexander, K. D.; Barkats, D.; Bischoff, C. A.; Boenish, H.; Bowens-Rubin, R.; Buder, I.; Buza, V.; Connors, J.; Harrison, S.; Karkare, K. S.; Kovac, J. M.; Richter, S.; Sorensen, C.; Vieregg, A. G.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Amiri, M.; Halpern, M.; Wiebe, D. V.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada. [Benton, S. J.; Netterfield, C. B.] Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada. [Benton, S. J.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Bock, J. J.; Megerian, K. G.; Nguyen, T.; O'Brient, R.; Staniszewski, Z. K.; Turner, A. D.; Weber, A. C.] Jet Prop Lab, Pasadena, CA 91109 USA. [Bullock, E.; Pryke, C.] Univ Minnesota, Minnesota Inst Astrophys, Minneapolis, MN 55455 USA. [Buza, V.; Kovac, J. M.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Filippini, J. P.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Filippini, J. P.] Univ Illinois, Dept Astron, Urbana, IL 61801 USA. [Fliescher, S.; Pryke, C.; Schwarz, R.; Sheehy, C. D.; Willmert, J.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA. [Hilton, G. C.; Irwin, K. D.; Reintsema, C. D.] NIST, Boulder, CO 80305 USA. [Leitch, E. M.; Sheehy, C. D.; Vieregg, A. G.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA. [Netterfield, C. B.] Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada. [Teply, G. P.] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA. [Vieregg, A. G.] Univ Chicago, Enrico Fermi Inst, Dept Phys, Chicago, IL 60637 USA. [Wu, W. L. K.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Hui, H (reprint author), CALTECH, Dept Phys, Pasadena, CA 91125 USA. EM hhui@caltech.edu OI Karkare, Kirit/0000-0002-5215-6993; Namikawa, Toshiya/0000-0003-3070-9240 NR 11 TC 0 Z9 0 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 99140T DI 10.1117/12.2232986 PN 1 PG 11 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800018 ER PT S AU Karkare, KS Ade, PAR Ahmed, Z Alexander, KD Amiri, M Barkats, D Benton, SJ Bischoff, CA Bock, JJ Boenish, H Bowens-Rubin, R Buder, I Bullock, E Buza, V Connors, J Filippini, JP Fliescher, ST Grayson, JA Halpern, M Harrison, SA Hilton, GC Hristov, VV Hui, H Irwin, KD Kang, JH Karpel, S Kefeli, S Kernasovskiy, SA Kovac, JM Kuo, CL Leitch, EM Lueker, M Megerian, KG Monticue, V Namikawa, T Netterfield, CB Nguyen, HT O'Brient, R Ogburn, RW Pryke, C Reintsema, CD Richter, S St Germaine, MT Schwarz, R Sheehy, CD Staniszewski, ZK Steinbach, B Teply, GP Thompson, KL Tolan, JE Tucker, C Turner, AD Vieregg, AG Wandui, A Weber, A Willmert, J Wong, CL Wu, WLK Yoon, KW AF Karkare, K. S. Ade, P. A. R. Ahmed, Z. Alexander, K. D. Amiri, M. Barkats, D. Benton, S. J. Bischoff, C. A. Bock, J. J. Boenish, H. Bowens-Rubin, R. Buder, I. Bullock, E. Buza, V. Connors, J. Filippini, J. P. Fliescher, S. T. Grayson, J. A. Halpern, M. Harrison, S. A. Hilton, G. C. Hristov, V. V. Hui, H. Irwin, K. D. Kang, J. H. Karpel, E. Kefeli, S. Kernasovskiy, S. A. Kovac, J. M. Kuo, C. L. Leitch, E. M. Lueker, M. Megerian, K. C. Monticue, V. Namikawa, T. Netterfield, C. B. Nguyen, H. T. O'Brient, R. Ogburn, R. W. Pryke, C. Reintsema, C. D. Richter, S. St Germaine, M. T. Schwarz, R. Sheehy, C. D. Staniszewski, Z. K. Steinbach, B. Teply, C. P. Thompson, K. L. Tolan, J. E. Tucker, C. Turner, A. D. Vieregg, A. G. Wandui, A. Weber, A. Willmert, J. Wong, C. L. Wu, W. L. K. Yoon, K. W. BE Holland, WS Zmuidzinas, J TI Optical characterization of the BICEP3 CMB polarimeter at the South Pole SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Inflation; Gravitational waves; Cosmic microwave background; Polarization; BICEP ID KECK ARRAY; PERFORMANCE; GHZ AB BICEP3 is a small-aperture refracting cosmic microwave background (CMB) telescope designed to make sensitive polarization maps in pursuit of a potential B-mode signal from inflationary gravitational waves. It is the latest in the BICEP/Keck Array series of CMB experiments located at the South Pole, which has provided the most stringent constraints on inflation to date. For the 2016 observing season, BICEP3 was outfitted with a full suite of 2400 optically coupled detectors operating at 95 GHz. In these proceedings we report on the far field beam performance using calibration data taken during the 2015-2016 summer deployment season in situ with a thermal chopped source. We generate high-fidelity per-detector beam maps, show the array-averaged beam profile, and characterize the differential beam response between co-located, orthogonally polarized detectors which contributes to the leading instrumental systematic in pair differencing experiments. We find that the levels of differential pointing, beamwidth, and ellipticity are similar to or lower than those measured for BICEP2 and Keck Array. The magnitude and distribution of BICEP3's differential beam mismatch - and the level to which temperature-to-polarization leakage may be marginalized over or subtracted in analysis - will inform the design of next-generation CMB experiments with many thousands of detectors. C1 [Karkare, K. S.; Alexander, K. D.; Barkats, D.; Bischoff, C. A.; Boenish, H.; Bowens-Rubin, R.; Buder, I.; Buza, V.; Connors, J.; Harrison, S. A.; Kovac, J. M.; Richter, S.; St Germaine, M. T.; Vieregg, A. G.; Wong, C. L.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Ade, P. A. R.; Tucker, C.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3AA, S Glam, Wales. [Ahmed, Z.; Grayson, J. A.; Irwin, K. D.; Kang, J. H.; Karpel, E.; Kernasovskiy, S. A.; Kuo, C. L.; Monticue, V.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Ahmed, Z.; Grayson, J. A.; Irwin, K. D.; Kang, J. H.; Kuo, C. L.; Namikawa, T.; Ogburn, R. W.; Thompson, K. L.; Tolan, J. E.; Wandui, A.; Wu, W. L. K.; Yoon, K. W.] SLAC Natl Accelerator Lab, Kavli Inst Particle Astrophys & Cosmol, Menlo Pk, CA 94025 USA. [Amiri, M.; Halpern, M.] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada. [Benton, S. J.; Netterfield, C. B.] Univ Toronto, Dept Phys, Toronto, ON M5S 1A7, Canada. [Benton, S. J.] Princeton Univ, Dept Phys, Princeton, NJ 08544 USA. [Bock, J. J.; Filippini, J. P.; Hristov, V. V.; Hui, H.; Kefeli, S.; Lueker, M.; Staniszewski, Z. K.; Steinbach, B.; Teply, C. P.] CALTECH, Dept Phys, Pasadena, CA 91125 USA. [Bock, J. J.; Megerian, K. C.; Nguyen, H. T.; O'Brient, R.; Staniszewski, Z. K.; Turner, A. D.; Weber, A.] Jet Prop Lab, Pasadena, CA 91109 USA. [Bullock, E.; Pryke, C.] Univ Minnesota, Minnesota Inst Astrophys, Minneapolis, MN 55455 USA. [Filippini, J. P.] Univ Illinois, Dept Phys, Urbana, IL 61801 USA. [Filippini, J. P.] Univ Illinois, Dept Astron, Urbana, IL 61801 USA. [Fliescher, S. T.; Pryke, C.; Schwarz, R.; Willmert, J.] Univ Minnesota, Sch Phys & Astron, Minneapolis, MN 55455 USA. [Hilton, G. C.; Irwin, K. D.; Reintsema, C. D.] NIST, Boulder, CO 80305 USA. [Leitch, E. M.; Sheehy, C. D.; Vieregg, A. G.] Univ Chicago, Chicago, IL 60637 USA. [Netterfield, C. B.] Canadian Inst Adv Res, Toronto, ON M5G 1Z8, Canada. [Wu, W. L. K.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. RP Karkare, KS (reprint author), 60 Garden St.MS 42, Cambridge, MA 02138 USA. EM kkarkare@cfa.harvard.edu OI Karkare, Kirit/0000-0002-5215-6993; Namikawa, Toshiya/0000-0003-3070-9240 NR 15 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 991430 DI 10.1117/12.2231747 PN 1 PG 17 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800075 ER PT S AU Posada, CM Ade, PAR Anderson, AJ Avva, J Ahmed, Z Arnold, KS Austermann, J Bender, AN Benson, BA Bleem, L Byrum, K Carlstrom, JE Carter, FW Chang, CL Cho, HM Cukierman, A Czaplewski, DA Ding, JJ Divan, RNS de Haan, T Dobbs, M Dutcher, D Everett, W Gannon, RN Guyser, RJ Halverson, NW Harrington, NL Hattori, K Henning, JW Hilton, GC Holzapfel, WL Huang, N Irwin, KD Jeong, O Khaire, T Korman, M Kubik, DL Kuo, CL Lee, AT Leitch, EM Escudero, SL Meyer, SS Miller, CS Montgomery, J Nadolski, A Natoli, TJ Nguyenm, H Novosad, V Padin, S Pan, ZD Pearson, JE Rahlin, A Reichardt, CL Ruhl, JE Saliwanchik, B Shirley, I Sayre, JT Shariff, JA Shirokoff, ED Stan, L Stark, AA Sobrin, J Story, K Suzuki, A Tang, QY Thakur, RB Thompson, KL Tucker, CE Vanderlinde, K Vieira, JD Wang, GS Whitehorn, N Yefremenko, V Yoon, KW AF Posada, Chrystian M. Ade, Peter A. R. Anderson, Adam J. Avva, Jessica Ahmed, Zeeshan Arnold, Kam S. Austermann, Jason Bender, Amy N. Benson, Bradford A. Bleem, Lindsey Byrum, Karen Carlstrom, John E. Carter, Faustin W. Chang, Clarence L. Cho, Hsiao-Mei Cukierman, Ari Czaplewski, David A. Ding, Junjia Divan, Ralu N. S. de Haan, Tijmen Dobbs, Matt Dutcher, Daniel Everett, Wendeline Gannon, Renae N. Guyser, Robert J. Halverson, Nils W. Harrington, Nicholas L. Hattori, Kaori Henning, Jason W. Hilton, Gene C. Holzapfel, William L. Huang, Nicholas Irwin, Kent D. Jeong, Oliver Khaire, Trupti Korman, Milo Kubik, Donna L. Kuo, Chao-Lin Lee, Adrian T. Leitch, Erik M. Escudero, Sergi Lendinez Meyer, Stephan S. Miller, Christina S. Montgomery, Joshua Nadolski, Andrew Natoli, Tyler J. Nguyenm, Hogan Novosad, Valentyn Padin, Stephen Pan, Zhaodi Pearson, John E. Rahlin, Alexandra Reichardt, Christian L. Ruhl, John E. Saliwanchik, Benjamin Shirley, Ian Sayre, James T. Shariff, Jamil A. Shirokoff, Erik D. Stan, Liliana Stark, Antony A. Sobrin, Joshua Story, Kyle Suzuki, Aritoki Tang, Qing Yang Thakur, Ritoban Basu Thompson, Keith L. Tucker, Carole E. Vanderlinde, Keith Vieira, Joaquin D. Wang, Gensheng Whitehorn, Nathan Yefremenko, Volodymyr Yoon, Ki Won BE Holland, WS Zmuidzinas, J TI Large arrays of dual-polarized multichroic TES detectors for CMB measurements with the SPT-3G receiver SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE CMB; SPT-3G; Bolometers; Transition Edge Sensors; Microfabrication; Superconducting Detectors; South Pole Telescope ID ELECTROTHERMAL FEEDBACK; MICROWAVE AB Detectors for cosmic microwave background (CMB) experiments are now essentially background limited, so a straightforward alternative to improve sensitivity is to increase the number of detectors. Large arrays of multichroic pixels constitute an economical approach to increasing the number of detectors within a given focal plane area. Here, we present the fabrication of large arrays of dual-polarized multichroic transition-edge-sensor (TES) bolometers for the South Pole Telescope third-generation CMB receiver (SPT-3G). The complete SPT-3G receiver will have 2690 pixels, each with six detectors, allowing for individual measurement of three spectral bands (centered at 95 GHz, 150 GHz and 220 GHz) in two orthogonal polarizations. In total, the SPT-3G focal plane will have 16140 detectors. Each pixel is comprised of a broad-band sinuous antenna coupled to a niobium microstrip transmission line. In-line filters are used to define the different band-passes before the millimeter-wavelength signal is fed to the respective Ti/Au TES sensors. Detectors are read out using a 64x frequency domain multiplexing (fMux) scheme. The microfabrication of the SPT-3G detector arrays involves a total of 18 processes, including 13 lithography steps. Together with the fabrication process, the effect of processing on the Ti/Au TES's T-c is discussed. In addition, detectors fabricated with Ti/Au TES films with Tc between 400 mK 560 mK are presented and their thermal characteristics are evaluated. Optical characterization of the arrays is presented as well, indicating that the response of the detectors is in good agreement with the design values for all three spectral bands (95 GHz, 150 GHz, and 220 GHz). The measured optical efficiency of the detectors is between 0.3 and 0.8. Results discussed here are extracted from a batch of research of development wafers used to develop the baseline process for the fabrication of the arrays of detectors to be deployed with the SPT-3G receiver. Results from these research and development wafers have been incorporated into the fabrication process to get the baseline fabrication process presented here. SPT-3G is scheduled to deploy to the South Pole Telescope in late 2016. C1 [Posada, Chrystian M.; Ding, Junjia; Khaire, Trupti; Escudero, Sergi Lendinez; Novosad, Valentyn; Pearson, John E.] Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. [Ade, Peter A. R.; Tucker, Carole E.] Cardiff Univ, Sch Phys & Astron, Cardiff CF24 3YB, S Glam, Wales. [Anderson, Adam J.; Bender, Amy N.; Benson, Bradford A.; Bleem, Lindsey; Carlstrom, John E.; Carter, Faustin W.; Chang, Clarence L.; Dutcher, Daniel; Henning, Jason W.; Leitch, Erik M.; Meyer, Stephan S.; Padin, Stephen; Pan, Zhaodi; Shirokoff, Erik D.; Sobrin, Joshua; Story, Kyle; Thakur, Ritoban Basu] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA. [Anderson, Adam J.; Benson, Bradford A.; Kubik, Donna L.; Rahlin, Alexandra] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Avva, Jessica; Cukierman, Ari; Harrington, Nicholas L.; Holzapfel, William L.; Huang, Nicholas; Jeong, Oliver; Lee, Adrian T.; Shirley, Ian; Suzuki, Aritoki; Whitehorn, Nathan] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Ahmed, Zeeshan; Irwin, Kent D.; Kuo, Chao-Lin; Thompson, Keith L.; Yoon, Ki Won] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, Stanford, CA 94305 USA. [Ahmed, Zeeshan; Irwin, Kent D.; Kuo, Chao-Lin; Thompson, Keith L.; Yoon, Ki Won] Stanford Univ, Dept Phys, Stanford, CA 94305 USA. [Ahmed, Zeeshan; Cho, Hsiao-Mei; Irwin, Kent D.; Kuo, Chao-Lin; Thompson, Keith L.; Yoon, Ki Won] SLAC Natl Accelerator Lab, 2575 Sand Hill Rd, Menlo Pk, CA 94025 USA. [Arnold, Kam S.] Univ Calif San Diego, Dept Phys, La Jolla, CA 92093 USA. [Austermann, Jason; Everett, Wendeline; Halverson, Nils W.; Nguyenm, Hogan; Sayre, James T.] Univ Colorado, Dept Astrophys & Planetary Sci, CASA, Boulder, CO 80309 USA. [Austermann, Jason; Hilton, Gene C.] NIST Quantum Devices Grp, Boulder, CO 80305 USA. [Bender, Amy N.; Bleem, Lindsey; Byrum, Karen; Carlstrom, John E.; Carter, Faustin W.; Chang, Clarence L.; Gannon, Renae N.; Wang, Gensheng; Yefremenko, Volodymyr] Argonne Natl Lab, Div High Energy Phys, Argonne, IL 60439 USA. [Benson, Bradford A.; Carlstrom, John E.; Chang, Clarence L.; Leitch, Erik M.; Meyer, Stephan S.; Shirokoff, Erik D.] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA. [Carlstrom, John E.; Meyer, Stephan S.] Univ Chicago, Enrico Fermi Inst, Chicago, IL 60637 USA. [Carlstrom, John E.; Dutcher, Daniel; Meyer, Stephan S.; Pan, Zhaodi; Sobrin, Joshua; Story, Kyle; Tang, Qing Yang] Univ Chicago, Dept Phys, Chicago, IL 60637 USA. [Czaplewski, David A.; Divan, Ralu N. S.; Miller, Christina S.; Stan, Liliana] Argonne Natl Lab, Ctr Nanoscale Mat, Argonne, IL 60439 USA. [de Haan, Tijmen; Dobbs, Matt; Montgomery, Joshua] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada. [Dobbs, Matt] Canadian Inst Adv Res, CIFAR Program Cosmol & Grav, Toronto, ON, Canada. [Guyser, Robert J.; Nadolski, Andrew; Vieira, Joaquin D.] Univ Illinois, Dept Astron, Urbana, IL 61801 USA. [Guyser, Robert J.; Vieira, Joaquin D.] Univ Illinois, Dept Phys, 1110 W Green St, Urbana, IL 61801 USA. [Halverson, Nils W.] Univ Colorado, Dept Phys, Boulder, CO 80309 USA. [Hattori, Kaori] High Energy Accelerator Res Org KEK, Tsukuba, Ibaraki 3050801, Japan. [Korman, Milo; Ruhl, John E.; Saliwanchik, Benjamin; Shariff, Jamil A.] Case Western Reserve Univ, Dept Phys, Cleveland, OH 44106 USA. [Lee, Adrian T.] Lawrence Berkeley Natl Lab, Div Phys, Berkeley, CA 94720 USA. [Natoli, Tyler J.; Vanderlinde, Keith] Univ Toronto, Dunlap Inst Astron & Astrophys, Toronto, ON M5S 3H4, Canada. [Reichardt, Christian L.] Univ Melbourne, Sch Phys, Melbourne, Vic, Australia. [Stark, Antony A.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Vanderlinde, Keith] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada. RP Posada, CM (reprint author), Argonne Natl Lab, Div Mat Sci, Argonne, IL 60439 USA. EM posada@anl.gov RI Novosad, V /J-4843-2015; DING, Junjia/K-2277-2013; OI DING, Junjia/0000-0002-9917-9156; Stark, Antony/0000-0002-2718-9996 NR 21 TC 2 Z9 2 U1 1 U2 1 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 991417 DI 10.1117/12.2232912 PN 1 PG 11 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800028 ER PT S AU Tong, CYE Grimes, PK Leiker, PS Zeng, LZ Lu, WC Chen, TJ Han, CC Wang, MJ AF Tong, C. -Y. Edward Grimes, Paul K. Leiker, Patrick S. Zeng, Lingzhen Lu, Wei-Chun Chen, Tse-Jun Han, Chih-Chiang Wang, Ming-Jye BE Holland, WS Zmuidzinas, J TI A Wideband 240 GHz Receiver for the Submillimeter Array SO MILLIMETER, SUBMILLIMETER, AND FAR-INFRARED DETECTORS AND INSTRUMENTATION FOR ASTRONOMY VIII SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII CY JUN 28-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE SIS receiver; Submillimeter receiver; wideband receiver; Local Oscillator; beam alignment; receiver commissioning AB We report on the design of a 240 GHz double-side-band receiver for the Submillimeter Array (SMA). The heart of this receiver is a 3-junction series connected SIS mixer, which allows it to provide intermediate frequency (IF) output up to more than 12 GHz. We have custom built a low noise Amplifier-Multiplier Chain for use as the receiver's Local Oscillator module, which is tunable from 210 to 270 GHz. The receiver has demonstrated low noise performance in laboratory. 7 out of the 8 SMA antennas are now equipped with this receiver. The receiver has already participated in Event Horizon Telescope observations in April 2016, working with the SMA-200 receiver to provide dual polarization coverage for the EHT Hawaii Station. This receiver has enabled the SMA to provide 32 Gbit per second data stream to the EHT observations. We are currently trying to improve the on-sky beam co-alignment of this receiver with respect to other SMA receivers. C1 [Tong, C. -Y. Edward; Grimes, Paul K.; Leiker, Patrick S.; Zeng, Lingzhen] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Lu, Wei-Chun; Chen, Tse-Jun; Han, Chih-Chiang; Wang, Ming-Jye] Acad Sinica, Inst Astron & Astrophys, Taipei, Taiwan. RP Tong, CYE (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM etong@cfa.harvard.edu OI Tong, Edward/0000-0002-7736-4203 NR 8 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0207-6; 978-1-5106-0208-3 J9 PROC SPIE PY 2016 VL 9914 AR UNSP 99140F DI 10.1117/12.2232776 PN 1 PG 7 WC Astronomy & Astrophysics; Optics SC Astronomy & Astrophysics; Optics GA BF9PQ UT WOS:000385793800009 ER PT S AU Gaskin, J Ozel, F Vikhlinin, A AF Gaskin, Jessica Ozel, Feryal Vikhlinin, Alexey CA X-Ray Surveyor STDT BE MacEwen, HA Fazio, GG Lystrup, M TI The X-Ray Surveyor Mission Concept Study: Forging the Path to NASA Astrophysics 2020 Decadal Survey Prioritization SO SPACE TELESCOPES AND INSTRUMENTATION 2016: OPTICAL, INFRARED, AND MILLIMETER WAVE SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Space Telescopes and Instrumentation - Optical, Infrared, and Millimeter Wave CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE X-Ray Surveyor; X-Ray Astronomy; NASA Astrophysics Mission Concept Study AB The X-Ray Surveyor mission concept is unique among those being studied for prioritization in the NASA Astrophysics 2020 Decadal Survey. The X-Ray Surveyor mission will explore the high-energy Universe; providing essential and complimentary observations to the Astronomy Community. The NASA Astrophysics Roadmap (Enduring Quests, Daring Visions) describes the need for an X-Ray Observatory that is capable of addressing topics such as the origin and growth of the first supermassive black holes, galaxy evolution and growth of the cosmic structure, and the origin and evolution of the stars that make up our Universe. To address these scientifically compelling topics and more, an Observatory that exhibits leaps in capability over that of previous X-Ray Observatories in needed. This paper describes the current status of the X-Ray Surveyor Mission Concept Study and the path forward, which includes scientific investigations, technology development, and community participation. C1 [Gaskin, Jessica] NASA, Marshall Space Flight Ctr, Huntsville, AL 35812 USA. [Ozel, Feryal] Univ Arizona, Dept Astron, 933 N Cherry Ave, Tucson, AZ 85721 USA. [Vikhlinin, Alexey] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA. RP Gaskin, J (reprint author), NASA, Marshall Space Flight Ctr, Huntsville, AL 35812 USA. EM Jessica.Gaskin@nasa.gov NR 14 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0187-1; 978-1-5106-0188-8 J9 PROC SPIE PY 2016 VL 9904 AR UNSP 99040N DI 10.1117/12.2240459 PG 7 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BF9PT UT WOS:000385794100020 ER PT S AU Matthews, GW Egerman, R Morse, JA Wilkes, B AF Matthews, Gary W. Egerman, Robert Morse, Jon A. Wilkes, Belinda BE MacEwen, HA Fazio, GG Lystrup, M TI ASTRO-1, a 1.8m unobscured space observatory for next generation UV/visible astrophysics and exoplanet exploration SO SPACE TELESCOPES AND INSTRUMENTATION 2016: OPTICAL, INFRARED, AND MILLIMETER WAVE SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Space Telescopes and Instrumentation - Optical, Infrared, and Millimeter Wave CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Lightweight Mirrors; Optical Systems; UV Systems AB The Hubble Space Telescope has been a scientific marvel that has provided remarkable imagery and scientific discovery. Its exquisite UV-Visible imaging performance is unmatched from the ground. In NASA's future planning, the earliest possible successor mission would be in the 2030s, well beyond the expected lifetime of Hubble. The ASTRO-1 space telescope is a 1.8m off-axis (unobscured) observatory that looks to fill this critical void with Hubble-like performance to continue the scientific quest while also providing the possibility for exoplanet research with a coronagraphic instrument and/or a free flying starshade. BoldlyGo Institute seeks to reach beyond NASA funding to leverage the high public interest in space research and exploration, and the search for life beyond Earth. C1 [Matthews, Gary W.; Egerman, Robert] Harris, Melbourne, FL 32919 USA. [Morse, Jon A.] BoldlyGo Inst, Albany, NY USA. [Wilkes, Belinda] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Matthews, GW (reprint author), Harris, Melbourne, FL 32919 USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0187-1; 978-1-5106-0188-8 J9 PROC SPIE PY 2016 VL 9904 AR UNSP 99041J DI 10.1117/12.2232021 PG 6 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BF9PT UT WOS:000385794100045 ER PT S AU Meixner, M Cooray, A Carter, R DiPirro, M Flores, A Leisawitz, D Armus, L Battersby, C Bergin, E Bradford, CM Ennico, K Melnick, GJ Milam, S Narayanan, D Pontoppidan, K Pope, A Roellig, T Sandstrom, K Su, KYL Vieira, J Wright, E Zmuidzinas, J Alato, S Carey, S Gerin, M Helmich, F Menten, K Scott, D Sakon, I Vavrek, R AF Meixner, M. Cooray, A. Carter, R. DiPirro, M. Flores, A. Leisawitz, D. Armus, L. Battersby, C. Bergin, E. Bradford, C. M. Ennico, K. Melnick, G. J. Milam, S. Narayanan, D. Pontoppidan, K. Pope, A. Roellig, T. Sandstrom, K. Su, K. Y. L. Vieira, J. Wright, E. Zmuidzinas, J. Alato, S. Carey, S. Gerin, M. Helmich, F. Menten, K. Scott, D. Sakon, I. Vavrek, R. BE MacEwen, HA Fazio, GG Lystrup, M TI The Far-Infrared Surveyor Mission Study: Paper I, the Genesis SO SPACE TELESCOPES AND INSTRUMENTATION 2016: OPTICAL, INFRARED, AND MILLIMETER WAVE SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Space Telescopes and Instrumentation - Optical, Infrared, and Millimeter Wave CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE ID ASTRONOMY AB This paper describes the beginning of the Far-Infrared Surveyor mission study for NASA's Astrophysics Decadal 2020. We describe the scope of the study, and the open process approach of the Science and Technology Definition Team. We are currently developing the science cases and provide some preliminary highlights here. We note key areas for technological innovation and improvements necessary to make a Far-Infrared Surveyor mission a reality. C1 [Meixner, M.; Pontoppidan, K.] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA. [Meixner, M.] Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA. [Cooray, A.] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA USA. [Carter, R.; DiPirro, M.; Flores, A.; Leisawitz, D.; Milam, S.] NASA, Goddard Space Flight Ctr, 8800 Greenbelt Rd, Greenbelt, MD 20771 USA. [Armus, L.; Carey, S.] NASA, Infrared Proc & Anal Ctr, Pasadena, CA USA. [Battersby, C.; Melnick, G. J.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Bergin, E.] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA. [Bradford, C. M.] NASA, Jet Prop Lab, Pasadena, CA USA. [Ennico, K.; Roellig, T.] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA. [Narayanan, D.] Univ Florida, Gainesville, FL USA. [Pope, A.] Univ Massachusetts, Dept Astron, LGRT B 619E, Amherst, MA 01003 USA. [Sandstrom, K.] Univ Calif San Diego, La Jolla, CA 92093 USA. [Su, K. Y. L.] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA. [Vieira, J.] Univ Illinois, Urbana, IL 61801 USA. [Wright, E.] Univ Calif Los Angeles, Los Angeles, CA USA. [Zmuidzinas, J.] CALTECH, Pasadena, CA 91125 USA. [Alato, S.] SNSB, Stockholm, Sweden. [Gerin, M.] CNES, Paris, France. [Helmich, F.] SRON, Utrecht, Netherlands. [Menten, K.] DLR, Cologne, Germany. [Scott, D.] Chinese Acad Sci, Beijing, Peoples R China. [Sakon, I.] JAXA, Chofu, Tokyo, Japan. [Vavrek, R.] ESA, Paris, France. RP Meixner, M (reprint author), Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA.; Meixner, M (reprint author), Johns Hopkins Univ, Dept Phys & Astron, 3400 N Charles St, Baltimore, MD 21218 USA. EM meixner@stsci.edu NR 9 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0187-1; 978-1-5106-0188-8 J9 PROC SPIE PY 2016 VL 9904 AR UNSP 99040K DI 10.1117/12.2240456 PG 8 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BF9PT UT WOS:000385794100018 ER PT S AU Ricker, GR Vanderspek, H Winn, J Seager, S Berta-Thompson, Z Levine, A Villasenor, J Latham, D Charbonneau, D Holman, M Johnson, J Sasselov, D Szentgyorgyi, A Torres, G Bakos, G Brown, T Christensen-Dalsgaard, J Kjeldsen, H Clampin, M Rinehart, S Deming, D Doty, J Dunham, E Ida, S Kawai, N Sato, B Jenkins, J Lissauer, J Jernigan, G Kaltenegger, L Laughlin, G Lin, D McCullough, P Narita, N Pepper, J Stassun, K Udry, S AF Ricker, G. R. Vanderspek, H. Winn, J. Seager, S. Berta-Thompson, Z. Levine, A. Villasenor, J. Latham, D. Charbonneau, D. Holman, M. Johnson, J. Sasselov, D. Szentgyorgyi, A. Torres, G. Bakos, G. Brown, T. Christensen-Dalsgaard, J. Kjeldsen, H. Clampin, M. Rinehart, S. Deming, D. Doty, J. Dunham, E. Ida, S. Kawai, N. Sato, B. Jenkins, J. Lissauer, J. Jernigan, G. Kaltenegger, L. Laughlin, G. Lin, D. McCullough, P. Narita, N. Pepper, J. Stassun, K. Udry, S. BE MacEwen, HA Fazio, GG Lystrup, M TI The Transiting Exoplanet Survey Satellite SO SPACE TELESCOPES AND INSTRUMENTATION 2016: OPTICAL, INFRARED, AND MILLIMETER WAVE SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Space Telescopes and Instrumentation - Optical, Infrared, and Millimeter Wave CY JUN 26-JUL 01, 2016 CL Edinburgh, SCOTLAND SP SPIE DE Exoplanet; extrasolar planet; photometry; satellite; transit ID PLANETS; KEPLER; STARS; TELESCOPE; CATALOG; SYSTEMS AB The Transiting Exoplanet Survey Satellite (TESS) will search the solar neighborhood for planets transiting bright stars. TESS has been selected by NASA for launch in 2017 as an Astrophysics Explorer mission. The spacecraft will be placed into a highly elliptical 13.7-day orbit around the Earth. During its two-year mission, TESS will employ four wide-field optical CCD cameras to monitor at least 200,000 main-sequence dwarf stars with I-C less than or similar to 13 for temporary drops in brightness caused by planetary transits. Each star will be observed for an interval ranging from one month to one year, depending on the star's ecliptic latitude. The longest observing intervals will be for stars near the ecliptic poles, which are the optimal locations for follow-up observations with the James Webb Space Telescope. Brightness measurements of preselected target stars will be recorded every 2 min, and full frame images will be recorded every 30 min. TESS stars will be 10-100 times brighter than those surveyed by the pioneering Kepler mission. This will make TESS planets easier to characterize with follow-up observations. TESS is expected to find more than a thousand planets smaller than Neptune, including dozens that are comparable in size to the Earth. Public data releases will occur every four months, inviting immediate community- wide efforts to study the new planets. The TESS legacy will be a catalog of the nearest and brightest stars hosting transiting planets, which will endure as highly favorable targets for detailed investigations. C1 [Ricker, G. R.; Vanderspek, H.; Winn, J.; Seager, S.; Berta-Thompson, Z.; Levine, A.; Villasenor, J.] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Latham, D.; Charbonneau, D.; Holman, M.; Johnson, J.; Sasselov, D.; Szentgyorgyi, A.; Torres, G.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Bakos, G.] Princeton Univ, Princeton, NJ 08544 USA. [Brown, T.] Las Cumbres Observ Global Telescope, Goleta, CA 93117 USA. [Christensen-Dalsgaard, J.; Kjeldsen, H.] Aarhus Univ, Stellar Astrophys Ctr, DK-8000 Aarhus C, Denmark. [Clampin, M.; Rinehart, S.] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. [Deming, D.] Univ Maryland, College Pk, MD 20742 USA. [Doty, J.] Noqsi Aerosp Ltd, Pine, CO 80470 USA. [Dunham, E.] Lowell Observ, 1400 W Mars Hill Rd, Flagstaff, AZ 86001 USA. [Ida, S.; Kawai, N.; Sato, B.] Tokyo Inst Technol, Meguro Ku, Tokyo 1528550, Japan. [Jenkins, J.; Lissauer, J.] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA. [Jernigan, G.] UCB, Space Sci Lab, Berkeley, CA 94720 USA. [Kaltenegger, L.] Cornell Univ, Ithaca, NY 14850 USA. [Laughlin, G.; Lin, D.] UCO, Lick Observ, Santa Cruz, CA 95064 USA. [McCullough, P.] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA. [McCullough, P.] Johns Hopkins Univ, Baltimore, MD 21218 USA. [Narita, N.] Natl Astron Observ Japan, Mitaka, Tokyo, Japan. [Pepper, J.] Lehigh Univ, Bethlehem, PA 18015 USA. [Stassun, K.] Vanderbilt Univ, 221 Kirkland Hall, Nashville, TN 37235 USA. [Stassun, K.] Fisk Univ, Nashville, TN 37235 USA. [Udry, S.] Observ Genve, CH-1290 Versoix, Switzerland. RP Ricker, GR (reprint author), MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA. EM grr@space.mit.edu OI Pepper, Joshua/0000-0002-3827-8417 NR 48 TC 0 Z9 0 U1 0 U2 0 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0187-1; 978-1-5106-0188-8 J9 PROC SPIE PY 2016 VL 9904 AR UNSP 99042B DI 10.1117/12.2232071 PG 18 WC Instruments & Instrumentation; Optics SC Instruments & Instrumentation; Optics GA BF9PT UT WOS:000385794100066 ER PT J AU Issawi, B Youssef, EAA Maxwell, T AF Issawi, Bahay Youssef, El Sayed A. A. Maxwell, Ted TI Cenozoic rivers of northeast Africa: Evidence of trans-Saharan drainage SO STRATIGRAPHY LA English DT Article DE Cenozoic; Paleohydrology; Africa; Trans-Saharan Drainage; Radar Rivers ID SELIMA SAND SHEET; EASTERN SAHARA; ACHEULIAN SITES; LATE QUATERNARY; URANIUM-SERIES; SOUTHERN EGYPT; RADAR RIVERS; BASIN; MIOCENE; SYSTEM AB Radar imagery of the Sahara of Egypt and eastern Libya has dramatically changed previous concepts in regard to long term aridity of this region, revealing an extensive network of buried fluvial channels documenting the river systems that developed in the proto-Sahara during the Late Paleogene and Neogene, following the early Eocene regression of the Mediterranean Sea, and prior to Pleistocene aridification. The fall in base level associated with the end-Miocene Messinian desiccation of the Mediterranean led to deep down-cutting and extension of river systems throughout much of North Africa and South Europe. The deep, infilled canyons beneath the modern Rhone and Nile are well known, but the radar imagery identifies other deep canyons under the North African Sahara that are now invisible. In eastern Libya, drainage from Serir Tebisti (Tebisti Massif) into the Mediterranean via the Sirt Basin was channeled by two main rivers, the Sahabi in the west and the Kufra in the east; these were subsequently united in the Early Pliocene when the latter captured the former. The Gilf River was another important channel that drained north from the Uweinat-Gilf highland in southwest Egypt, in a system that may have been connected with the Kufra during the Neogene and enabling fish to move from the presently isolated Chad Basin to northern Libya and Egypt. The interplay of these north-flowing rivers and the constant northward retreat of the Mediterranean shoreline from Oligocene onward resulted in deposits of fluvial and marine sedimentation in every possible combinaton that have been described by many authors in the region between the Tebisti and the present Mediterranean shoreline. Prior to the establishment of the Nile, a southwestward drainage, the Qena River, was initiated by Oligocene uplift and lateral faulting along the Red Sea shoulder of the East African Rift. This river discharged into a distributive network known as the Radar Rivers near latitude 23 degrees 30'N in the Southwestern Desert. It has been suggested that waters from the Qena River continued to flow southwestward to the Atlantic Ocean, in what is known as Trans African Drainage System (TADS). C1 [Issawi, Bahay] 16 El Mesaha St, Giza, Egypt. [Youssef, El Sayed A. A.] Cairo Univ, Fac Sci, Dept Geol, POB 12613, Cairo, Egypt. [Maxwell, Ted] Smithsonian Natl Air & Space Museum, 600 Independence Ave SW, Washington, DC 20560 USA. RP Issawi, B (reprint author), 16 El Mesaha St, Giza, Egypt. EM bissawi@yahoo.com NR 128 TC 1 Z9 1 U1 4 U2 4 PU MICRO PRESS PI FLUSHING PA 6530 KISSENA BLVD, FLUSHING, NY 11367 USA SN 1547-139X J9 STRATIGRAPHY JI Stratigraphy PY 2016 VL 13 IS 1 BP 49 EP 66 PG 18 WC Geology; Paleontology SC Geology; Paleontology GA DZ0ND UT WOS:000385536100003 ER PT J AU Ng, PKL Meyer, C AF Ng, Peter K. L. Meyer, Chistopher TI A new species of pea crab of the genus Serenotheres Ahyong & Ng, 2005 (Crustacea, Brachyura, Pinnotheridae) from the date mussel Leiosolenus Carpenter, 1857 (Mollusca, Bivalvia, Mytilidae, Lithophaginae) from the Solomon Islands SO ZOOKEYS LA English DT Article DE Pinnotheridae; taxonomy; symbiotic crab; new species; symbiotic crab; Serenotheres janus; Solomon Islands AB The pea crab genus Serenotheres Ahyong & Ng, 2005 (Pinnotheridae) is currently only represented by one species, S. besutensis (Serene, 1967). A new species is now assigned to this genus, described from a date mussel Leiosolenus obesus Carpenter, 1857 (Mollusca: Bivalvia: Mytilidae: Lithophaginae) collected in the Solomon Islands. Serenotheres janus sp. n. differs from S. besutensis in possessing a conspicuously broader carapace, with the lateral margins of the dorsal lamellum distinctly produced and the posterolateral part deeply concave, the dorsal lamellum being highest at the median cleft, the rostrum is relatively more prominent, the surfaces of the anterolateral margin and hepatic region are less prominently pitted and eroded, the ischiomerus of the third maxilliped is relatively more rectangular, and the P2 merus is proportionately longer. C1 [Ng, Peter K. L.] Natl Univ Singapore, Lee Kong Chian Nat Hist Museum, Fac Sci, 2 Conservatory Dr, Singapore 117377, Singapore. [Meyer, Chistopher] Smithsonian Inst, US Natl Museum Nat Hist, Dept Invertebrate Zool, Washington, DC 20013 USA. RP Ng, PKL (reprint author), Natl Univ Singapore, Lee Kong Chian Nat Hist Museum, Fac Sci, 2 Conservatory Dr, Singapore 117377, Singapore. EM peterng@nus.edu.sg NR 11 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 623 BP 31 EP 41 DI 10.3897/zookeys.623.10272 PG 11 WC Zoology SC Zoology GA DY8FS UT WOS:000385364800003 PM 27843386 ER PT B AU Eakle, AJ AF Eakle, A. Jonathan BE Enriquez, G Johnson, E Kontovourki, S Mallozzi, CA TI BODIES WITH AND WITHOUT ORGANS Literacies of a True Crime Sex and Violence Drama SO LITERACIES, LEARNING, AND THE BODY: PUTTING THEORY AND RESEARCH INTO PEDAGOGICAL PRACTICE SE Expanding Literacies in Education LA English DT Article; Book Chapter ID SCHOOL; SPACES C1 [Eakle, A. Jonathan] George Washington Univ, Educ, Washington, DC 20052 USA. [Eakle, A. Jonathan] Smithsonian, Washington, DC 20560 USA. [Eakle, A. Jonathan] Corcoran Sch Arts & Design, Washington, DC 20006 USA. RP Eakle, AJ (reprint author), George Washington Univ, Educ, Washington, DC 20052 USA.; Eakle, AJ (reprint author), Smithsonian, Washington, DC 20560 USA.; Eakle, AJ (reprint author), Corcoran Sch Arts & Design, Washington, DC 20006 USA. NR 32 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE PI ABINGDON PA 2 PARK SQ, MILTON PARK, ABINGDON OX14 4RN, OXFORD, ENGLAND BN 978-1-138-90621-1; 978-1-315-69563-1; 978-1-138-90619-8 J9 EXPAND LITERACIES ED PY 2016 BP 221 EP 235 PG 15 WC Education & Educational Research; Social Sciences, Interdisciplinary SC Education & Educational Research; Social Sciences - Other Topics GA BF7YA UT WOS:000384576300015 ER PT J AU Arellano, G Cala, V Fuentes, A Cayola, L Jorgensen, PM Macia, MJ AF Arellano, G. Cala, V. Fuentes, A. Cayola, L. Jorgensen, P. M. Macia, M. J. TI A STANDARD PROTOCOL FOR WOODY PLANT INVENTORIES AND SOIL CHARACTERISATION USING TEMPORARY 0.1-HA PLOTS IN TROPICAL FORESTS SO JOURNAL OF TROPICAL FOREST SCIENCE LA English DT Article DE Census methods; edaphic assessment; floristic assessment; floristic standardisation; lianas; plant biodiversity; plant-soil relationship ID ELEVATIONAL GRADIENT; BETA-DIVERSITY; RAIN-FOREST; PATTERNS; NETWORK; BOLIVIA AB The use of both uniform woody plant inventories and laboratory soil analysis methods facilitates data sharing and improves the understanding of large-scale biological patterns in tropical forests. Temporary small 0.1-ha plots, fast and cheap to install, are increasingly employed in the tropics. This study presents a standard protocol for woody plant inventories and soil characterisation using 0.1-ha plots. The protocol gives specific recommendations on the size and shape of a 0.1-ha plot, taxa to be included in the inventories, minimum stem diameter cut-offs, evaluation of multiple stems and height estimation. In addition, we present a number of recommendations on soil sampling and analysis, whose standarisation is much required in tropical forest research. We suggest to measure Al and nutrients simultaneously after Mehlich-3 extraction, followed by inductively coupled plasma spectrometry, and to measure C and N through total combustion. The pH, texture and bulk density can be measured with standard manual methods. The study also includes guidelines to create and maintain a standardised database and metadata. All the proposed recommendations are compatible with those already employed in the standardised establishment of large plots. Each recommendation represents a reasonable trade-off between investment and data quality and is oriented to obtain low-cost standardised baseline data, useful to a broad range of studies. C1 [Arellano, G.] Smithsonian Trop Res Inst, Ctr Trop Forest Sci ForestGEO, NMNH Constitut Av & 10th St NW, Washington, DC 20521 USA. [Arellano, G.; Macia, M. J.] Univ Autonoma Madrid, Dept Biol, Area Bot, Calle Darwin 2, ES-28049 Madrid, Spain. [Cala, V.] Univ Autonoma Madrid, Dept Geol & Geoquim, ES-28049 Madrid, Spain. [Fuentes, A.; Cayola, L.] Univ Mayor San Andres, Herbario Nacl Bolivia, Casilla 10077 Correo Cent, La Paz, Bolivia. [Jorgensen, P. M.] Missouri Bot Garden, POB 299, St Louis, MO USA. RP Arellano, G (reprint author), Smithsonian Trop Res Inst, Ctr Trop Forest Sci ForestGEO, NMNH Constitut Av & 10th St NW, Washington, DC 20521 USA.; Arellano, G (reprint author), Univ Autonoma Madrid, Dept Biol, Area Bot, Calle Darwin 2, ES-28049 Madrid, Spain. EM gabriel.arellano.torres@gmail.com RI Macia, Manuel/H-4631-2012 OI Macia, Manuel/0000-0002-4676-612X FU European Union (INCO-DC) [IC18-CT960038]; Consejeria de Educacion; Comunidad Autonoma de Madrid; National Geographic Society [8047-06, 7754-04]; National Science Foundation (DEB) [0101775, 0743457]; Centro de Estudios de America Latina, Universidad Autonoma de Madrid, Banco Santander FX The authors thank M Lohbeck, NG Swenson, M Pena-Claros, J Powers, C Baraloto and S Rifkin. The work was funded by the European Union (INCO-DC, IC18-CT960038), Consejeria de Educacion, Comunidad Autonoma de Madrid, National Geographic Society (8047-06, 7754-04), National Science Foundation (DEB#0101775, DEB#0743457) and Centro de Estudios de America Latina, Universidad Autonoma de Madrid, Banco Santander. NR 46 TC 0 Z9 0 U1 1 U2 1 PU FOREST RESEARCH INST MALAYSIA PI KUALA LUMPUR PA PUBLICATION UNIT, KEPONG, KUALA LUMPUR 52109, MALAYSIA SN 0128-1283 J9 J TROP FOR SCI JI J. Trop. For. Sci. PY 2016 VL 28 IS 4 BP 508 EP 516 PG 9 WC Forestry SC Forestry GA DX9JO UT WOS:000384711100013 ER PT J AU Doherty, T Ingalls, H Kerr, A Maynor, C Umberger, L AF Doherty, Tiarna Ingalls, Helen Kerr, Amber Maynor, Catherine Umberger, Leslie TI Conserving the self-taught artists collection at the Smithsonian American Art Museum SO STUDIES IN CONSERVATION LA English DT Article DE Self-taught artists; African American; James Hampton; Purvis Young; Mingering Mike AB Evolving curatorial frameworks for art beyond the mainstream have influenced how conservators approach preservation and degrees of intervention. Unconventional materials and techniques, along with inconsistent or compromised care during the artist's lifetime necessitate artist-specific materials knowledge and a curatorial perspective that considers the artist's historical lack of agency as a factor in preservation strategies. C1 [Doherty, Tiarna; Ingalls, Helen; Kerr, Amber; Maynor, Catherine; Umberger, Leslie] Smithsonian Amer Art Museum, MRC 970 POB 37012, Washington, DC 20013 USA. RP Doherty, T (reprint author), Smithsonian Amer Art Museum, MRC 970 POB 37012, Washington, DC 20013 USA. EM dohertyt@si.edu NR 9 TC 0 Z9 0 U1 1 U2 1 PU ROUTLEDGE JOURNALS, TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0039-3630 EI 2047-0584 J9 STUD CONSERV JI Stud. Conserv. PY 2016 VL 61 SU 2 SI SI BP 38 EP 43 DI 10.1080/00393630.2016.1188616 PG 6 WC Archaeology; Art; Chemistry, Applied; Chemistry, Analytical; Spectroscopy SC Archaeology; Art; Chemistry; Spectroscopy GA DX5ZU UT WOS:000384462200009 ER PT J AU Hornbeck, SE Moffett, DL AF Hornbeck, Stephanie E. Moffett, Dana L. TI Altered surfaces, taking the long view: Applications of ethnographic conservation practices to the conservation of contemporary art SO STUDIES IN CONSERVATION LA English DT Article DE African art; Ethnographic conservation; Surface alteration; Minimal intervention; Artistic intent; Contemporary art AB While working together on tradition-based and contemporary works at the Smithsonian's National Museum of African Art (NMAfA) and in private practice, the authors found that their expertise in ethnographic conservation can be applied to the conservation of contemporary works. The treatment approach to ethnographic works has evolved over decades, shifting from alteration of original surfaces and heavy restoration to an emphasis on preserving the original integrity of the artwork through minimal intervention. This paper describes the evolution of ethnographic object conservation regarding surface alteration, while specifically focusing on African objects, and discusses applications of this approach to the conservation of contemporary art. The historical change in treatment attitudes is presented using examples from NMAfA's collections to underscore why the profession developed a minimal intervention approach and to argue for the relevance of this approach to related contemporary media. C1 [Hornbeck, Stephanie E.] Caryatid Conservat Serv Inc, 500 NE 29th St,606, Miami, FL 33137 USA. [Moffett, Dana L.] Smithsonian Inst, Natl Museum African Art, Washington, DC 20560 USA. RP Hornbeck, SE (reprint author), Caryatid Conservat Serv Inc, 500 NE 29th St,606, Miami, FL 33137 USA. EM shornbeck@caryatid-conservation.com NR 9 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE JOURNALS, TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0039-3630 EI 2047-0584 J9 STUD CONSERV JI Stud. Conserv. PY 2016 VL 61 SU 2 SI SI BP 84 EP 90 DI 10.1080/00393630.2016.1190906 PG 7 WC Archaeology; Art; Chemistry, Applied; Chemistry, Analytical; Spectroscopy SC Archaeology; Art; Chemistry; Spectroscopy GA DX5ZU UT WOS:000384462200015 ER PT J AU McHugh, K Gunnison, A AF McHugh, Kelly Gunnison, Anne TI Finding common ground and inherent differences: Artist and community engagement in cultural material and contemporary art conservation SO STUDIES IN CONSERVATION LA English DT Article DE Ethnographic objects; Cultural material; Contemporary art; Consultations; Interviews; National Museum of the American Indian; Yale University Art Gallery AB Comparisons are often made between the conservation of cultural material collections, often described as ethnographic, and contemporary art collections, and indeed there are significant parallels. The stewardship of both of these types of collections can challenge traditional tenets of conservation, requiring conservators to ask themselves 'What are we preserving?' as preservation extends beyond the physical. The work must be placed in a broader conceptual context and the conservator must seek out those who are deemed to have the most authority - whether it is the artist, the artist's assistants and estate or the source community - to establish this context. Engagement with constituents creates valuable reciprocal relationships, which can benefit the artist, community, and museum. The relationships and the parallel practice of two seemingly disparate fields are examined using examples from the National Museum of the American Indian (NMAI) and the Yale University Art Gallery (YUAG). Conservators at NMAI, a living culture museum containing archeological, historic, and contemporary art collections, are in the unique position of working with community stakeholders with direct ties to historic collections and contemporary artists whose work is actively acquired by the museum. Conservators at YUAG, an encyclopedic museum with a pedagogical directive, are attempting to establish a more rigorous program of artist engagement to direct preservation and understanding of contemporary art collections. C1 [McHugh, Kelly] Smithsonian Inst, Natl Museum Amer Indian, Washington, DC 20560 USA. [Gunnison, Anne] Yale Univ Art Gallery, New Haven, CT 06510 USA. RP Gunnison, A (reprint author), Yale Univ Art Gallery, New Haven, CT 06510 USA. EM anne.gunnison@yale.edu NR 11 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE JOURNALS, TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0039-3630 EI 2047-0584 J9 STUD CONSERV JI Stud. Conserv. PY 2016 VL 61 SU 2 SI SI BP 126 EP 129 DI 10.1080/00393630.2016.1181349 PG 4 WC Archaeology; Art; Chemistry, Applied; Chemistry, Analytical; Spectroscopy SC Archaeology; Art; Chemistry; Spectroscopy GA DX5ZU UT WOS:000384462200022 ER PT J AU Kovalchuk, O Ferraris, CJ AF Kovalchuk, Oleksandr Ferraris, Carl J. TI Late Cenozoic catfishes of Southeastern Europe with inference to their taxonomy and palaeogeography SO PALAEONTOLOGIA ELECTRONICA LA English DT Article DE Clariidae; Siluridae; new species; late Miocene; Pliocene; Pleistocene ID MIOCENE; SILURIFORMES; VEGETATION; MOLDOVA; SILURUS; FISHES AB We describe fossil catfish (Siluriformes) material from late Miocene through Pleistocene strata of Southeastern Europe. The material under study is represented by disarticulated bones from 26 localities in the territory of Southern Ukraine and the Russian Federation. Catfish fossils in that region are represented by members of two genera, Heterobranchus and Silurus, of two families (Clariidae and Siluridae, respectively), and five species, including one as new for science (Silurus spinosus n. sp.) and two described in open nomenclature (Silurus cf. S. glanis, Silurus sp.). The presence of dagger Heterobranchus austriacus in the late Sarmatian of Southern Ukraine can be explained by expansion of this species from Africa to Europe during the late Miocene (earlier remains of this taxon were documented only in Central and Western Europe). Geographic distribution of Silurus soldatovi was broader in the past as indicated by the numerous findings of its bones in the late Miocene and Pliocene deposits of Southeastern Europe. Modern Silurus glanis first appeared during the final stage of late Miocene (Pontian) and probably supplanted S. soldatovi because of its wider ecological plasticity (especially temperature tolerance - this species can spawn in cooler waters). An interesting evolutionary trend has been observed in the change of size, shape and orientation of denticulations on the shaft of pectoral-fin spine in different species of the genus Silurus. Such tendency may be explained in terms of the oligomerization of homologous structures, but this question deserves a special study and is not addressed herein. C1 [Kovalchuk, Oleksandr] Natl Acad Sci Ukraine, Dept Paleontol, Natl Museum Nat Hist, 15 Bogdan Khmelnitsky Str, UA-01601 Kiev, Ukraine. [Ferraris, Carl J.] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20560 USA. [Ferraris, Carl J.] 545 NE Floral Pl, Portland, OR 97232 USA. RP Kovalchuk, O (reprint author), Natl Acad Sci Ukraine, Dept Paleontol, Natl Museum Nat Hist, 15 Bogdan Khmelnitsky Str, UA-01601 Kiev, Ukraine. EM biologiest@ukr.net; carlferraris@comcast.net NR 56 TC 0 Z9 0 U1 1 U2 1 PU COQUINA PRESS PI AMHERST PA C/O WHITEY HAGADORN, EXECUTIVE EDITOR, AMHERST COLLEGE, DEPT GEOLOGY, AMHERST, MA 01002 USA SN 1935-3952 EI 1094-8074 J9 PALAEONTOL ELECTRON JI Palaeontol. electron. PY 2016 VL 19 IS 3 AR 34A PG 17 WC Paleontology SC Paleontology GA DX1QB UT WOS:000384140900003 ER PT J AU Boeve, JL Marin-Armijos, DS Dominguez, DF Smith, DR AF Boeve, Jean-Luc Marin-Armijos, Diego S. Dominguez, Diego F. Smith, David R. TI Sawflies (Hymenoptera: Argidae, Pergidae, Tenthredinidae) from southern Ecuador, with a new record for the country and some ecological data SO JOURNAL OF HYMENOPTERA RESEARCH LA English DT Article DE Species list; paramo; host plant; Fuchsia; Lagideus; larva; defence behaviour ID SYMPHYTA; AMERICA AB An illustrated list of species of sawflies collected during 2014 and 2015 in southern Ecuador is given. One genus and species, Pristiphora fernandezi Smith (Tenthredinidae), is new for the country. Ecological data are provided for Lagideus podocarpus Smith, sp. n. (Pergidae) that was observed feeding on Fuchsia vulcanica L. (Onagraceae). Three new combinations are proposed: Bolivius notabilis (Konow, 1899), Plaumanniana biclinea (Konow, 1899), and Proselandria alvina (Konow, 1899) (Tenthredinidae: Selandriinae). C1 [Boeve, Jean-Luc] Royal Belgian Inst Nat Sci, OD Taxon & Phylogeny, Rue Vautier 29, B-1000 Brussels, Belgium. [Marin-Armijos, Diego S.; Dominguez, Diego F.] Univ Tecn Particular Loja, Dept Ciencias Nat, Museo Colecciones Biol, San Cayetano Alto S-N, Loja, Ecuador. [Smith, David R.] ARS, Systemat Entomol Lab, USDA, Natl Museum Nat Hist,Smithsonian Inst, POB 37012,MRC 168, Washington, DC 20013 USA. RP Boeve, JL (reprint author), Royal Belgian Inst Nat Sci, OD Taxon & Phylogeny, Rue Vautier 29, B-1000 Brussels, Belgium. EM jean-luc.boeve@naturalsciences.be FU Belgian Directorate-General for Development Cooperation FX Thibaut Delsinne is warmly thanked for the identification of ants, and for providing a significant amount of specimens and several pictures. We thank Alain Pauly (RBINS, Brussels) who also provided us with specimens, Hugo Omar Cabrera (Herbario UTPL) for the identification of plants, Ximena Cueva and Carlos Ruiz Carreira (MUTPL) for attending some field trips, and M. Reynders (Botanical Garden Meise, Belgium) for providing Fuchsia plants, as well as the subject editor Marko Prous, and the reviewers Stefan Schmidt and Andrew Liston for comments on the manuscript. D. R. Smith thanks A. Taeger (SDEI) for allowing study of Konow's type material. The GTI project was managed in collaboration with C. R. Carreira and David Donoso (MUTPL) and funded by the Belgian Directorate-General for Development Cooperation. Permits were obtained from the Ministerio del Ambiente Loja, Ecuador. NR 20 TC 0 Z9 0 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1070-9428 EI 1314-2607 J9 J HYMENOPT RES JI J. Hymenopt. Res. PY 2016 VL 51 BP 55 EP 89 DI 10.3897/jhr.51.9830 PG 35 WC Entomology SC Entomology GA DW1EN UT WOS:000383385900002 ER PT J AU Seeger, A AF Seeger, Anthony TI Hopi Katsina Songs SO KIVA-JOURNAL OF SOUTHWESTERN ANTHROPOLOGY AND HISTORY LA English DT Book Review C1 [Seeger, Anthony] Univ Calif Los Angeles, Ethnomusicol Emeritus, Los Angeles, CA 90024 USA. [Seeger, Anthony] Smithsonian Folkways Recordings, Washington, DC 20024 USA. RP Seeger, A (reprint author), Univ Calif Los Angeles, Ethnomusicol Emeritus, Los Angeles, CA 90024 USA.; Seeger, A (reprint author), Smithsonian Folkways Recordings, Washington, DC 20024 USA. EM aseeger@arts.ucla.edu NR 1 TC 0 Z9 0 U1 0 U2 0 PU ROUTLEDGE JOURNALS, TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0023-1940 EI 2051-6177 J9 KIVA JI Kiva PY 2016 VL 82 IS 2 BP 207 EP 208 PG 2 WC Archaeology SC Archaeology GA DW0VJ UT WOS:000383360800007 ER PT J AU Wood, KR Appelhans, MS Wagner, WL AF Wood, Kenneth R. Appelhans, Marc S. Wagner, Warren L. TI Melicope oppenheimeri, section Pelea (Rutaceae), a new species from West Maui, Hawaiian Islands: with notes on its ecology, conservation, and phylogeneticplacement SO PHYTOKEYS LA English DT Article DE Rutaceae; Melicope; M. section Pelea; new species; Hawaiian Islands; West Maui; Critically Endangered ID EXTINCTIONS; SAPINDALES; PHYLOGENY; PATTERNS; RECORD; KAUAI AB Melicope oppenheimeri K.R. Wood, Appelhans & W.L. Wagner (section Pelea (A. Gray) Hook. f., Rutaceae), a rare endemic tree from West Maui, Hawaiian Islands, is described and illustrated with notes on its ecology, conservation, and phylogenetic placement. The new species differs from Hawaiian congeners by its carpels basally connate 1/5, narrowed into a strongly reflexed beak 10-15 mm long. It also differs in a combination of leaves with 7-10 pair of secondary veins; cymes to 3 cm long; peduncles 5-6.5 mm long; flowers perfect; capsules 4-9 x 40-52 mm; and a densely appressed short-sericeous ovary. Melicope oppenheimeri is known only from an isolated cliff-base plateau in upper Waihe'e Valley, West Maui. Its discovery brings the number of recognized Melicope J.R. Forst. & G. Forst. species in the Hawaiian Islands to 49. A table is included indicating the conservation status of Hawaiian Melicope and Platydesma H. Mann., which is nested within Melicope sect. Pelea. Melicope oppenheimeri falls into the IUCN Critically Endangered (CR) Red List category. C1 [Wood, Kenneth R.] Natl Trop Bot Garden, 3530 Papalina Rd, Kalaheo, HI 96741 USA. [Appelhans, Marc S.] Univ Gottingen, Dept Systemat Bot, Albrecht von Haller Inst Plant Sci, Untere Karspule 2, D-37073 Gottingen, Germany. [Appelhans, Marc S.; Wagner, Warren L.] Smithsonian Inst, Dept Bot, POB 37012, Washington, DC 20013 USA. RP Wood, KR (reprint author), Natl Trop Bot Garden, 3530 Papalina Rd, Kalaheo, HI 96741 USA. EM kwood@ntbg.org NR 27 TC 0 Z9 0 U1 8 U2 8 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 69 BP 51 EP 64 DI 10.3897/phytokeys.69.8844 PG 14 WC Plant Sciences SC Plant Sciences GA DW1DQ UT WOS:000383383600006 ER PT J AU Funk, VA Hind, DJN AF Funk, Vicki A. Hind, D. J. Nicholas TI Typification of species names in Adenocaulon and Eriachaenium (Compositae/Asteraceae, Subfamily Mutisioideae, Tribe Mutisieae, Subtribe Adenocaulinae) SO PHYTOKEYS LA English DT Article DE Asteraceae; Composiate; North; Central and South America; Asia; Asia-America disjunct distribution AB During the course of a recent research project on Adenocaulon and Eriachaenium it became apparent that some of the species names had not been typified. In this study we located and designated as much type material as possible for these two genera. We indicate holotypes or lectotypes where appropriate, including one for the type of the genus Adenocaulon. C1 [Funk, Vicki A.] Smithsonian Inst, NMNH, Dept Bot, POB 37012, Washington, DC 20013 USA. [Hind, D. J. Nicholas] Royal Bot Gardens, Herbarium, Richmond TW9 3AE, Surrey, England. RP Funk, VA (reprint author), Smithsonian Inst, NMNH, Dept Bot, POB 37012, Washington, DC 20013 USA. EM funkv@si.edu NR 26 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 69 BP 121 EP 128 DI 10.3897/phytokeys.69.9779 PG 8 WC Plant Sciences SC Plant Sciences GA DW1DQ UT WOS:000383383600010 ER PT S AU Farfurnik, D Jarmola, A Pham, LM Wang, ZH Dobrovitski, VV Walsworth, RL Budker, D Bar-Gill, N AF Farfurnik, D. Jarmola, A. Pham, L. M. Wang, Z. H. Dobrovitski, V. V. Walsworth, R. L. Budker, D. Bar-Gill, N. BE Stuhler, J Shields, AJ TI Improving the coherence properties of solid-state spin ensembles via optimized dynamical decoupling SO QUANTUM OPTICS SE Proceedings of SPIE LA English DT Proceedings Paper CT Conference on Quantum Optics CY APR 05-07, 2016 CL Brussels, BELGIUM SP SPIE, Brussels Photon Team, Res Fdn Flanders, Visit Brussels DE nitrogen vacancy; NV; coherence; decoherence; dynamical decoupling; concatenated; XY8; magnetometry ID ELECTRONIC SPIN; DIAMOND SPINS; RESOLUTION; SEQUENCES; CENTERS; TIME; BATH; NMR AB In this work, we optimize a dynamical decoupling (DD) protocol to improve the spin coherence properties of a dense ensemble of nitrogen-vacancy (NV) centers in diamond. Using liquid nitrogen-based cooling and DD microwave pulses, we increase the transverse coherence time T-2 from similar to 0.7 ms up to similar to 30 ms. We extend previous work of single-axis (Carr-Purcell-Meiboom-Gill) DD towards the preservation of arbitrary spin states. After performing a detailed analysis of pulse and detuning errors, we compare the performance of various DD protocols. We identify that the concatenated XY8 pulse sequences serves as the optimal control scheme for preserving an arbitrary spin state. Finally, we use the concatenated sequences to demonstrate an immediate improvement of the AC magnetic sensitivity up to a factor of two at 250 kHz. For future work, similar protocols may be used to increase coherence times up to NV-NV interaction time scales, a major step toward the creation of quantum collective NV spin states. C1 [Farfurnik, D.; Bar-Gill, N.] Hebrew Univ Jerusalem, Racah Inst Phys, IL-9190401 Jerusalem, Israel. [Farfurnik, D.; Bar-Gill, N.] Hebrew Univ Jerusalem, Ctr Nanosci & Nanotechnol, IL-9190401 Jerusalem, Israel. [Jarmola, A.; Budker, D.] Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA. [Pham, L. M.; Walsworth, R. L.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Wang, Z. H.] Univ Southern Calif, Dept Chem, Los Angeles, CA 90089 USA. [Dobrovitski, V. V.] Iowa State Univ, Ames Lab, Ames, IA 50011 USA. [Walsworth, R. L.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Budker, D.] JGU, Helmholtz Inst, Mainz, Germany. [Bar-Gill, N.] Hebrew Univ Jerusalem, Dept Appl Phys, Rachel & Selim Sch Engn, IL-9190401 Jerusalem, Israel. RP Farfurnik, D (reprint author), Hebrew Univ Jerusalem, Racah Inst Phys, IL-9190401 Jerusalem, Israel.; Farfurnik, D (reprint author), Hebrew Univ Jerusalem, Ctr Nanosci & Nanotechnol, IL-9190401 Jerusalem, Israel. NR 39 TC 0 Z9 0 U1 2 U2 2 PU SPIE-INT SOC OPTICAL ENGINEERING PI BELLINGHAM PA 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA SN 0277-786X BN 978-1-5106-0145-1 J9 PROC SPIE PY 2016 VL 9900 AR 99000N DI 10.1117/12.2227479 PG 10 WC Optics; Physics, Applied SC Optics; Physics GA BF6KN UT WOS:000383224000010 ER PT J AU Kayal, E Bentlage, B Collins, AG AF Kayal, Ehsan Bentlage, Bastian Collins, Allen G. TI Insights into the transcriptional and translational mechanisms of linear organellar chromosomes in the box jellyfish Alatina alata (Cnidaria: Medusozoa: Cubozoa) SO RNA BIOLOGY LA English DT Article DE Alatina alata; linear mitochondrial DNA; mitochondrial gene expression; mitochondrial polymerase; tRNA C-to-U editing ID COMPLETE MITOCHONDRIAL GENOME; TARGETING SEQUENCES; PHYLOGENETIC ANALYSIS; DNA-POLYMERASE; TRANSFER-RNAS; EVOLUTION; PROTEINS; MTDNA; IDENTIFICATION; REPLICATION AB Background: In most animals, the mitochondrial genome is characterized by its small size, organization into a single circular molecule, and a relative conservation of the number of encoded genes. In box jellyfish (Cubozoa, Cnidaria), the mitochondrial genome is organized into 8 linear mito-chromosomes harboring between one and 4 genes each, including 2 extra protein-coding genes: mt-polB and orf314. Such an organization challenges the traditional view of mitochondrial DNA (mtDNA) expression in animals. In this study, we investigate the pattern of mitochondrial gene expression in the box jellyfish Alatina alata, as well as several key nuclear-encoded molecular pathways involved in the processing of mitochondrial gene transcription. Results: Read coverage of DNA-seq data is relatively uniform for all 8 mito-chromosomes, suggesting that each mito-chromosome is present in equimolar proportion in the mitochondrion. Comparison of DNA and RNA-seq based assemblies indicates that mito-chromosomes are transcribed into individual transcripts in which the beginning and ending are highly conserved. Expression levels for mt-polB and orf314 are similar to those of other mitochondrial-encoded genes, which provides further evidence for them having functional roles in the mitochondrion. Survey of the transcriptome suggests recognition of the mitochondrial tRNA-Met by the cytoplasmic aminoacyl-tRNA synthetase counterpart and C-to-U editing of the cytoplasmic tRNA-Trp after import into the mitochondrion. Moreover, several mitochondrial ribosomal proteins appear to be lost. Conclusions: This study represents the first survey of mitochondrial gene expression of the linear multi-chromosomal mtDNA in box jellyfish (Cubozoa). Future exploration of small RNAs and the proteome of the mitochondrion will test the hypotheses presented herein. C1 [Kayal, Ehsan; Bentlage, Bastian; Collins, Allen G.] Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, Washington, DC 20560 USA. [Collins, Allen G.] NOAA, Natl Systemat Lab, Fisheries Serv, Natl Museum Nat Hist, Washington, DC USA. RP Kayal, E (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, Washington, DC 20560 USA. EM kayale@si.edu FU Smithsonian Institution Peter Buck postdoctoral fellowship FX Some of this work was performed using resources of the Laboratories of Analytical Biology at the Smithsonian National Museum of Natural History. EK and BB were supported by a Smithsonian Institution Peter Buck postdoctoral fellowship. We also want to thank two anonymous reviewers for providing constructive criticisms to earlier versions of this manuscript. NR 57 TC 0 Z9 0 U1 2 U2 2 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 1547-6286 EI 1555-8584 J9 RNA BIOL JI RNA Biol. PY 2016 VL 13 IS 9 BP 799 EP 809 DI 10.1080/15476286.2016.1194161 PG 11 WC Biochemistry & Molecular Biology SC Biochemistry & Molecular Biology GA DW0UK UT WOS:000383358100008 PM 27267414 ER PT J AU Capa, M Osborn, KJ Bakken, T AF Capa, Maria Osborn, Karen J. Bakken, Torkild TI Sphaerodoridae (Annelida) of the deep Northwestern Atlantic, including remarkable new species of Euritmia and Sphaerephesia SO ZOOKEYS LA English DT Article DE Generic synonymy; Amacrodorum; Ephesiopsis; epithelial tubercles; NW Atlantic; shelf; slope ID CAROLINA CONTINENTAL-SLOPE; POLYCHAETA SPHAERODORIDAE; SPATIAL HETEROGENEITY; DIVERSITY; REVISION; PACIFIC; GENUS AB Sphaerodoridae (Annelida) is a seeming uncommon and minimally diverse group of polychaetes in the northwestern Atlantic, with only seven species reported from the United States, and none from the eastern coast of Canada, before the present study. Review of the large Smithsonian collection (National Museum of Natural History, Washington) revealed the presence of two morphologically extraordinary undescribed species and added a new record to the north-western Atlantic region. Euritmia carolensis sp. n. is characterised by bearing approximately 20 sessile spherical papillae arranged in three transverse rows per segment, ventrum with 4-6 larger papillae near the parapodial bases and parapodia without papillae; bearing 4-5 simple chaetae that are enlarged subdistally. Sphaerephesia amphorata sp. n. is distinguished from other congeners in the presence of four longitudinal rows of sessile, bottle-shaped macrotubercles with exceptionally long digitiform terminal papilla, and parapodia with four rounded and small papillae, bearing 4-7 compound chaetae, with blades 7-11 times as long as wide. Other encountered species are also herein re-described, including intraspecific variation and updated iconography. Comparison of material also allowed some systematic changes in the group, including the synonymisation of the genus Amacrodorum with Euritmia, and the transfer of Ephesiopsis shivae to Ephesiella. A key to the species reported from the Northwestern Atlantic is provided. C1 [Capa, Maria; Bakken, Torkild] Norwegian Univ Sci & Technol, NTNU Univ Museum, NO-7491 Trondheim, Norway. [Osborn, Karen J.] Smithsonian Natl Museum Nat Hist, Dept Invertebrate Zool, 10th & Constitut Ave NW, Washington, DC USA. RP Capa, M (reprint author), Norwegian Univ Sci & Technol, NTNU Univ Museum, NO-7491 Trondheim, Norway. EM maria.capa@ntnu.no OI Osborn, Karen/0000-0002-4226-9257 NR 49 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 615 BP 1 EP 32 DI 10.3897/zookeys.615.9530 PG 32 WC Zoology SC Zoology GA DW1AT UT WOS:000383375800001 ER PT J AU Hiller, A Werding, B AF Hiller, Alexandra Werding, Bernd TI A new species of the genus Petrolisthes Stimpson (Crustacea, Decapoda, Porcellanidae) from the Central Pacific, with remarks and new records for P. aegyptiacus Werding & Hiller SO ZOOKEYS LA English DT Article DE Crustacea; Porcellanidae; Petrolisthes; new species; Indo-West Pacific; species complex; range extension ID ANOMURA PORCELLANIDAE; SOUTHWESTERN JAPAN; RYUKYU ISLANDS; N. SP.; MORPHOLOGY; COLOR AB Petrolisthes paulayi sp. n. is described from specimens collected in French Polynesia. The new species belongs to an assemblage of morphologically similar Indo-West Pacific (IWP) species, here designated as the "mesobranchial-spine group". All species in the group bear carapace spines, including one or more mesobranchial spines, and transverse, piliferous striations on the dorsal surface of carapace and chelipeds. Petrolisthes paulayi sp. n. is distinguishable from all species in the group by its forwardly produced, trilobate front, and a characteristic combination of carapace spines. We also report on the range extension and live coloration of P. aegyptiacus Werding & Hiller, another species of the mesobranchial-spine group, so far considered a Red Sea endemic. Specimens from the Mascarene Islands confirm that the geographic range of the species extends to the southern Indian Ocean. While specimens morphologically similar to P. aegyptiacus, and collected in the Line and Society Islands, suggest a large range extension to the Central Pacific, it is probable that these individuals represent an undescribed species closely related to P. aegyptiacus. C1 [Hiller, Alexandra] Smithsonian Trop Res Inst, Apartado 0843-03092, Panama City, Panama. [Werding, Bernd] Univ Giessen, Inst Tierokol & Spezielle Zool, Heinrich Buff Ring 29 Tierhaus, D-35392 Giessen, Germany. RP Hiller, A (reprint author), Smithsonian Trop Res Inst, Apartado 0843-03092, Panama City, Panama. EM hillera@si.edu FU Smithsonian grant; Center of Excellence in Marine Sciences (CEMarin) FX We are grateful to the following colleagues for facilitating access to porcellanid material, and for hosting us: G. Paulay, A. Bemis and J. Slapcinsky (Florida Museum of Natural History, Gainesville, U.S.A.) and L. Corbari (MNHN, Paris). We thank S. De Grave, E. MacPherson and M. Osawa for valuable comments and editings that helped improving this manuscript. This study was supported by a Smithsonian grant to A.H., and by the Center of Excellence in Marine Sciences (CEMarin). NR 24 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 617 BP 19 EP 29 DI 10.3897/zookeys.617.9893 PG 11 WC Zoology SC Zoology GA DW1BE UT WOS:000383376900002 PM 27667952 ER PT J AU Harl, H Stevens, L Margulis, SW Petersen, J AF Harl, Heather Stevens, Lisa Margulis, Susan W. Petersen, Jay TI Gibbon Aggression During Introductions: An International Survey SO JOURNAL OF APPLIED ANIMAL WELFARE SCIENCE LA English DT Article DE Gibbon (Hylobatidae); introductions; aggression ID WHITE-HANDED GIBBONS; FOOD RESOURCES; HYLOBATES-LAR; INTRAGROUP AB Little is known regarding the prevalence of aggression seen during introductions of captive gibbons (Hylobatidae). In this study, an online survey was developed to quantify and collect contextual details regarding the frequency and types of aggression seen during introductions of captive gibbons (Hylobatidae). Nineteen percent of institutions (17 institutions) reported observing aggression, and 6 of these institutions recorded multiple instances of aggression, though a vast majority of these cases resulted in mild injuries or none at all. The female was the primary aggressor in 23% of cases, the male was the primary aggressor in 58% of cases, and both were the primary aggressor in 1 case. Although these aggressive interactions were often not associated with a known cause, 27% of cases were associated with food displacement. In most cases, management changes, including trying new pairings, greatly reduced situational aggression, suggesting that individual personalities may play a factor in aggression. These data begin to explain the extent of aggression observed in captive gibbons; future studies will address possible correlations with aggression and introduction techniques. C1 [Harl, Heather; Stevens, Lisa] Smithsonian Natl Zool Pk, Washington, DC USA. [Margulis, Susan W.] Canisius Coll, Dept Anim Behav Ecol & Conservat, Buffalo, NY 14208 USA. [Petersen, Jay] Brookfield Zoo, Chicago Zool Soc, Brookfield, IL USA. RP Harl, H (reprint author), Smithsonian Natl Zool Pk, Primate Dept, 3001 Connecticut Ave NW,MRC 5507,POB 37012, Washington, DC 20013 USA. EM harlh@si.edu NR 17 TC 0 Z9 0 U1 0 U2 1 PU ROUTLEDGE JOURNALS, TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 1088-8705 EI 1532-7604 J9 J APPL ANIM WELF SCI JI J. Appl. Anim. Welf. Sci. PY 2016 VL 19 IS 3 BP 260 EP 270 DI 10.1080/10888705.2015.1130631 PG 11 WC Veterinary Sciences SC Veterinary Sciences GA DU6DB UT WOS:000382302700004 PM 26963568 ER PT J AU Ross, DA Guzman, HM Van Hinsberg, VJ Potvin, C AF Ross, David A. Guzman, Hector M. Van Hinsberg, Vincent J. Potvin, Catherine TI Metal contents of marine turtle eggs (Chelonia mydas; Lepidochelys olivacea) from the tropical eastern pacific and the implications for human health SO JOURNAL OF ENVIRONMENTAL SCIENCE AND HEALTH PART B-PESTICIDES FOOD CONTAMINANTS AND AGRICULTURAL WASTES LA English DT Article DE Green turtle; olive ridley; eggs; cadmium; Panama; toxicology ID RIDLEY SEA-TURTLE; CARETTA-CARETTA; HEAVY-METALS; LEPIDOCHELYS-OLIVACEA; DERMOCHELYS-CORIACEA; MATERNAL TRANSFER; NESTING COLONY; CHELONIA-MYDAS; ERETMOCHELYS-IMBRICATA; ARSENIC ACCUMULATION AB Concentrations of eight elements were measured in Chelonia mydas and Lepidochelys olivacea eggs collected along the Pacific coast of Panama. Manganese (Mn), iron (Fe), copper (Cu), zinc (Zn), arsenic (As), cadmium (Cd), and mercury (Hg) concentrations were similar to previous reports of these species from around the world, while lead (Pb) was lower than previous reports. Cd posed the highest health risk to people who regularly eat the eggs, with average consumption rates leading to target hazard quotients (THQ) of up to 0.35 +/- 0.15. Our conclusions indicate that current turtle egg consumption in isolated, coastal Pacific communities may pose a health concern for young children, and that youth and young adults should limit their consumption of turtle eggs to reduce their total intake of nonessential metals. C1 [Ross, David A.; Potvin, Catherine] McGill Univ, Dept Biol, 1205 Ave Docteur Penfield, Montreal, PQ H3A 1B1, Canada. [Guzman, Hector M.] Smithsonian Trop Res Inst, Panama City, Panama. [Van Hinsberg, Vincent J.] McGill Univ, Dept Earth & Planetary Sci, Montreal, PQ, Canada. RP Ross, DA (reprint author), McGill Univ, Dept Biol, 1205 Ave Docteur Penfield, Montreal, PQ H3A 1B1, Canada. EM davidanross5@gmail.com FU McGill-STRI NEO Program, McGill University; Molson and Hilton Hart Fellowship [00286SC]; Smithsonian Tropical Research Institute; Secretaria Nacional de Ciencia y Tecnologia de Panama (SENACYT) FX Funding for this research was provided by the McGill-STRI NEO Program, McGill University, Dr. Richard Hart (Molson and Hilton Hart Fellowship-00286SC), the Smithsonian Tropical Research Institute, and Secretaria Nacional de Ciencia y Tecnologia de Panama (SENACYT) through funding to H.M. Guzman. NR 89 TC 0 Z9 0 U1 6 U2 6 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 0360-1234 EI 1532-4109 J9 J ENVIRON SCI HEAL B JI J. Environ. Sci. Health Part B-Pestic. Contam. Agric. Wastes PY 2016 VL 51 IS 10 BP 675 EP 687 DI 10.1080/03601234.2016.1191888 PG 13 WC Environmental Sciences; Public, Environmental & Occupational Health SC Environmental Sciences & Ecology; Public, Environmental & Occupational Health GA DV0NA UT WOS:000382613200004 PM 27323656 ER PT S AU Goldstein, G Santiago, LS AF Goldstein, Guillermo Santiago, Louis S. BE Goldstein, G Santiago, LS TI Tropical Tree Physiology Adaptations and Responses in a Changing Environment Preface SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Editorial Material; Book Chapter C1 [Goldstein, Guillermo] Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina. [Goldstein, Guillermo] Univ Miami, Dept Biol, Coral Gables, FL 33124 USA. [Santiago, Louis S.] Univ Calif Riverside, Dept Bot & Plant Sci, Riverside, CA 92521 USA. [Santiago, Louis S.] Smithsonian Trop Res Inst, Panama City, Panama. RP Goldstein, G (reprint author), Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina.; Goldstein, G (reprint author), Univ Miami, Dept Biol, Coral Gables, FL 33124 USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP V EP IX D2 10.1007/978-3-319-27422-5 PG 5 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800001 ER PT S AU Silvera, K Lasso, E AF Silvera, Katia Lasso, Eloisa BE Goldstein, G Santiago, LS TI Ecophysiology and Crassulacean Acid Metabolism of Tropical Epiphytes SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter DE Epiphytes; Crassulacean acid metabolism (CAM); Bromeliaceae; Orchidaceae; Conservation ID VASCULAR EPIPHYTES; PHOTOSYNTHETIC PATHWAYS; ELEVATIONAL GRADIENT; SPECIES COMPOSITION; WATER RELATIONS; CLOUD FOREST; RAIN-FOREST; PUERTO-RICO; COSTA-RICA; LIFE-FORMS AB Epiphytes are plants that germinate and grow upon other plants without contact with mineral soil and without parasitizing their host plant. Therefore, they derive nutrients and water from the environment. Epiphytes are primarily tropical in distribution and may be the most species-rich life form in very wet rainforest sites, constituting about 10 % of all vascular plants. Nearly 80 % of all vascular epiphytes belong to one of three families: Orchidaceae (orchids), Bromeliaceae (bromeliads), and Polypodiaceae (ferns). Orchids in particular, are the most species rich in epiphytes. In this review, information on the ecophysiology of vascular epiphytes is presented, in an attempt to find patterns that explain the ecophysiological adaptations of canopy living. We highlight the ecophysiology of orchids and bromeliads, and whenever possible, provide insight into other epiphytic families. We discuss morphological, anatomical and physiological novelties that epiphytes have evolved to face the challenges of living in the canopy, including adaptations to increase water capture, to facilitate water storage or to reduce water loss. Because epiphytes are particularly susceptible to climate change, and can be monitored as a component of forest health, we also consider their distribution and physiological responses to climate change as a key aspect of conservation programs. C1 [Silvera, Katia; Lasso, Eloisa] Smithsonian Trop Res Inst, POB 0843-03092, Balboa, Ancon, Panama. [Silvera, Katia] Univ Calif Riverside, Dept Bot & Plant Sci, Riverside, CA 92521 USA. [Lasso, Eloisa] Univ Los Andes, Dept Ciencias Biol, Bogota, Colombia. RP Silvera, K (reprint author), Smithsonian Trop Res Inst, POB 0843-03092, Balboa, Ancon, Panama. EM katia.silvera@ucr.edu; e.lasso@uniandes.edu.co OI Lasso, Eloisa/0000-0003-4586-8674 NR 71 TC 0 Z9 0 U1 2 U2 2 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 25 EP 43 DI 10.1007/978-3-319-27422-5_2 D2 10.1007/978-3-319-27422-5 PG 19 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800003 ER PT S AU Campanello, PI Manzane, E Villagra, M Zhang, YJ Panizza, AM di Francescantonio, D Rodriguez, SA Chen, YJ Santiago, LS Goldstein, G AF Campanello, Paula I. Manzane, Eric Villagra, Mariana Zhang, Yong-Jiang Panizza, Adela M. di Francescantonio, Debora Rodriguez, Sabrina A. Chen, Ya-Jun Santiago, Louis S. Goldstein, Guillermo BE Goldstein, G Santiago, LS TI Carbon Allocation and Water Relations of Lianas Versus Trees SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter DE Capacitance; Freestanding liana seedlings; Support-seeker liana seedlings; Stomatal conductance; Transpiration; Long distance water transport ID BARRO-COLORADO ISLAND; TROPICAL FOREST; RAIN-FOREST; STOMATAL CONDUCTANCE; HYDRAULIC ARCHITECTURE; ABOVEGROUND BIOMASS; NEOTROPICAL FOREST; AMAZONIAN FORESTS; LOWLAND FOREST; FRENCH-GUIANA AB Despite lianas being fundamental components of tropical and subtropical forest ecosystems throughout the world, the physiological characteristics of this growth form are not well known. Different behaviors at the seedling stage were until recently largely unnoticed. In one extreme of a continuum of adaptive traits, freestanding liana seedlings invest a large proportion of biomass in self-support tissue while on the other extreme support-seeker seedlings invest more resources in rapid elongation of slender stems with an efficient hydraulic conductive system. Adult lianas often have lower wood density and higher specific leaf area than trees and have most of their leaves deployed at the top of the canopy, experiencing high irradiance and transpirational demands, which requires effective regulation of water loss to avoid desiccation. Recent studies show that lianas have faster stomatal responses to increasing vapor pressure deficit (VPD) and exhibit stronger partial stomatal closure compared to trees. Strong stomatal control and efficient water transport help lianas maintain leaf water potential (Psi(leaf)) within a safe hydraulic range to avoid xylem dysfunction despite their low stem water storage capacity, which is achieved at a minimum cost in terms of carbon assimilation. Liana colonization of tree crowns can significantly reduce tree growth and transpiration with consequences for carbon and water economy at individual tree and ecosystem levels. C1 [Campanello, Paula I.; Villagra, Mariana; Panizza, Adela M.; di Francescantonio, Debora; Rodriguez, Sabrina A.] Univ Nacl Misiones, Lab Ecol Forestal & Ecofisiol, Inst Biol Subtrop, CONICET,FCF, Puerto Iguazu, Argentina. [Manzane, Eric; Santiago, Louis S.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Panama City, Panama. [Zhang, Yong-Jiang] Harvard Univ, Dept Organism & Evolutionary Biol, Cambridge, MA 02138 USA. [Zhang, Yong-Jiang; Chen, Ya-Jun] Chinese Acad Sci, Key Lab Trop Forest Ecol, Xishuangbana Trop Bot Garden, Mengla 666303, Yunnan, Peoples R China. [Santiago, Louis S.] Univ Calif Riverside, Dept Bot & Plant Sci, Riverside, CA 92521 USA. [Goldstein, Guillermo] Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina. [Goldstein, Guillermo] Univ Miami, Dept Biol, Coral Gables, FL 33146 USA. RP Campanello, PI (reprint author), Univ Nacl Misiones, Lab Ecol Forestal & Ecofisiol, Inst Biol Subtrop, CONICET,FCF, Puerto Iguazu, Argentina. EM pcampanello@gmail.com; bioerman@gmail.com; marian.villagra@gmail.com; yongjiangz@126.com; adelamariapanizza@gmail.com; debodifra@gmail.com; sabrinarodriguez78@yahoo.com.ar; chenyj@xtbg.org.cn; santiago@ucr.edu; gold@bio.miami.edu NR 77 TC 0 Z9 0 U1 5 U2 5 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 103 EP 124 DI 10.1007/978-3-319-27422-5_5 D2 10.1007/978-3-319-27422-5 PG 22 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800006 ER PT S AU Santiago, LS Bonal, D De Guzman, ME Avila-Lovera, E AF Santiago, Louis S. Bonal, Damien De Guzman, Mark E. Avila-Lovera, Eleinis BE Goldstein, G Santiago, LS TI Drought Survival Strategies of Tropical Trees SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter ID CUTICULAR WATER PERMEABILITY; STEM CO2 FIXATION; RAIN-FOREST; GAS-EXCHANGE; COORDINATED ADJUSTMENTS; PRECIPITATION GRADIENT; VEGETATION MORTALITY; SPECIES COMPOSITION; MIDDAY DEPRESSION; AMAZONIAN FORESTS AB Climate change is predicted to increase the occurrence of extreme droughts, which are associated with elevated mortality rates in tropical trees. Drought-induced mortality is thought to occur by two main mechanisms: hydraulic failure or carbon starvation. This chapter focuses on the strategies that plants use to survive these two drought-induced mortality mechanisms and how these mechanisms are distributed among the immense diversity of tropical tree species. The traits that tropical trees may use to survive drought include (1) xylem that is resistant to drought-induced cavitation, (2) high sapwood capacitance that protects xylem from critically low water potentials, (3) drought deciduousness, (4) photosynthetic stems that have the potential to assimilate carbon at greater water-use efficiency than leaves, (5) deep roots, (6) regulation of gas exchange to reduce leaf water loss or to maintain photosynthesis at low leaf water potential and (7) when all else fails, low cuticular conductance from exposed tissues during extended drought. To date, most research has focused on deciduousness, resistant xylem, soil water, gas exchange behavior and sapwood capacitance, whereas little is known about the role of photosynthetic stems or cuticular conductance during extreme extended drought, making these processes a high priority for a complete understanding of tropical tree physiology during drought. C1 [Santiago, Louis S.; De Guzman, Mark E.; Avila-Lovera, Eleinis] Univ Calif Riverside, Dept Bot & Plant Sci, 2150 Batchelor Hall, Riverside, CA 92521 USA. [Santiago, Louis S.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Panama City, Panama. [Bonal, Damien] Univ Lorraine, INRA, UMR EEF, F-54280 Champenoux, France. RP Santiago, LS (reprint author), Univ Calif Riverside, Dept Bot & Plant Sci, 2150 Batchelor Hall, Riverside, CA 92521 USA. EM santiago@ucr.edu; bonal@nancy.inra.fr; mark.deguzman@email.ucr.edu; eleinis.avilalovera@email.ucr.edu NR 80 TC 1 Z9 1 U1 6 U2 6 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 243 EP 258 DI 10.1007/978-3-319-27422-5_11 D2 10.1007/978-3-319-27422-5 PG 16 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800012 ER PT S AU Dalling, JW Heineman, K Lopez, OR Wright, SJ Turner, BL AF Dalling, James W. Heineman, Katherine Lopez, Omar R. Wright, S. Joseph Turner, Benjamin L. BE Goldstein, G Santiago, LS TI Nutrient Availability in Tropical Rain Forests: The Paradigm of Phosphorus Limitation SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter DE Ecosystem nutrient budget; Fertilization experiments; Nutrient uptake; Physiological traits; Soil nutrients ID SOIL ORGANIC PHOSPHORUS; BASIN-WIDE VARIATIONS; LITTER DECOMPOSITION; MICROBIAL BIOMASS; FOLIAR NUTRIENTS; NITROGEN; PRODUCTIVITY; GROWTH; DYNAMICS; AMAZON AB A long-standing paradigm in tropical ecology is that phosphorus (P) availability limits the productivity of most lowland forests, with the largest pool of plant-available P resident in biomass. Evidence that P limits components of productivity is particularly strong for sites in Panama and the Amazon basin. Analyses of forest communities in Panama also show that tree species distributions are strongly affected by P availability at the regional scale, but that their local distributions in a single site on Barro Colorado Island (BCI) are as frequently correlated with base cations as with P. Traits associated with species sensitivity to P availability require more detailed exploration, but appear to show little similarity with those associated with N limitation in temperate forests. Recent research indicates that a large fraction of P in tropical forests exists as organic and microbial P in the soil; plant adaptations to access organic P, including the synthesis of phosphatase enzymes, likely represent critical adaptations to low P environments. Plants also cope with low P availability through increases in P use-efficiency resulting from increased retention time of P in biomass and decreased tissue P concentration. Although foliar P responds strongly to P addition, we show here that foliar P and N:P are highly variable within communities, and at BCI correlate with regional species distributional affinity for P. An improved understanding of P limitation, and in particular the plasticity of responses to P availability, will be critical to predicting community and ecosystem responses of tropical forests to climate change. C1 [Dalling, James W.] Univ Illinois, Dept Plant Biol, 505 S Goodwin Ave, Urbana, IL 61801 USA. [Dalling, James W.; Lopez, Omar R.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Panama City, Panama. [Heineman, Katherine] Univ Illinois, Program Ecol Evolut & Conservat Biol, 505 S Goodwin Ave, Urbana, IL 61801 USA. [Lopez, Omar R.] Inst Invest Cient & Serv Alta Tecnol, Apartado Postal 0843-01103, Panama City, Panama. [Wright, S. Joseph; Turner, Benjamin L.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Panama City, Panama. RP Dalling, JW (reprint author), Univ Illinois, Dept Plant Biol, 505 S Goodwin Ave, Urbana, IL 61801 USA. EM dalling@illinois.edu; kheineman@life.illinois.edu; olopez@indicasat.org.pa; WRIGHTJ@si.edu; TurnerBL@si.edu NR 55 TC 1 Z9 1 U1 4 U2 4 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 261 EP 273 DI 10.1007/978-3-319-27422-5_12 D2 10.1007/978-3-319-27422-5 PG 13 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800013 ER PT S AU Santiago, LS Goldstein, G AF Santiago, Louis S. Goldstein, Guillermo BE Goldstein, G Santiago, LS TI Is Photosynthesis Nutrient Limited in Tropical Trees? SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter DE Nitrogen; Phosphorus; Potassium Meta-analysis; Fertilization; Atmospheric carbon-dioxide ID SEEDLING GROWTH-RESPONSES; WATER-USE EFFICIENCY; PHOSPHORUS LIMITATION; RAIN-FOREST; CARBON-DIOXIDE; ELEVATED CO2; PRECIPITATION GRADIENT; NITROGEN RELATIONSHIPS; SAVANNA TREES; WET FOREST AB Tropical forests play an enormously important role in the global cycling of carbon. However, the extent to which nutrients limit the potential for tropical trees to increase carbon gain as atmospheric carbon dioxide rises, a phenomenon known as the carbon-concentration feedback, is uncertain. This chapter addresses our current state of knowledge on nutrient limitation of photosynthesis in tropical trees, summarizing and synthesizing the results of over 20 studies on photosynthetic responses to nutrient manipulation experiments. Our results indicate that nutrient limitation of photosynthesis is widespread, but that contrasting species and ecosystems vary in their responses, with savannah trees showing the least response at the leaf scale. Second, although photosynthesis is strongly limited by N in particular species, N limitation of photosynthesis is modest compared to P limitation of photosynthesis when considering all of the available literature. Finally, alleviation of nutrient limitation through addition of combined nutrient treatments produces the strongest photosynthetic responses, highlighting the potentially complex stroichiometric interactions among elements. The authors discuss several ways forward for resolving questions regarding the potential and limits of tropical trees to influence key carbon cycling processes and thus improve our ability to forecast global responses and feedbacks to climate change. C1 [Santiago, Louis S.] Univ Calif Riverside, Dept Bot & Plant Sci, 2150 Batchelor Hall, Riverside, CA 92521 USA. [Santiago, Louis S.] Smithsonian Trop Res Inst, Panama City, Panama. [Goldstein, Guillermo] Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina. [Goldstein, Guillermo] Univ Miami, Dept Biol, Coral Gables, FL 33146 USA. RP Santiago, LS (reprint author), Univ Calif Riverside, Dept Bot & Plant Sci, 2150 Batchelor Hall, Riverside, CA 92521 USA. EM santiago@ucr.edu; gold@bio.miami.edu NR 80 TC 0 Z9 0 U1 3 U2 3 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 299 EP 315 DI 10.1007/978-3-319-27422-5_14 D2 10.1007/978-3-319-27422-5 PG 17 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800015 ER PT S AU Goldstein, G Santiago, LS Campanello, PI Avalos, G Zhang, YJ Villagra, M AF Goldstein, Guillermo Santiago, Louis S. Campanello, Paula I. Avalos, Gerardo Zhang, Yong-Jiang Villagra, Mariana BE Goldstein, G Santiago, LS TI Facing Shortage or Excessive Light: How Tropical and Subtropical Trees Adjust Their Photosynthetic Behavior and Life History Traits to a Dynamic Forest Environment SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter DE Electron transport rate; Hydraulic architecture; Leaf pigments; Photoinhibition; Photosynthesis; Plasticity; Shade tolerant trees ID THERMAL-ENERGY DISSIPATION; RAIN-FOREST; CARBON GAIN; HAWAIIAN LOBELIADS; ADAPTIVE RADIATION; MOISTURE GRADIENT; FUNCTIONAL TRAITS; XANTHOPHYLL CYCLE; AGE-DETERMINATION; CO2 ASSIMILATION AB Light is critical for plant establishment, growth, and survival in wet tropical forests. The objective of this chapter is to analyze paradigms of photosynthetic performance and life history traits of tropical forest trees to contrasting light environments across the forest floor, gaps and upper canopy. Physiological and morphological plasticity as well as genetically fixed adaptive traits are analyzed, including leaf optical properties and photoprotection from high irradiance. Photosynthetic adaptations to contrasting light environments of closely related species are discussed. This approach has the advantage among comparative studies of adaptations across species in that genetic relationships among species are known. Species-specific variations in maximum photosynthetic rates, which reflect the degree of adaptation to growth irradiance, are shown to be gradual, suggesting that classification into two distinct functional groups in terms of light requirements is somewhat arbitrary. Trees growing in gaps or in the upper canopy rely strongly on biochemical mechanisms to dissipate excess energy and to avoid damage to the light reaction centers and photosystems. Consistent with their high photosynthetic capacity, light demanding species are capable of plastic changes in hydraulic architecture, such as increases in hydraulic conductivity under high irradiance, which makes them more competitive in open habitats. C1 [Goldstein, Guillermo] Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina. [Goldstein, Guillermo] Univ Miami, Dept Biol, Coral Gables, FL 33146 USA. [Santiago, Louis S.] Univ Calif Riverside, Dept Bot & Plant Sci, 2150 Batchelor Hall, Riverside, CA 92521 USA. [Santiago, Louis S.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Balboa, Panama. [Campanello, Paula I.; Villagra, Mariana] Univ Nacl Misiones, Lab Ecol Forestal & Ecofisiol, Inst Biol Subtrop, CONICET,FCF, Posadas, Argentina. [Avalos, Gerardo] Univ Costa Rica, Escuela Biol, San Jose 115012060, Costa Rica. [Avalos, Gerardo] Sch Field Studies, Ctr Sustainable Dev Studies, Cummings Ctr 100, Suite 534-G, Beverly, MA 01915 USA. [Zhang, Yong-Jiang] Dept Organism & Evolutionary Biol, 16 Divin Ave, Cambridge, MA 02138 USA. RP Goldstein, G (reprint author), Univ Buenos Aires, Lab Ecol Func, Dept Ecol Genet & Evoluc, Fac Ciencias Exactas & Nat,Inst IEGEBA CONICET UB, Buenos Aires, DF, Argentina. EM goldstein@ege.fcen.uba.ar; santiago@ucr.edu; pcampanello@yahoo.com; gerardo.avalos@ucr.ac.cr; yongjiangzhang@oeb.harvard.edu; marian.villagra@gmail.com NR 89 TC 1 Z9 1 U1 1 U2 1 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 319 EP 336 DI 10.1007/978-3-319-27422-5_15 D2 10.1007/978-3-319-27422-5 PG 18 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800016 ER PT S AU Russo, SE Kitajima, K AF Russo, Sabrina E. Kitajima, Kaoru BE Goldstein, G Santiago, LS TI The Ecophysiology of Leaf Lifespan in Tropical Forests: Adaptive and Plastic Responses to Environmental Heterogeneity SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter ID NITROGEN USE EFFICIENCY; BORNEAN RAIN-FOREST; PHOTOSYNTHETIC CAPACITY; PHENOTYPIC PLASTICITY; CONSTRUCTION COST; SHADE TOLERANCE; EVERGREEN SHRUB; CARBON BALANCE; PIONEER TREE; DRY FOREST AB Leaf lifespan, the time from leaf expansion to shedding, exhibits wide variation and is a key integrator of relationships with photosynthetic rate, leaf mass per area (LMA), and leaf nitrogen among coexisting tropical tree species. We present a hierarchical view of sources of variation in leaf lifespan in tropical forests, emphasizing the importance of substantial within-species variation, which has rarely been addressed. Interspecific variation in leaf lifespan is positively correlated with LMA, varying from short-lived, low-LMA leaves to long-lived, high-LMA leaves of species associated with resource-rich versus resource-depleted habitats, respectively. Phenotypic responses of leaf lifespan and LMA to light show counter-gradient variation: with acclimation to shade, leaf lifespan increases, and LMA decreases, but both increase with adaptation to shade. In contrast, phenotypic responses to soil fertility are predicted to show co-gradient variation: both leaf lifespan and LMA increase with declining fertility both inter-and intraspecifically. We present new data analyses supporting these predictions, but the interactive effects of light and soil resources can produce complex phenotypic responses. Future studies of leaf lifespan should devote more attention to within-species variation to better quantify and explain how leaf lifespan is central to trade-offs generating the contrasting ecological strategies of tropical tree species. C1 [Russo, Sabrina E.] Univ Nebraska, Sch Biol Sci, Lincoln, NE 68588 USA. [Kitajima, Kaoru] Kyoto Univ, Grad Sch Agr, Kyoto, Japan. [Kitajima, Kaoru] Smithsonian Trop Res Inst, Balboa, Panama. RP Russo, SE (reprint author), Univ Nebraska, Sch Biol Sci, Lincoln, NE 68588 USA. EM srusso2@unl.edu; kaoruk@kais.kyoto-u.ac.jp NR 108 TC 1 Z9 1 U1 4 U2 4 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 357 EP 383 DI 10.1007/978-3-319-27422-5_17 D2 10.1007/978-3-319-27422-5 PG 27 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800018 ER PT S AU Slot, M Winter, K AF Slot, Martijn Winter, Klaus BE Goldstein, G Santiago, LS TI The Effects of Rising Temperature on the Ecophysiology of Tropical Forest Trees SO TROPICAL TREE PHYSIOLOGY: ADAPTATIONS AND RESPONSES IN A CHANGING ENVIRONMENT SE Tree Physiology LA English DT Article; Book Chapter ID ISOPRENE EMISSION; CLIMATE-CHANGE; RAIN-FOREST; LEAF RESPIRATION; THERMAL-ACCLIMATION; GROWTH TEMPERATURE; FICUS-INSIPIDA; RUBISCO ACTIVASE; HEAT TOLERANCE; PHOTOSYNTHETIC RESPONSES AB The response of tropical trees to rising temperatures represents a key uncertainty that limits our ability to predict biosphere-atmosphere feedbacks in a warming world. We review the current understanding of temperature effects on the ecophysiology of tropical trees from organelle to biome level, where we distinguish between short-term responses, acclimation, and adaptation. We present new data on short-term temperature responses of photosynthesis and dark respiration, and temperature acclimation of photosynthesis. We also compare new field and laboratory-obtained photosynthesis-temperature response data. We identify several priority study areas. (1) Acclimation: We need to better understand photosynthetic acclimation, for example to determine whether the adjustment of the thermal optimum of photosynthesis (TOpt) is consistently negated by a decrease in photosynthesis at TOpt, as we observed. (2) Growth: Whereas tropical seedlings may grow better with warming, canopy trees reportedly grow worse; we do not currently know what explains these contrasting temperature effects. (3) Reproduction: Tropical trees may be close to reproductive temperature thresholds, as heat sterility in crops occurs in the upper 30 degrees C range. Nonetheless, the temperature sensitivity of tropical tree reproduction is virtually unstudied. (4) Mortality: How does heat-induced atmospheric drought (high leaf-to-air vapor pressure deficit) affect tropical tree mortality? (5) Stomatal behavior: What is the specific role of temperature in the induction of midday-stomtal closure on sunny days? Better knowledge in these areas will improve our ability to predict carbon fluxes in tropical forests experiencing ongoing warming. C1 [Slot, Martijn; Winter, Klaus] Smithsonian Trop Res Inst, Apartado 0843-03092, Balboa, Ancon, Panama. RP Slot, M (reprint author), Smithsonian Trop Res Inst, Apartado 0843-03092, Balboa, Ancon, Panama. EM SlotM@si.edu NR 136 TC 1 Z9 1 U1 10 U2 10 PU SPRINGER PI DORDRECHT PA PO BOX 17, 3300 AA DORDRECHT, NETHERLANDS SN 1568-2544 BN 978-3-319-27422-5; 978-3-319-27420-1 J9 TREE PHYSIOL-NETH PY 2016 VL 6 BP 385 EP 412 DI 10.1007/978-3-319-27422-5_18 D2 10.1007/978-3-319-27422-5 PG 28 WC Forestry SC Forestry GA BF5XG UT WOS:000382766800019 ER PT B AU Gratwicke, B Neff, M Mayer, LR Ryan, S Sevin, J AF Gratwicke, Brian Neff, Matthew Mayer, Lindsay Renick Ryan, Sharon Sevin, Jennifer BE Dodd, CK TI Education and outreach SO REPTILE ECOLOGY AND CONSERVATION: A HANDBOOK OF TECHNIQUES SE Techniques in Ecology and Conservation Series LA English DT Article; Book Chapter ID CITIZEN SCIENCE; CONSERVATION; LEADERSHIP; SNAKES C1 [Gratwicke, Brian; Neff, Matthew] Smithsonians Natl Zool Pk, Smithsonian Conservat Biol Inst, 3001 Connecticut Ave NW, Washington, DC 20009 USA. [Mayer, Lindsay Renick] Global Wildlife Conservat, POB 129, Austin, TX 78767 USA. [Ryan, Sharon] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Panama City, Panama. [Sevin, Jennifer] Ctr Leadership Global Sustainabil, 900 North Glebe Rd, Arlington, VA 22203 USA. RP Gratwicke, B (reprint author), Smithsonians Natl Zool Pk, Smithsonian Conservat Biol Inst, 3001 Connecticut Ave NW, Washington, DC 20009 USA. EM gratwickeb@si.edu; NeffM@si.edu; renickmayer@gmail.com; RyanSM@si.edu; jennifer.sevin@gmail.com NR 41 TC 0 Z9 0 U1 0 U2 0 PU OXFORD UNIV PRESS PI NEW YORK PA 198 MADISON AVENUE, NEW YORK, NY 10016 USA BN 978-0-19-872614-2; 978-0-19-872613-5 J9 TECH ECOL CONSERVAT PY 2016 BP 436 EP 448 D2 10.1093/acprof:oso/9780198726135.001.0001 PG 13 WC Zoology SC Zoology GA BF5NE UT WOS:000382301800031 ER PT J AU Mathis, WN Costa, DNR Marinoni, L AF Mathis, Wayne N. Costa, Daniel N. R. Marinoni, Luciane TI A review of the Neotropical species of the shore-fly genera Orasiopa and Pectinifer (Diptera: Ephydridae) SO ZOOLOGIA LA English DT Review DE Neotropical Region; shore flies; Discocerinini; taxonomy ID REVISION AB Species of two genera of the tribe Discocerinini from the Neotropics are reviewed with an emphasis on the fauna from Brazil. The two species, Orasiopa (Reymontopa) mera (Cresson, 1939) and Pectinifer aeneus (Cresson, 1918), are described, illustrated and new occurrence data are provided. Phylogenetic relationships of these two genera into the tribe are discussed. To facilitate identification of these species, we have included diagnoses of the Discocerinini and both genera and have also provided an annotated key to the New World genera in this tribe. We have also provided illustrations, photographs, and scanning electron micrographs of external structures and of structures of the male terminalia for included species. C1 [Mathis, Wayne N.] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, POB 37012,MRC 169, Washington, DC 20013 USA. [Costa, Daniel N. R.; Marinoni, Luciane] Univ Fed Parana, Dept Zool, Caixa Postal 19020, BR-81531980 Curitiba, PR, Brazil. RP Costa, DNR (reprint author), Univ Fed Parana, Dept Zool, Caixa Postal 19020, BR-81531980 Curitiba, PR, Brazil. EM mathisw@si.edu; negosekidan@ufpr.br; lmarinoni@ufpr.br RI Marinoni, Luciane /C-5720-2013 FU Conselho Nacional de Desenvolvimento Cientifico e Tecnologico - Brazil (CNPq) [234167/2014-9]; Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brazil; CNPq [401609/2009-0] FX We gratefully acknowledge the assistance and cooperation of many organizations and individuals who contributed to the field work and production of this paper. Photographs of the specimens, especially the faces, were expertly taken with a Visionary Digital System. For reviewing a draft of this paper we thank Tadeusz Zatwarnicki, who also allowed us to use illustrations of the male terminalia that he prepared. We thank the curators and collections managers who loaned collections or facilitated work in their museums: Jon K. Gelhaus and Jason D. Weintraub (ANSP) and Carlos Jose Einicker Lamas (MZUSP). This study was supported by grants from Conselho Nacional de Desenvolvimento Cientifico e Tecnologico - Brazil (CNPq process number 234167/2014-9) and Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brazil, including a recent field work in Brazil (December 2009-June 2010) that resulted in the vast majority of specimens from Brazil that were studied in this paper was supported by a grant from CNPq (Visiting Researcher/Process number 401609/2009-0), which we gratefully acknowledge and thank. We thank Dianne Mathis for helping with all aspects of the production of this paper, especially the field work in Brazil. We also thank A. Bernardo Carvalho and his lab (Elisa, Monica, Susana) for hosting us while conducting field work along the coast of Sao Paulo. NR 32 TC 0 Z9 0 U1 0 U2 0 PU SOC BRASILEIRA ZOOLOGIA, UNIV FEDERAL PARANA PI CURITIBA PA CAIXA POSTAL 19020, CURITIBA, PARANA 81531-980, BRAZIL SN 1984-4670 J9 ZOOLOGIA-CURITIBA JI Zoologia PY 2016 VL 33 IS 3 AR e20150169 DI 10.1590/S1984-4689zool-20150169 PG 15 WC Zoology SC Zoology GA DS5VM UT WOS:000380851100003 ER PT J AU Ryan, T AF Ryan, Terre TI "Changing the Conversation" Contexts for Reading Michelle Obama's American Grown: The Story of the White House Kitchen Garden and Gardens Across America SO FRONTIERS-A JOURNAL OF WOMEN STUDIES LA English DT Article C1 [Ryan, Terre] Harvard Univ, Dumbarton Oaks Res Lib & Collect, Cambridge, MA 02138 USA. [Ryan, Terre] Smithsonian Inst, Washington, DC 20560 USA. [Ryan, Terre] Loyola Univ Maryland, Writing, Baltimore, MD 21210 USA. RP Ryan, T (reprint author), Smithsonian Inst, Washington, DC 20560 USA.; Ryan, T (reprint author), Loyola Univ Maryland, Writing, Baltimore, MD 21210 USA. NR 96 TC 0 Z9 0 U1 0 U2 0 PU UNIV NEBRASKA PRESS PI LINCOLN PA 1111 LINCOLN MALL, LINCOLN, NE 68588-0630 USA SN 0160-9009 EI 1536-0334 J9 FRONTIERS JI Frontiers-J. Women Stud. PY 2016 VL 37 IS 2 BP 75 EP 108 PG 34 WC Women's Studies SC Women's Studies GA DS7TR UT WOS:000380986300005 ER PT J AU Schejter, L Bremec, CS Cairns, SD AF Schejter, Laura Bremec, Claudia S. Cairns, Stephen D. TI Scleractinian corals recorded in the Argentinean Antarctic expeditions between 2012 and 2014, with comments on Flabellum (Flabellum) areum Cairns, 1982 SO POLAR RESEARCH LA English DT Article DE cold-water corals; Antarctica; range extension; bathymetric range extension; Scleractinia ID COLD-WATER CORALS AB In this contribution, we provide a list of the scleractinian corals recorded during the Argentinean Antarctic expeditions on board the oceanographic vessel Puerto Deseado (Argentina) in the austral summers in 2012, 2013 and 2014. The identified taxa consist of six solitary species (Flabellum impensum, F. flexuosum, F. areum, Caryophyllia antarctica, Paraconotrochus antarcticus and Javania antarctica), recorded from 19 sampling sites located off the Antarctic Peninsula and South Shetland and South Orkney islands. We also update the information of F. areum, previously known only from south-west Atlantic waters, extending its distribution range to Antarctic waters and its upper bathymetric range to 218 m. C1 [Schejter, Laura] Inst Nacl Invest & Desarrollo Pesquero, Paseo Victoria Ocampo 1, RA-7600 Mar Del Plata, Buenos Aires, Argentina. [Schejter, Laura; Bremec, Claudia S.] Consejo Nacl Invest Cient & Tecn, Inst Invest Marinas & Costeras, RA-7600 Mar Del Plata, Buenos Aires, Argentina. [Cairns, Stephen D.] Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, Washington, DC 20560 USA. RP Schejter, L (reprint author), Inst Nacl Invest & Desarrollo Pesquero, Paseo Victoria Ocampo 1, RA-7600 Mar Del Plata, Buenos Aires, Argentina. EM schejter@inidep.edu.ar FU National Scientific and Technical Research Council (Consejo Nacional de Investigaciones Cientificas y Tecnicas); Argentinean National Antarctic Direction; National Institute for Fisheries Research and Development (Instituto Nacional de Investigacion y Desarrollo Pesquero); PICT [2013-0629] FX We wish to thank to the crew and participants of the Antarctic expeditions that collaborated during sampling procedures. This study was partially supported by the National Scientific and Technical Research Council (Consejo Nacional de Investigaciones Cientificas y Tecnicas), the Argentinean National Antarctic Direction, the National Institute for Fisheries Research and Development (Instituto Nacional de Investigacion y Desarrollo Pesquero) and PICT 2013-0629 (to SL). This is INIDEP contribution no. 1948. NR 10 TC 0 Z9 0 U1 0 U2 0 PU CO-ACTION PUBLISHING PI JARFALLA PA RIPVAGEN 7, JARFALLA, SE-175 64, SWEDEN SN 0800-0395 EI 1751-8369 J9 POLAR RES JI Polar Res. PY 2016 VL 35 AR 29762 DI 10.3402/polar.v35.29762 PG 6 WC Ecology; Geosciences, Multidisciplinary; Oceanography SC Environmental Sciences & Ecology; Geology; Oceanography GA DS8OR UT WOS:000381043200001 ER PT J AU Velez-Juarbe, J Wood, AR Pimiento, C AF Velez-Juarbe, Jorge Wood, Aaron R. Pimiento, Catalina TI PYGMY SPERM WHALES (ODONTOCETI, KOGIIDAE) FROM THE PLIOCENE OF FLORIDA AND NORTH CAROLINA SO JOURNAL OF VERTEBRATE PALEONTOLOGY LA English DT Article ID CETACEA; ATLANTIC; MIOCENE AB We describe fossil kogiid periotics from the Lower Pliocene upper Bone Valley Formation in central Florida and the Lower to Upper Pliocene Yorktown Formation at Lee Creek Mine, North Carolina. The fossils show diagnostic characters that identify them as belonging to Kogiidae, such as three spines in the anterior process, presence of an incudal process, and a posterior process oriented along the long axis of the bone. Morphological comparisons and morphometric and statistical analyses of periotic proportions confirm the presence of a large and a small morphotype within the sample. The large morphotype (mean length = 39.76 mm) belongs to an unknown kogiid that occurs in both formations, whereas the small morphotype (mean length = 28.64 mm), referred to aff. Kogia sp., occurs only in the Yorktown Formation. The cooccurrence of two taxa in North Carolina may represent one of the earliest evidences of sympatry in kogiids and may demonstrate that this ecological behavior has been part of the natural history of this group at least since the deposition of the Yorktown Formation at Lee Creek (similar to 4.8-3.1 Ma). In addition, the occurrence of the large morphotype in the upper Bone Valley Formation, herein reported for the first time, shows that we are still far from understanding the diversity of marine mammals of that formation and that revision of newly acquired material is necessary. C1 [Velez-Juarbe, Jorge] Nat Hist Museum Los Angeles Cty, Dept Mammal, 900 Exposit Blvd, Los Angeles, CA 90007 USA. [Velez-Juarbe, Jorge; Wood, Aaron R.; Pimiento, Catalina] Univ Florida, Florida Museum Nat Hist, 1659 Museum Rd, Gainesville, FL 32611 USA. [Velez-Juarbe, Jorge] Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol, Washington, DC 20560 USA. [Wood, Aaron R.] Iowa State Univ, Dept Geol & Atmospher Sci, Ames, IA 50011 USA. [Pimiento, Catalina] Univ Zurich, Paleontol Inst & Museum, CH-8006 Zurich, Switzerland. [Pimiento, Catalina] Smithsonian Trop Res Inst, Box 2072, Balboa, Panama. RP Velez-Juarbe, J (reprint author), Nat Hist Museum Los Angeles Cty, Dept Mammal, 900 Exposit Blvd, Los Angeles, CA 90007 USA.; Velez-Juarbe, J (reprint author), Univ Florida, Florida Museum Nat Hist, 1659 Museum Rd, Gainesville, FL 32611 USA.; Velez-Juarbe, J (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol, Washington, DC 20560 USA. EM jvelezjuar@nhm.org; awood@iastate.edu; pimientoc@ufl.edu FU NSF CSBR grant [1203222]; NSF PIRE grant [0966884]; NSF Earth Sciences Postdoctoral Fellowship grant [1249920] FX We thank D. J. Bohaska, C. W. Potter, and N. D. Pyenson (USNM); R. C. Hulbert, Jr., and C. L. McCaffery (FLMNH); C. Argot, G. Billet, and C. deMuizon (MNHN) for providing access to specimens under their care. We are grateful to G. Bianucci, R. E. Fordyce, and Editor O. Lambert for their thorough and helpful review of our article. We extend our gratitude to J. E. Ranson, Jr., for collecting and kindly donating some of the Bone Valley material. The pictures of the UF material were taken by S. Moran as part of ongoing curatorial efforts sponsored by NSF CSBR grant#1203222. This project was funded by NSF PIRE grant #0966884 and NSF Earth Sciences Postdoctoral Fellowship grant #1249920. NR 40 TC 0 Z9 0 U1 4 U2 4 PU TAYLOR & FRANCIS INC PI PHILADELPHIA PA 530 WALNUT STREET, STE 850, PHILADELPHIA, PA 19106 USA SN 0272-4634 EI 1937-2809 J9 J VERTEBR PALEONTOL JI J. Vertebr. Paleontol. PY 2016 VL 36 IS 4 AR e1135806 DI 10.1080/02724634.2016.1135806 PG 10 WC Paleontology SC Paleontology GA DS2EJ UT WOS:000380558100012 ER PT J AU Vari, RP Melo, BF Oliveira, C AF Vari, Richard P. Melo, Bruno F. Oliveira, Claudio TI Protocheirodon, a new genus of Characidae (Teleostei: Characiformes) with the redescription of the poorly known Protocheirodon pi SO Neotropical Ichthyology LA English DT Article DE Aphyocharacinae; Amazon basin; Cheirodontinae; Leptagoniates; Taxonomy ID PHYLOGENY; SUBFAMILY AB Protocheirodon, a new genus of the Characidae, is proposed to include a species previously assigned to Leptagoniates. This action is supported by molecular and morphological phylogenetic hypotheses that place Protocheirodon pi as the sister group of the remaining tribes in the Cheirodontinae versus the traditional assignment of the species to the Aphyocharacinae. The phylogenetic position of Protocheirodon is recognized as a new tribe, the Protocheirodontini. Protocheirodon pi, originally described based on a small number of specimens from a single location in the rio Mamore basin in the southwestern Amazon, is redescribed on the basis of larger series of specimens from the western and central portions of the Amazon basin. C1 [Vari, Richard P.; Melo, Bruno F.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, MCR-159,Box 37012, Washington, DC 20013 USA. [Melo, Bruno F.; Oliveira, Claudio] Univ Estadual Paulista, Inst Biociencias, Dept Morfol, Dist Rubiao Jr S-N, BR-18618970 Botucatu, SP, Brazil. RP Melo, BF (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, MCR-159,Box 37012, Washington, DC 20013 USA.; Melo, BF (reprint author), Univ Estadual Paulista, Inst Biociencias, Dept Morfol, Dist Rubiao Jr S-N, BR-18618970 Botucatu, SP, Brazil. EM melo@ibb.unesp.br; claudio@ibb.unesp.br FU Herbert R. and Evelyn Axelrod Chair in Systematic Ichthyology, Division of Fishes, National Museum of Natural History; FAPESP [2011/08374-1, 2011/50282-7]; CNPq [140193/2015-4] FX We thank Sandra Raredon (USNM) for Fig. 2a and radiographs, Martin and Peter Hoffmann for Fig. 2b, Barbara Brown (AMNH), Mark Sabaj Perez (ANSP), David Catania (CAS), Caleb McMahan and Susan Mochel (FMNH), and Osvaldo Oyakawa and Alessio Datovo (MZUSP) for hospitality during visits and the loan of specimens. We also thank Fernando Carvalho (UFMS), Luiz Malabarba (UFRGS) and an anonymous reviewer for valuable suggestions on the manuscript. Support for the project was provided by the Herbert R. and Evelyn Axelrod Chair in Systematic Ichthyology, Division of Fishes, National Museum of Natural History (RPV), and FAPESP #2011/08374-1, CNPq #140193/2015-4 (BFM) and FAPESP #2011/50282-7 (CO). NR 14 TC 0 Z9 0 U1 1 U2 1 PU SOC BRASILEIRA ICTIOLOGIA PI SAO PAULO PA UNIV SAO PAULO, DEPT FISIOLOGIA-IB, RUA DO MATAO, TRAVESSA 14 N 321, SAO PAULO, SP 05508-900, BRAZIL SN 1679-6225 J9 NEOTROP ICHTHYOL JI Neotrop. Ichthyol. PY 2016 VL 14 IS 2 AR e150154 DI 10.1590/1982-0224-20150154 PG 7 WC Zoology SC Zoology GA DS5OP UT WOS:000380831900015 ER PT J AU Mawdsley, JR AF Mawdsley, Jonathan R. TI The blue carpenter bees: a synopsis of the "Cyaneoderes group" of genus Xylocopa Latreille, 1802 (Hymenoptera: Apidae) SO ORIENTAL INSECTS LA English DT Article DE Apidae; Xylocopa; bee; carpenter bee; large carpenter bee; Cyaneoderes; taxonomy; identification AB A review is presented of the species included within the "Cyaneoderes group" of the genus Xylocopa Latreille, 1802, subgenus Koptortosoma Gribodo, 1894. The 14 names applied to members of this group by previous authors represent six valid species. Females of five species in this group have bright blue and black pubescence on the dorsal surface: X. abbotti (Cockerell, 1909); X. bangkaensis Friese, 1903; X. caerulea (Fabricius, 1804); X. insularis Smith, 1857; and X. tumida, Friese, 1903. A key, diagnostic table, and set of illustrations is presented to facilitate the identification of females of all five species. The known males of species in this group (X. caerulea and X. insularis) are illustrated. Xylocopa dormeyeri Enderlein, 1909, is placed as a synonym of X. insularis Smith, while X. meade-waldoi Hurd, 1959, is placed as a synonym of X. caerulea (Fabricius), New Synonymies. Diagnostic notes are presented for X. incompleta Ritsema, 1880, a species with bright orange (rather than blue) pubescence, which was included in the "Cyaneoderes group" by previous workers. C1 [Mawdsley, Jonathan R.] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. RP Mawdsley, JR (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. EM mawdsleyj@si.edu NR 23 TC 0 Z9 0 U1 0 U2 0 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OR14 4RN, OXON, ENGLAND SN 0030-5316 EI 2157-8745 J9 ORIENT INSECTS JI Orient. Insects PY 2016 VL 50 IS 2 BP 51 EP 60 DI 10.1080/00305316.2016.1170734 PG 10 WC Entomology SC Entomology GA DS0DV UT WOS:000380266500003 ER PT J AU Melo, BF Benine, RC Britzke, R Gama, CS Oliveira, C AF Melo, Bruno F. Benine, Ricardo C. Britzke, Ricardo Gama, Cecile S. Oliveira, Claudio TI An inventory of coastal freshwater fishes from Amapa highlighting the occurrence of eight new records for Brazil SO ZOOKEYS LA English DT Article DE Amazon; French Guyana; Neotropical; South America; Teleostei ID CHARACIFORMES; RIVER AB The Amazon Basin occupies a vast portion of northern South America and contains some of the highest species richness in the world. The northern Brazilian state of Amapa is delimited by the Amazonas River to the south, the Oyapock River to the northern boundary with French Guyana, and the Atlantic northeastern coast to Amazon estuary. Despite several expeditions to the Amazon in recent decades, little is known about the freshwater ichthyofauna from Amapa, with records limited to local inventories and species descriptions. This paper presents a compilation of the freshwater fish diversity sampled in fifteen sites covering two major Amapa ecoregions during the dry season of 2015. 120 species representing eight orders and 40 families are reported upon in this work. Eight species appear for the first time in the Brazilian territory providing new information for future conservation status evaluations. C1 [Melo, Bruno F.; Oliveira, Claudio] Univ Estadual Paulista, Inst Biociencias, Dept Morfol, Rubiao Jr S-N, BR-18618689 Botucatu, SP, Brazil. [Melo, Bruno F.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. [Benine, Ricardo C.] Univ Estadual Paulista, Inst Biociencias, Dept Zool, Rubiao Jr S-N, BR-18618689 Botucatu, SP, Brazil. [Britzke, Ricardo] Univ Tecn Machala, Fac Ciencias Agr, Lab Acuacultura, Av Panamer Km 4 1-2,Via Machala Pasaje, Machala 070150, El Oro, Ecuador. [Gama, Cecile S.] Inst Pesquisas Cient & Tecnol Estado Amapa, Av Feliciano Coelho 1509, BR-68900260 Macapa, Amapa, Brazil. RP Melo, BF (reprint author), Univ Estadual Paulista, Inst Biociencias, Dept Morfol, Rubiao Jr S-N, BR-18618689 Botucatu, SP, Brazil.; Melo, BF (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. EM melo@ibb.unesp.br OI Melo, Bruno F./0000-0002-0499-567X NR 33 TC 1 Z9 1 U1 1 U2 5 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 606 BP 127 EP 140 DI 10.3897/zookeys.606.9297 PG 14 WC Zoology SC Zoology GA DR7ZM UT WOS:000380118200008 PM 27551225 ER PT J AU Baldwin, CC Pitassy, DE Robertson, DR AF Baldwin, Carole C. Pitassy, Diane E. Ross Robertson, D. TI A new deep-reef scorpionfish (Teleostei, Scorpaenidae, Scorpaenodes) from the southern Caribbean with comments on depth distributions and relationships of western Atlantic members of the genus SO ZOOKEYS LA English DT Article DE Manned submersible; Smithsonian Deep Reef Observation Project (DROP); Substation Curacao; ocean exploration; integrative taxonomy; phylogeny ID SEQUENCES AB A new species of scorpionfish, Scorpaenodes barrybrowni Pitassy & Baldwin, sp. n. which is described, was collected during submersible diving in the southern Caribbean as part of the Smithsonian's Deep Reef Observation Project (DROP). It differs from the other two western Atlantic species of the genus, S. caribbaeus and S. tredecimspinosus, in various features, including its color pattern, having an incomplete lateral line comprising 8-10 pored scales, tending to be more elongate, usually having the 11th-12th pectoral-fin rays elongate, and by 20-23% divergence in the cytochrome c oxidase I (COI) DNA barcode sequences. It further differs from one or the other of those species in head spination and in numbers of soft dorsal-fin rays, pectoral-fin rays, and precaudal + caudal vertebrae. Inhabiting depths of 95-160 m, the new species is the deepest western Atlantic member of the genus (S. caribbaeus occurs at depths < 35 m and S. tredecimspinosus from 7 to 82 m). DNA barcode data do not rigorously resolve relationships among the ten species of the genus for which those data are available. C1 [Baldwin, Carole C.; Pitassy, Diane E.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. [Ross Robertson, D.] Smithsonian Trop Res Inst, Balboa, Panama. RP Baldwin, CC (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. EM baldwinc@si.edu FU NMNH Research Programs; Consortium for Understanding and Sustaining a Biodiverse Planet; Competitive Grants for the Promotion of Science program; Herbert R. and Evelyn Axelrod Endowment Fund for systematic ichthyology; National Geographic Society's Committee for Research and Exploration [9102-12] FX For contributing in various ways to this project, we thank the following (in alphabetical order): Bruce Brandt, Barry Brown, Cristina Castillo, Amy Driskell, Tico Christiaan, Rob Loendersloot, Dan Mulcahy, Sandra Raredon, Laureen Schenk, Adriaan Schrier, Barbara van Bebber, Lee Weigt, Jeff Williams, and Carol Youmans. Funding for the Smithsonian Institution's Deep Reef Observation Project was provided internally by NMNH Research Programs to CCB, the Consortium for Understanding and Sustaining a Biodiverse Planet to CCB, the Competitive Grants for the Promotion of Science program to CCB and DRR, and the Herbert R. and Evelyn Axelrod Endowment Fund for systematic ichthyology to CCB; and externally by National Geographic Society's Committee for Research and Exploration to CCB (Grant #9102-12). This is Ocean Heritage Foundation/Curacao Sea Aquarium/Substation Curacao (OHF/SCA/SC) contribution number 25. NR 22 TC 1 Z9 1 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 606 BP 141 EP 158 DI 10.3897/zookeys.606.8590 PG 18 WC Zoology SC Zoology GA DR7ZM UT WOS:000380118200009 PM 27551226 ER PT S AU Smith, FA Payne, JL Heim, NA Balk, MA Finnegan, S Kowalewski, M Lyons, SK McClain, CR McShea, DW Novack-Gottshall, PM Anich, PS Wang, SC AF Smith, Felisa A. Payne, Jonathan L. Heim, Noel A. Balk, Meghan A. Finnegan, Seth Kowalewski, Michal Lyons, S. Kathleen McClain, Craig R. McShea, Daniel W. Novack-Gottshall, Philip M. Anich, Paula Spaeth Wang, Steve C. BE Jeanloz, R Freeman, KH TI Body Size Evolution Across the Geozoic SO ANNUAL REVIEW OF EARTH AND PLANETARY SCIENCES, VOL 44 SE Annual Review of Earth and Planetary Sciences LA English DT Review; Book Chapter DE allometry; biovolume; maximum body size; macroevolution; geobiology ID LIFE-HISTORY PUZZLE; COPES RULE; CLIMATE-CHANGE; CRETACEOUS MOLLUSKS; POPULATION-DENSITY; TRIASSIC RECOVERY; FORMING PLANTS; APEX CHERT; MAMMALS; EXTINCTION AB The Geozoic encompasses the 3.6 Ga interval in Earth history when life has existed. Over this time, life has diversified from exclusively tiny, single-celled organisms to include large, complex multicellular forms. Just how and why this diversification occurred has been a major area of interest for paleontologists and evolutionary biologists for centuries. Here, we compile data on organism size throughout the Geozoic fossil record for the three domains of life. We describe canonical trends in the evolution of body size, synthesize current understanding of the patterns and causal mechanisms at various hierarchical scales, and discuss the biological and geological consequences of variation in organismal size. C1 [Smith, Felisa A.; Balk, Meghan A.] Univ New Mexico, Dept Biol, Albuquerque, NM 87131 USA. [Payne, Jonathan L.; Heim, Noel A.] Stanford Univ, Dept Geol Sci, Stanford, CA 94305 USA. [Finnegan, Seth] Univ Calif Berkeley, Dept Integrat Biol, Berkeley, CA 94720 USA. [Kowalewski, Michal] Univ Florida, Florida Museum Nat Hist, Gainesville, FL 32611 USA. [Lyons, S. Kathleen] Smithsonian Inst, Dept Paleobiol, Natl Museum Nat Hist, Washington, DC 20560 USA. [McClain, Craig R.] Natl Evolutionary Synth Ctr, Durham, NC 27705 USA. [McShea, Daniel W.] Duke Univ, Dept Biol, Durham, NC 27708 USA. [Novack-Gottshall, Philip M.] Benedictine Univ, Dept Biol Sci, Lisle, IL 60532 USA. [Anich, Paula Spaeth] Northland Coll, Dept Biol & Nat Resources, Ashland, WI 54806 USA. [Wang, Steve C.] Swarthmore Coll, Dept Math & Stat, Swarthmore, PA 19081 USA. RP Smith, FA (reprint author), Univ New Mexico, Dept Biol, Albuquerque, NM 87131 USA. EM fasmith@unm.edu RI Kowalewski, Michal/B-4263-2008; OI Kowalewski, Michal/0000-0002-8575-4711; McClain, Craig/0000-0003-0574-428X; Novack-Gottshall, Philip/0000-0002-2583-2968; Heim, Noel/0000-0002-4528-345X; Payne, Jonathan/0000-0002-9601-3310 NR 174 TC 2 Z9 2 U1 5 U2 10 PU ANNUAL REVIEWS PI PALO ALTO PA 4139 EL CAMINO WAY, PO BOX 10139, PALO ALTO, CA 94303-0897 USA SN 0084-6597 BN 978-0-8243-2044-7 J9 ANNU REV EARTH PL SC JI Annu. Rev. Earth Planet. Sci. PY 2016 VL 44 BP 523 EP 553 DI 10.1146/annurev-earth-060115-012147 PG 31 WC Astronomy & Astrophysics; Geosciences, Multidisciplinary SC Astronomy & Astrophysics; Geology GA BF0QT UT WOS:000379329700020 ER PT J AU Nowlan, CR Liu, X Leitch, J Chance, K Abad, GG Liu, C Zoogman, P Cole, J Delker, T Good, W Murcray, F Ruppert, L Soo, D Follette-Cook, MB Janz, SJ Kowalewski, MG Loughner, CP Pickering, KE Herman, JR Beaver, MR Long, RW Szykman, JJ Judd, LM Kelley, P Luke, WT Ren, XR Al-Saadi, JA AF Nowlan, Caroline R. Liu, Xiong Leitch, JamesW. Chance, Kelly Abad, Gonzalo Gonzalez Liu, Cheng Zoogman, Peter Cole, Joshua Delker, Thomas Good, William Murcray, Frank Ruppert, Lyle Soo, Daniel Follette-Cook, Melanie B. Janz, Scott J. Kowalewski, Matthew G. Loughner, Christopher P. Pickering, Kenneth E. Herman, Jay R. Beaver, Melinda R. Long, Russell W. Szykman, James J. Judd, Laura M. Kelley, Paul Luke, Winston T. Ren, Xinrong Al-Saadi, Jassim A. TI Nitrogen dioxide observations from the Geostationary Trace gas and Aerosol Sensor Optimization (GeoTASO) airborne instrument: Retrieval algorithm and measurements during DISCOVER-AQ Texas 2013 SO ATMOSPHERIC MEASUREMENT TECHNIQUES LA English DT Article ID OZONE MONITORING INSTRUMENT; IMAGING DOAS INSTRUMENT; TROPOSPHERIC NO2 RETRIEVAL; ABSORPTION CROSS-SECTION; CMAQ MODELING SYSTEM; SATELLITE RETRIEVALS; STRATOSPHERIC OZONE; FORMALDEHYDE; OMI; SCATTERING AB The Geostationary Trace gas and Aerosol Sensor Optimization (GeoTASO) airborne instrument is a test bed for upcoming air quality satellite instruments that will measure backscattered ultraviolet, visible and near-infrared light from geostationary orbit. GeoTASO flew on the NASA Falcon aircraft in its first intensive field measurement campaign during the Deriving Information on Surface Conditions from Column and Vertically Resolved Observations Relevant to Air Quality (DISCOVER-AQ) Earth Venture Mission over Houston, Texas, in September 2013. Measurements of backscattered solar radiation between 420 and 465 nm collected on 4 days during the campaign are used to determine slant column amounts of NO2 at 250 m x 250 m spatial resolution with a fitting precision of 2.2 x 10(15) molecules cm(-2). These slant columns are converted to tropospheric NO2 vertical columns using a radiative transfer model and trace gas profiles from the Community Multiscale Air Quality (CMAQ) model. Total column NO2 from GeoTASO is well correlated with ground-based Pandora observations (r = 0 : 90 on the most polluted and cloud-free day of measurements and r = 0.74 overall), with GeoTASO NO2 slightly higher for the most polluted observations. Surface NO2 mixing ratios inferred from GeoTASO using the CMAQ model show good correlation with NO2 measured in situ at the surface during the campaign (r = 0 : 85). NO2 slant columns from GeoTASO also agree well with preliminary retrievals from the GEO-CAPE Airborne Simulator (GCAS) which flew on the NASA King Air B200 (r = 0.81, slope = 0.91). Enhanced NO2 is resolvable over areas of traffic NOx emissions and near individual petrochemical facilities. C1 [Nowlan, Caroline R.; Liu, Xiong; Chance, Kelly; Abad, Gonzalo Gonzalez; Liu, Cheng; Zoogman, Peter] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Leitch, JamesW.; Cole, Joshua; Delker, Thomas; Good, William; Murcray, Frank; Ruppert, Lyle; Soo, Daniel] Ball Aerosp & Technol Corp, Boulder, CO 80301 USA. [Follette-Cook, Melanie B.] Morgan State Univ, GESTAR, Baltimore, MD 21251 USA. [Follette-Cook, Melanie B.; Janz, Scott J.; Kowalewski, Matthew G.; Loughner, Christopher P.; Pickering, Kenneth E.] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. [Loughner, Christopher P.; Kelley, Paul; Ren, Xinrong] Univ Maryland, College Pk, MD 20742 USA. [Herman, Jay R.] Univ Maryland Baltimore Cty, Baltimore, MD 21201 USA. [Beaver, Melinda R.; Long, Russell W.; Szykman, James J.] US EPA, Res Triangle Pk, NC 27711 USA. [Judd, Laura M.] Univ Houston, Houston, TX 77004 USA. [Kelley, Paul; Luke, Winston T.; Ren, Xinrong] NOAA, Air Resources Lab, College Pk, MD 20740 USA. [Al-Saadi, Jassim A.] NASA, Langley Res Ctr, Hampton, VA 23681 USA. [Liu, Cheng] Univ Sci & Technol, Hefei, Anhui, Peoples R China. RP Nowlan, CR (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM cnowlan@cfa.harvard.edu RI Liu, Xiong/P-7186-2014; Ren, Xinrong/E-7838-2015; Pickering, Kenneth/E-6274-2012; OI Liu, Xiong/0000-0003-2939-574X; Ren, Xinrong/0000-0001-9974-1666; Gonzalez Abad, Gonzalo/0000-0002-8090-6480; Loughner, Christopher/0000-0002-3833-2014 FU NASA Earth Science Technology Office (ESTO) Instrument Incubator Program; NASA GEO-CAPE Program FX This work was supported under the NASA Earth Science Technology Office (ESTO) Instrument Incubator Program and the NASA GEO-CAPE Program. MODIS MCD43GF V005 data were provided by the MODIS remote sensing group at the University of Massachusetts, Boston. We acknowledge the free use of tropospheric NO2 column data from GOME-2/Metop-A from http://www.temis.nl. The US Environmental Protection Agency through its Office of Research and Development under the Air, Climate and Energy Research Program collaborated on this research. It has been subjected to agency review and approved for publication. NR 63 TC 3 Z9 3 U1 5 U2 6 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1867-1381 EI 1867-8548 J9 ATMOS MEAS TECH JI Atmos. Meas. Tech. PY 2016 VL 9 IS 6 BP 2647 EP 2668 DI 10.5194/amt-9-2647-2016 PG 22 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DQ7OM UT WOS:000379397100013 ER PT J AU Abad, GG Vasilkov, A Seftor, C Liu, X Chance, K AF Abad, Gonzalo Gonzalez Vasilkov, Alexander Seftor, Colin Liu, Xiong Chance, Kelly TI Smithsonian Astrophysical Observatory Ozone Mapping and Profiler Suite (SAO OMPS) formaldehyde retrieval SO ATMOSPHERIC MEASUREMENT TECHNIQUES LA English DT Article ID ROTATIONAL RAMAN-SCATTERING; ABSORPTION CROSS-SECTIONS; MONITORING INSTRUMENT; SATELLITE-OBSERVATIONS; GOME-2 OBSERVATIONS; GLOBAL OBSERVATIONS; ISOPRENE EMISSIONS; COLUMNS; CLIMATE; HCHO AB This paper presents our new formaldehyde (H2CO) retrievals, obtained from spectra recorded by the nadir instrument of the Ozone Mapping and Profiler Suite (OMPS) flown on board NASA's Suomi National Polar-orbiting Partnership (SUOMI-NPP) satellite. Our algorithm is similar to the one currently in place for the production of NASA's Ozone Monitoring Instrument (OMI) operational H2CO product. We are now able to produce a set of long-term data from two different instruments that share a similar concept and a similar retrieval approach. The ongoing overlap period between OMI and OMPS offers a perfect opportunity to study the consistency between both data sets. The different spatial and spectral resolution of the instruments is a source of discrepancy in the retrievals despite the similarity of the physic assumptions of the algorithm. We have concluded that the reduced spectral resolution of OMPS in comparison with OMI is not a significant obstacle in obtaining good-quality retrievals. Indeed, the improved signal-to-noise ratio of OMPS with respect to OMI helps to reduce the noise of the retrievals performed using OMPS spectra. However, the size of OMPS spatial pixels imposes a limitation in the capability to distinguish particular features of H2CO that are discernible with OMI. With root mean square (RMS) residuals similar to 5 x 10(-4) for individual pixels we estimate the detection limit to be about 7.5 x 10(15)aEuro-molecules cm(-2). Total vertical column density (VCD) errors for individual pixels range between 40aEuro-% for pixels with high concentrations to 100aEuro-% or more for pixels with concentrations at or below the detection limit. We compare different OMI products (SAO OMI v3.0.2 and BIRA OMI v14) with our OMPS product using 1 year of data, between September 2012 and September 2013. The seasonality of the retrieved slant columns is captured similarly by all products but there are discrepancies in the values of the VCDs. The mean biases among the two OMI products and our OMPS product are 23aEuro-% between OMI SAO and OMPS SAO and 28aEuro-% between OMI BIRA and OMPS SAO for eight selected regions. C1 [Abad, Gonzalo Gonzalez; Liu, Xiong; Chance, Kelly] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Vasilkov, Alexander; Seftor, Colin] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA. RP Abad, GG (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM ggonzalezabad@cfa.harvard.edu RI Liu, Xiong/P-7186-2014; OI Liu, Xiong/0000-0003-2939-574X; Gonzalez Abad, Gonzalo/0000-0002-8090-6480 FU NASA Atmospheric Composition Program/Aura Science Team [NNX11AE58G]; Consortium for Unlocking the Mysteries of the Universe FX This study is supported by NASA Atmospheric Composition Program/Aura Science Team (NNX11AE58G) and internal Smithsonian Institution funds from the Consortium for Unlocking the Mysteries of the Universe. The Dutch-Finnish OMI instrument is part of the NASA EOS Aura satellite payload. The OMI Project is managed by NIVR and KNMI in the Netherlands. We acknowledge the OMI and OMPS projects for providing data used in this study. We thank Kai Yang for his valuable input understanding the characteristics of OMPS-NM. NR 52 TC 1 Z9 1 U1 3 U2 3 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1867-1381 EI 1867-8548 J9 ATMOS MEAS TECH JI Atmos. Meas. Tech. PY 2016 VL 9 IS 7 BP 2797 EP 2812 DI 10.5194/amt-9-2797-2016 PG 16 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DQ7VY UT WOS:000379417200003 ER PT J AU Sylvester, SP Soreng, RJ Peterson, PM Sylvester, MDPV AF Sylvester, Steven P. Soreng, Robert J. Peterson, Paul M. Sylvester, Mitsy D. P. V. TI An updated checklist and key to the open-panicled species of Poa L. (Poaceae) in Peru including three new species, Poa ramoniana, Poa tayacajaensis, and Poa urubambensis SO PHYTOKEYS LA English DT Article DE Checklist; Gramineae; new species; Peru; Poa; Pooideae; Polylepis forest; Pooideae; Puna grassland; grass taxonomy ID POOIDEAE POEAE POINAE; DISSANTHELIUM POACEAE; ANDES; VEGETATION; PHYLOGENY; COLOMBIA AB We provide an updated checklist and key to the 30 Poa species with open panicles from Peru which includes previously circumscribed Dissanthelium and Aphanelytrum species, new taxon records, and three undescribed species. Poa compressa, P. grisebachii, and P. leioclada are recorded from Peru for the first time. A number of species are placed in synonymy: Poa carazensis, P. ferreyrae and P. tovarii are synonymized under the name P. fibrifera; Poa adusta (tentatively) and P. pilgeri are synonymized under P. candamoana; Poa superata is synonymized under P. grisebachii; and Poa paramoensis is synonymized under P. huancavelicae. Included within this treatment are three new species, Poa ramoniana, P. tayacajaensis and P. urubambensis, which are described and illustrated. Poa ramoniana, found growing near lakes in high elevation Puna grasslands of Junn, is similar to a small form of P. glaberrima, but differs in having rhizomes and growing to only 5 cm tall. Poa tayacajaensis, found from shrublands on Andean slopes of Huancavelica and Huanuco, bears similarities to Poa aequatoriensis but differs in having shorter lemmas which are pubescent between the veins, densely scabrous sheaths with smooth, glabrous throats, and shorter ligules. Poa urubambensis, a common element of the undisturbed Polylepis forest understory of the Cordillera Urubamba, Cusco, is distinct from all other members of open-panicled Poa's by having glabrous lemmas with a smooth and glabrous callus, and notably small anthers. The type material for the name Poa adusta is discussed and a lectotype is selected. C1 [Sylvester, Steven P.; Sylvester, Mitsy D. P. V.] Univ Zurich, Inst Systemat & Evolutionary Bot, Zollikerstr 107, CH-8008 Zurich, Switzerland. [Sylvester, Steven P.] Univ Marburg, Dept Geog, Deutschhausstr 10, D-35032 Marburg, Germany. [Soreng, Robert J.; Peterson, Paul M.] Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, Washington, DC 20013 USA. [Sylvester, Mitsy D. P. V.] Univ Nacl San Antonio Abad Cusco, Ave Cultura 733, Cuzco, Peru. RP Sylvester, SP (reprint author), Univ Zurich, Inst Systemat & Evolutionary Bot, Zollikerstr 107, CH-8008 Zurich, Switzerland.; Sylvester, SP (reprint author), Univ Marburg, Dept Geog, Deutschhausstr 10, D-35032 Marburg, Germany. EM steven_sylvester@hotmail.com OI Sylvester, Steven Paul/0000-0001-5577-8782 FU Leverhulme Trust; SNSF Early Postdoc Mobility Grant [P2ZHP3_161988]; Smithsonian Institution's Restricted Endowment Fund; Scholarly Studies Program, Research Opportunities; Atherton Seidell Foundation; Biodiversity Surveys and Inventories Program; National Geographic Society for Research and Exploration [8848-10, 8087-06] FX This research was funded by a studentship grant from The Leverhulme Trust and an SNSF Early Postdoc Mobility Grant (Grant No. P2ZHP3_161988) to SPS and expedition grants to PMP from the Smithsonian Institution's Restricted Endowment Fund, the Scholarly Studies Program, Research Opportunities, Atherton Seidell Foundation, Biodiversity Surveys and Inventories Program, Small Grants, and the National Geographic Society for Research and Exploration (Grant Nos. 8848-10, 8087-06). Thanks go to Uwe Braun (HAL) for loaning the Poa adusta isotype. We thank Simon Laegaard (AAU), Diego Giraldo-Canas (COL), Asuncion Cano Echevarria (USM), Otakar Sida (PR) for providing information and checking specimens, and Gerrit Davidse (MO) for loans of Poa from Latin America to US. Michael Kessler, ECOAN-Peru and Washington Galiano are thanked for their support, especially with in-country logistics, for SPS, and Asuncion Cano, Maria Isabel La Torre and Nancy Refulio Rodriguez (and others at USM) for same to PMP et al. during fieldwork in Peru. We thank Alice R. Tangerini for providing the Illustrations. Tarciso Filgueiras and an anonymous reviewer are thanked for helpful comments on an earlier version of this manuscript. NR 48 TC 1 Z9 1 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 65 BP 57 EP 90 DI 10.3897/phytokeys.65.7024 PG 34 WC Plant Sciences SC Plant Sciences GA DQ9TK UT WOS:000379552000006 ER PT J AU Herrick, JR Mastromonaco, G Songsasen, N Comizzoli, P AF Herrick, Jason R. Mastromonaco, Gabriela Songsasen, Nucharin Comizzoli, Pierre TI Biomaterials repositories: the science and business of biobanking Foreword SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Editorial Material C1 [Herrick, Jason R.] Colorado Ctr Reprod Med, 10290 RidgeGate Circle, Lone Tree, CO 80124 USA. [Mastromonaco, Gabriela] Toronto Zoo, 361A Old Finch Ave, Toronto, ON M1B 5K7, Canada. [Songsasen, Nucharin] Smithsonian Conservat Biol Inst, 1500 Remount Rd, Front Royal, VA 22630 USA. [Comizzoli, Pierre] Smithsonian Conservat Biol Inst, Natl Zool Pk, 3001 Connecticut Ave,NW, Washington, DC 20008 USA. RP Herrick, JR (reprint author), Colorado Ctr Reprod Med, 10290 RidgeGate Circle, Lone Tree, CO 80124 USA. EM jherrick@flcolo.com NR 11 TC 0 Z9 0 U1 5 U2 6 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 8 BP III EP IV DI 10.1071/RDv28n8_FO PG 2 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DQ0ZN UT WOS:000378930400001 ER PT J AU Hagedorn, M Carter, VL AF Hagedorn, Mary Carter, Virginia L. TI Cryobiology: principles, species conservation and benefits for coral reefs SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Review DE cryopreservation; spermatozoa; Symbiodinium ID GREAT-BARRIER-REEF; CLIMATE-CHANGE; SCLERACTINIAN CORALS; SEASONAL-VARIATION; CYTOTOXIC DIACETYLENES; ACROPORA-DIGITIFERA; MONTIPORA-CAPITATA; GENETIC DIVERSITY; ALGAL SYMBIOSIS; COLD-HARDINESS AB Coral reefs are some of the oldest, most diverse and valuable ecosystems on Earth because they can support one-quarter of all marine life in our oceans. Despite their importance, the world's coral reefs continue to be degraded at unprecedented rates by local and global threats that are warming and creating a more acidic ocean. This paper explores the reproductive challenges of coral for ex situ conservation, using IVF and cryopreservation, and our practical biobanking methods. Coral present challenges for cryopreservation because their reproductive period is often limited to a few nights yearly, they are mostly hermaphrodites with diverse modes of reproduction, including asexual reproduction (i.e. fragmentation and parthenogenesis) and sexual reproduction (i.e. self-and cross-fertilisation) and they express physiological toxins that can inhibit cryopreservation. We have banked spermatozoa from 12 coral species using the same field-hardy methods and have created new coral with thawed spermatozoa. In addition, we describe the cryopreservation of coral symbionts, whose physiology only permits the highest success seasonally. As part of a multidisciplinary conservation strategy, these collections may provide a major hedge against extinction for corals facing the damaging effects of climate change and loss of genetic diversity, and promise to help offset threats to our reefs worldwide. C1 [Hagedorn, Mary; Carter, Virginia L.] Smithsonian Conservat Biol Inst, Natl Zool Pk, Ctr Species Survival, Front Royal, VA 22630 USA. [Hagedorn, Mary] Univ Hawaii, Hawaii Inst Marine Biol, Kaneohe, HI 96744 USA. RP Hagedorn, M (reprint author), Smithsonian Conservat Biol Inst, Natl Zool Pk, Ctr Species Survival, Front Royal, VA 22630 USA. EM hagedornm@si.edu FU Smithsonian Institution; Hawaii Institute of Marine Biology; Australian Institute of Marine Science; Taronga Conservation Society Australia; Roddenberry Foundation; Matthew Frank Foundation; Anela Kolohe Foundation; Cedarhill Foundation FX The authors' experiments reported herein were supported through funds from the Smithsonian Institution, the Hawaii Institute of Marine Biology, the Australian Institute of Marine Science, the Taronga Conservation Society Australia, the Roddenberry Foundation, the Matthew Frank Foundation, the Anela Kolohe Foundation and the Cedarhill Foundation. The authors thank Dr Budhan Pukazhenthi for comments on this manuscript and Nik Zuchowicz, Julio F. Camperio Ciani, Alison N. Dygert and Reuben D. Schleiger for technical assistance. This manuscript was approved for publication by the Hawaii Institute of Marine Biology as contribution # 1647. NR 105 TC 1 Z9 1 U1 18 U2 20 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 8 BP 1049 EP 1060 DI 10.1071/RD16082 PG 12 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DQ0ZN UT WOS:000378930400002 ER PT J AU Hagedorn, M Carter, VL Lager, C Ciani, JFC Dygert, AN Schleiger, RD Henley, EM AF Hagedorn, Mary Carter, Virginia L. Lager, Claire Ciani, Julio F. Camperio Dygert, Alison N. Schleiger, Reuben D. Henley, E. Michael TI Potential bleaching effects on coral reproduction SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Article DE cryopreservation; Fungia scutaria; Montipora capitata; sperm; Symbiodinium ID MONTIPORA-CAPITATA; ELEVATED-TEMPERATURE; REEF; HAWAIIAN; ZOOXANTHELLAE; SPECIFICITY; SETTLEMENT; DIVERSITY; MORTALITY; RADIATION AB Bleaching profoundly impacts coral reproduction, often for years after an event. However, detailed reproductive characteristics of coral after bleaching have not been broadly described, especially as they relate to cryopreservation. Therefore, in the present study we measured several reproductive characteristics in coral in Kaneohe Bay, Hawaii, for two species, namely Fungia scutaria and Montipora capitata, during the bleaching period of 2014 and 2015. We examined spawning periods, egg morphometry, sperm concentration, fresh and cryopreserved sperm motility exposed to different concentrations of dimethyl sulfoxide, time of first cleavage, larval survival with fresh and cryopreserved spermatozoa, infection success and settlement success. Many of these reproductive parameters were reduced in 2015, especially sperm motility. Once the reduced-motility spermatozoa from 2015 post-bleach were cryopreserved, there was a steep decline in post-thaw viability and this would prevent any substantive further use of these samples in reproduction for conservation benefit. Worldwide, as bleaching events become more frequent, the ability to bank and conserve coral ex situ may be significantly reduced. Thus, it is imperative that while genetic diversity is still high in these populations, intensive efforts are made to bank coral species during non-bleaching periods. C1 [Hagedorn, Mary; Carter, Virginia L.; Ciani, Julio F. Camperio; Dygert, Alison N.; Schleiger, Reuben D.; Henley, E. Michael] Smithsonian Conservat Biol Inst, Natl Zool Pk, Dept Reprod Sci, Front Royal, VA 22630 USA. [Hagedorn, Mary; Carter, Virginia L.; Lager, Claire; Ciani, Julio F. Camperio; Dygert, Alison N.; Schleiger, Reuben D.; Henley, E. Michael] Univ Hawaii, Hawaii Inst Marine Biol, Kaneohe, HI 96744 USA. RP Hagedorn, M (reprint author), Smithsonian Conservat Biol Inst, Natl Zool Pk, Dept Reprod Sci, Front Royal, VA 22630 USA.; Hagedorn, M (reprint author), Univ Hawaii, Hawaii Inst Marine Biol, Kaneohe, HI 96744 USA. EM hagedornm@si.edu FU Smithsonian Institution; Hawaii Institute of Marine Biology; Roddenberry Foundation; Matthew Frank Foundation; Anela Kolohe Foundation; Cedarhill Foundation FX These experiments were supported through funds from the Smithsonian Institution, the Hawaii Institute of Marine Biology, the Roddenberry Foundation, the Matthew Frank Foundation, the Anela Kolohe Foundation and the Cedarhill Foundation. The authors thank Dr Budhan Pukazhenthi for comments on the manuscript and Evan Phillipson for his technical assistance. This manuscript was approved for publication by the Hawaii Institute of Marine Biology as Contribution # 1642. NR 41 TC 1 Z9 1 U1 13 U2 16 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 8 BP 1061 EP 1071 DI 10.1071/RD15526 PG 11 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DQ0ZN UT WOS:000378930400003 ER PT J AU Pukazhenthi, BS AF Pukazhenthi, Budhan S. TI Saving wild ungulate diversity through enhanced management and sperm cryopreservation SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Review DE assisted reproduction; biobanking; conservation; Persian onager; semen collection ID EQUUS-FERUS-PRZEWALSKII; DRIED MOUSE SPERMATOZOA; ASSISTED REPRODUCTIVE TECHNOLOGIES; CERATOTHERIUM-SIMUM-COTTONI; VITRO FERTILIZATION SYSTEM; ULTRASOUND-GUIDED MASSAGE; GENETIC RESOURCE BANKS; LIQUID-NITROGEN VAPOR; ACCESSORY SEX GLANDS; CERVUS-ELDI THAMIN AB Wild ungulates throughout the world face the impending risk of extinction. Small founding population size, lack of interest in exhibiting wild ungulates and declining space in zoos are not sustaining ex situ populations. Animals managed in ex situ collections continue to experience >20% neonate loss globally. To ensure population sustainability there is a critical need to: (1) manage ungulates in large herds, increasing mate choice and reproductive efficiency; (2) improve husbandry and genetic management; and (3) develop consistent assisted reproductive technologies, including sperm cryopreservation and AI. Recently, new models in the management of ungulates have begun to emerge. Animal managers and researchers are also beginning to exploit advances in genomics to improve genetic management of their collections. Furthermore, the past decade has witnessed significant advances particularly in semen collection and cryopreservation in numerous species. Advances in gonadal tissue cryopreservation now offer additional opportunities to preserve male genomes. The new knowledge generated is enabling the creation of genetic (sperm) banks to rescue and enhance reproductive management of wild ungulates. The present paper reviews the threats to ungulate populations, the status and relevance of animal management and biomaterial banking efforts to ensure long-term survival of these charismatic species. C1 [Pukazhenthi, Budhan S.] Smithsonian Conservat Biol Inst, Ctr Species Survival, Front Royal, VA 22630 USA. RP Pukazhenthi, BS (reprint author), Smithsonian Conservat Biol Inst, Ctr Species Survival, Front Royal, VA 22630 USA. EM pukazhenthib@si.edu NR 126 TC 2 Z9 2 U1 6 U2 6 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 8 BP 1133 EP 1144 DI 10.1071/RD15412 PG 12 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DQ0ZN UT WOS:000378930400011 ER PT J AU Comizzoli, P Holt, WV AF Comizzoli, Pierre Holt, William V. TI Implications of the Nagoya Protocol for genome resource banks composed of biomaterials from rare and endangered species SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Review DE breeding; conservation biology; genetic materials; museum collections; population management; zoological parks ID ARTIFICIAL-INSEMINATION; STORAGE AB The Nagoya Protocol on Access to Genetic Resources and the Fair and Equitable Sharing of Benefits Arising from their Utilisation is a multilateral legal instrument within the Convention on Biodiversity. It has now come into force, having been signed by 92 countries, 68 of which have ratified it, but notably these do not yet include the US, China, Canada and Russia. The overarching objective of the Nagoya Protocol is to prevent the unfair commercial exploitation of a country's biodiversity and it also protects traditional knowledge. Although the intentions seem reasonable and equitable, the provisions of the Nagoya Protocol will have major effects on the ability of researchers in both the commercial and non-commercial sectors to access genetic materials (which are widely defined and include almost every conceivable animal product, as well as whole animals) from around the world. It also places a heavy bureaucratic burden on researchers and their institutions, which must comply with an international standard and obtain an International Certificate of Compliance proving that all samples will be collected according to the terms of the Protocol. Herein we review of the unforeseen implications of the Nagoya Protocol in relation to biobanking and animal conservation. C1 [Comizzoli, Pierre] Smithsonian Conservat Biol Inst, Natl Zool Pk, 3001 Connecticut Ave NW, Washington, DC 20008 USA. [Holt, William V.] Univ Sheffield, Acad Unit Reprod & Dev Med, Jessop Wing, Sheffield S10 2SF, S Yorkshire, England. RP Comizzoli, P (reprint author), Smithsonian Conservat Biol Inst, Natl Zool Pk, 3001 Connecticut Ave NW, Washington, DC 20008 USA. EM comizzolip@si.edu NR 14 TC 1 Z9 1 U1 5 U2 6 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 8 BP 1145 EP 1151 DI 10.1071/RD15429 PG 7 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DQ0ZN UT WOS:000378930400012 ER PT J AU Pineda, S Medina, M Figueroa, JI Henry, TJ Mena, LV Chavarrieta, JM Gomez, B Valdez, JM Lobit, P Martinez, AM AF Pineda, Samuel Medina, Manuel Figueroa, Jose I. Henry, Thomas J. Mena, Laura V. Chavarrieta, Juan M. Gomez, Benjamin Valdez, Jorge M. Lobit, Philipphe Martinez, Ana M. TI Life history, diagnosis, and biological aspects of Engytatus varians (Hemiptera: Miridae), a predator of Bactericera cockerelli (Hemiptera: Triozidae) SO BIOCONTROL SCIENCE AND TECHNOLOGY LA English DT Article DE Engytatus varians; biological parameters; predation; Bactericera cockerelli ID WESTERN FLOWER THRIPS; HETEROPTERA MIRIDAE; DICYPHUS TAMANINII; HOMOPTERA; CUCUMBER; INSECTS; TOMATO; MEXICO; POTATO; CROPS AB The life cycle and several life parameters of the zoophytophagous predator Engytatus varians (Distant) (Heteroptera: Miridae), including nymphal growth according to Dyar's rule, were examined in the laboratory. The egg, nymph (five instars), and adult stages were 9.20, 17.36, and 19.02 d in length, respectively. The growth ratio for nymphs was consistent with Dyar's rule based on the lengths of the femora of the forelegs, the tibiae and femora of the middle legs, and the antennae. Some biological characteristics of E. varians were also evaluated when the mirid was fed three different diets (B. cockerelli third instars, Sitotroga cerealella Olivier [ Lepidoptera: Gelechiidae] eggs, and a mixture of both instars and eggs). The length of the nymphal stage was three days longer on a diet of only S. cerealella eggs than when the mirids were fed the third instars of B. cockerelli only or a mixture of both. The sex ratio was not affected by the type of diet. Nymphs of E. varians consumed B. cockerelli nymphs (80-85) when fed third instars only and third instars + S. cerealella eggs, respectively. The potential use of this predator as a biological control agent of B. cockerelli is discussed. C1 [Pineda, Samuel; Medina, Manuel; Figueroa, Jose I.; Mena, Laura V.; Chavarrieta, Juan M.; Lobit, Philipphe; Martinez, Ana M.] Univ Michoacana, Inst Invest Agr & Forestales, Km 9-5 Carr, Tarimbaro 58880, Michoacan, Mexico. [Henry, Thomas J.] Smithsonian Inst, ARS, USDA, Systemat Entomol Lab,Natl Museum Nat Hist, Washington, DC 20560 USA. [Gomez, Benjamin] Univ Michoacana, Fac Med Vet & Zootecnia, Tarimbaro 58880, Michoacan, Mexico. [Valdez, Jorge M.] Colegio Postgrad, Programa Entomol & Acarol, Montecillo, Mexico. RP Martinez, AM (reprint author), Univ Michoacana, Inst Invest Agr & Forestales, Km 9-5 Carr, Tarimbaro 58880, Michoacan, Mexico. EM amabel_66@hotmail.com FU Coordinacion de la Investigacion Cientifica de la Universidad Michoacana de San Nicolas de Hidalgo; Consejo Estatal de Ciencia, Tecnologia e Innovacion de Michoacan [03-2014/2015] FX This work was financially supported by the Coordinacion de la Investigacion Cientifica de la Universidad Michoacana de San Nicolas de Hidalgo and by Consejo Estatal de Ciencia, Tecnologia e Innovacion de Michoacan [Project 03-2014/2015]. NR 37 TC 0 Z9 0 U1 2 U2 2 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OR14 4RN, OXON, ENGLAND SN 0958-3157 EI 1360-0478 J9 BIOCONTROL SCI TECHN JI Biocontrol Sci. Technol. PY 2016 VL 26 IS 8 BP 1073 EP 1086 DI 10.1080/09583157.2016.1185088 PG 14 WC Biotechnology & Applied Microbiology; Entomology SC Biotechnology & Applied Microbiology; Entomology GA DP7PW UT WOS:000378692300005 ER PT J AU Cabi, E Soreng, RJ AF Cabi, Evren Soreng, Robert J. TI Two new records and one confirmation of the genus Poa L. (Poaceae) for the Flora of Turkey SO TURKISH JOURNAL OF BOTANY LA English DT Article DE Poa; Poaceae; new records; confirmation; revision; Turkey AB The ongoing revision of the genus Poa in Turkey has resulted in two new Poa records for the Flora of Turkey as Poa pratensis subsp. irrigata (Lindm.) H. Lindb. and Poa eigii Feinbrun. In addition, the presence of Poa palustris L. is confirmed. A brief discussion and an illustration for each taxon are provided. C1 [Cabi, Evren] Namik Kemal Univ, Fac Arts & Sci, Dept Biol, Tekirdag, Turkey. [Soreng, Robert J.] Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, Washington, DC 20560 USA. RP Cabi, E (reprint author), Namik Kemal Univ, Fac Arts & Sci, Dept Biol, Tekirdag, Turkey. EM ecabi@nku.edu.tr FU TUBITAK [212T113]; TUBITAK-BIDEB FX Our gratitude is extended to Lynn Gillespie for joint fieldwork in Turkey in 2011; to Tugrul Koruklu, Ayse Mine Gencler Ozkan, Osman Tugay, Neriman Ozhatay, and Emine Akalin for access to the ANK, AEF, KNYA, and ISTE herbaria in 2014; to TUBITAK, for grant no. 212T113; and to TUBITAK-BIDEB for the support that allowed R.J. Soreng's visit to Namik Kemal University possible. NR 17 TC 0 Z9 0 U1 2 U2 2 PU TUBITAK SCIENTIFIC & TECHNICAL RESEARCH COUNCIL TURKEY PI ANKARA PA ATATURK BULVARI NO 221, KAVAKLIDERE, ANKARA, 00000, TURKEY SN 1300-008X EI 1303-6106 J9 TURK J BOT JI Turk. J. Bot. PY 2016 VL 40 IS 4 BP 439 EP 445 DI 10.3906/bot-1509-27 PG 7 WC Plant Sciences SC Plant Sciences GA DP7OY UT WOS:000378689900011 ER PT J AU Hershler, R Liu, HP Babbitt, C Kellogg, MG Howard, JK AF Hershler, Robert Liu, Hsiu-Ping Babbitt, Caitlin Kellogg, Michael G. Howard, Jeanette K. TI Three new species of western California springsnails previously confused with Pyrgulopsis stearnsiana (Caenogastropoda, Hydrobiidae) SO ZOOKEYS LA English DT Article DE Gastropoda; United States; freshwater; taxonomy; conservation ID AMERICAN NYMPHOPHILINE GASTROPODS; MITOCHONDRIAL-DNA SEQUENCES; GENUS PYRGULOPSIS; SYSTEMATICS; RISSOOIDEA; SNAILS; BASIN AB We describe three new, allopatric species of springsnails (genus Pyrgulopsis) from western California (P. lindae, P. ojaiensis, P. torrida) that were previously identified as P. stearnsiana. The new species are differentiated from P. stearnsiana and each other both by mtCOI sequences (3.9-9.9%) and details of penial morphology. We also provide a phylogeny with increased sampling which confirms a previous finding that P. stearnsiana sensu stricto is paraphyletic relative to two other California species (P. diablensis, P. giulianii). Our molecular and morphological evidence suggests that P. stearnsiana paraphyly is an artifact of conservative taxonomy, however additional studies utilizing rapidly evolving genetic markers will be needed to confidently tease apart the cryptic diversity in this widely ranging springsnail. The new species described herein are narrowly distributed and vulnerable to anthropogenic stressors. The single known population of P. torrida may have become extirpated between 2000 and 2015. C1 [Hershler, Robert] Smithsonian Inst, Dept Invertebrate Zool, Washington, DC 20013 USA. [Liu, Hsiu-Ping; Babbitt, Caitlin] Metropolitan State Univ Denver, Dept Biol, Denver, CO 80217 USA. [Kellogg, Michael G.] San Francisco Publ Util Commiss, 525 Golden Gate Ave, San Francisco, CA 94102 USA. [Howard, Jeanette K.] Nature Conservancy, 201 Mission St, San Francisco, CA 94105 USA. RP Hershler, R (reprint author), Smithsonian Inst, Dept Invertebrate Zool, Washington, DC 20013 USA. EM hershlerr@si.edu FU San Francisco Public Utilities Commission [CS-108]; Nature Conservancy [06132013-1651] FX Linda Lee Crisostomo, Pat Jones, David Lindberg, Thomas Melia and Tim Sullivan assisted with fieldwork. Jim Avant, Rick Duffy and Don Lampe kindly identified springs and facilitated access to San Francisco Public Utilities Commission watershed lands. Jeremy Lukins (SFPUC) shared pertinent GIS shapefiles, and Maggie Ditmore and Chris Higgins obtained useful information on the Salvada Gulch locality. Yolanda Villacampa prepared the scanning electron micrographs, Karolyn Darrow photographed the lectotype of P. stearnsiana, and Freya Goetz prepared the anatomical drawings and figures. This project was supported, in part, by awards (to RH) from the San Francisco Public Utilities Commission (Contract CS-108), and The Nature Conservancy (Contract 06132013-1651). We thank reviewers Art Bogan, Gonzalo Collado, and Alejandro Varela-Romero for their helpful comments on the submitted manuscript. NR 29 TC 1 Z9 1 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 601 BP 1 EP 19 DI 10.3897/zookeys.601.9040 PG 19 WC Zoology SC Zoology GA DQ1AW UT WOS:000378934100001 PM 27551184 ER PT B AU Schwartz, P Heinzel, P Jejcic, S Rybak, J Kotrc, P Farnik, F Kupryakov, YA Deluca, EE Golub, L Jibben, PR Anzer, U Tlatov, AG Guseva, SA AF Schwartz, P. Heinzel, P. Jejcic, S. Rybak, J. Kotrc, P. Farnik, F. Kupryakov, Yu. A. Deluca, E. E. Golub, L. Jibben, P. R. Anzer, U. Tlatov, A. G. Guseva, S. A. BE Dorotovic, I Fischer, CE Temmer, M TI Is it Possible to Use the Green Coronal Line Instead of X rays to Cancel an Effect of the Coronal Emissivity Deficit in Estimation of the Prominence Total Mass from Decrease of the EUV-corona Intensities? SO GROUND-BASED SOLAR OBSERVATIONS IN THE SPACE INSTRUMENTATION ERA SE Astronomical Society of the Pacific Conference Series LA English DT Proceedings Paper CT Coimbra Solar Physics Meeting on Ground-based Solar Observations in the Space Instrumentation Era CY OCT 05-09, 2015 CL Univ Coimbra, Coimbra, PORTUGAL SP SCOSTEP, Variabil Sun & Its Terrestrial Impact, European Space Agcy, Fundacio Ciencia & Tecnologia, Univ Coimbra Reitoria, Univ Coimbra, Dept Matemat, Observat Paris HO Univ Coimbra ID ABSORPTION FEATURES; QUIESCENT PROMINENCE; MISSION; HINODE; SOLAR; TRACE; SOHO; TELESCOPE; IMAGES AB Total masses of six quiescent prominences observed from April through June 2011 were estimated using multi-spectral observations (in EUV, X-rays, Ha, and Can H). The method for the total mass estimation is based on the fact that the intensity of the EUV solar corona at wavelengths below 912 angstrom is reduced at a prominence by the absorption in resonance continua (photoionisation) of hydrogen and possibly by helium and subsequently an amount of absorbed radiation is proportional to the column density of hydrogen and helium plasma. Moreover, the deficit of the coronal emissivity in volume occupied by the cool prominence plasma also contributes to the intensity decrease. The observations in X-rays which are not absorbed by the prominence plasma, allow us to separate these two mechanisms from each other. The X-ray observations of XRT onboard the Hinode satellite made with the Al-mesh focal filter were used because the X-ray coronal radiation formed in plasma of temperatures of the order of 10(6) K was registered and EUV spectral lines occurring in the 193, 211 and 335 angstrom channels of the Atmospheric Imaging Assembly of the Solar Dynamics Observatory satellite are also formed at such temperatures. Unfortunately, the Al-mesh filter has a secondary peak of the transmittance at around 171 angstrom which causes a contribution from the EUV corona to the measured data of up to 11 % in the quiet corona. Thus, absorption in prominence plasma influences XRT X-ray data when using the Al-mesh filter. On the other hand, other X-ray XRT filters are more sensitive to plasma of much higher temperatures (log T of the order of 7), thus observations using these filters cannot be used together with the AIA observations in the method for mass estimations. This problem could be solved using observations in the green coronal line instead of X-rays. Absorption of the green coronal line by a prominence plasma is negligible and this line is formed at temperatures of the order of 106 K. We compare values of the total mass of the prominence observed on. 20 October 2012 on the SE limb estimated when using XRT X-ray observations and observations in the green coronal line obtained at Kislovodsk Mountain Astronomical Station of the Pulkovo observatory (Russia). C1 [Schwartz, P.; Rybak, J.] Slovak Acad Sci, Astron Inst, Tatranska Lomnica 05960, Slovakia. [Heinzel, P.; Kotrc, P.; Farnik, F.; Kupryakov, Yu. A.] Acad Sci Czech Republic, Astron Inst, Ondrejov 25165, Czech Republic. [Jejcic, S.] Univ Ljubljana, Fac Math & Phys, Ljubljana 1000, Slovenia. [Kupryakov, Yu. A.] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119899, Russia. [Deluca, E. E.; Golub, L.; Jibben, P. R.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Anzer, U.] Max Planck Inst Astrophys, Karl Schwarzschild Str 1, D-85740 Garching, Germany. [Tlatov, A. G.; Guseva, S. A.] Pulkovo Observ, Kislovodsk Mt Astron Stn, Gagarina 100, Kislovodsk 357700, Russia. RP Schwartz, P (reprint author), Slovak Acad Sci, Astron Inst, Tatranska Lomnica 05960, Slovakia. EM pschwartz@astro.sk RI Farnik, Frantisek/G-9010-2014; Kotrc, Pavel/G-9030-2014; Heinzel, Petr/G-9014-2014 NR 20 TC 0 Z9 0 U1 0 U2 1 PU ASTRONOMICAL SOC PACIFIC PI SAN FRANCISCO PA 390 ASHTON AVE, SAN FRANCISCO, CA 94112 USA BN 978-1-58381-892-3 J9 ASTR SOC P PY 2016 VL 504 BP 89 EP 96 PG 8 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9RQ UT WOS:000378098700014 ER PT J AU Talamas, EJ Miko, I Copeland, RS AF Talamas, Elijah J. Miko, Istvan Copeland, Robert S. TI Revision of Dvivarnus (Scelionidae, Teleasinae) SO JOURNAL OF HYMENOPTERA RESEARCH LA English DT Article DE Teleasinae; Dvivarnus; Trimorus; Gryonoides; mesoscutellum AB Two new species, Dvivarnus elektrolythron Talamas & Miko, sp. n. and D. mikuki Talamas & Miko, sp. n. are described. The genus is redescribed and a key is provided to separate Dvivarnus from other groups in Teleasinae with mesoscutellar spines. C1 [Talamas, Elijah J.] Smithsonian Inst, Systemat Entomol Lab, USDA ARS, NMNH, Washington, DC 20560 USA. [Miko, Istvan] Penn State Univ, Frost Entomol Museum, State Coll, PA USA. [Copeland, Robert S.] Int Ctr Insect Physiol & Ecol, POB 30772, Nairobi, Kenya. [Copeland, Robert S.] Natl Museums Kenya, Nairobi, Kenya. RP Talamas, EJ (reprint author), Smithsonian Inst, Systemat Entomol Lab, USDA ARS, NMNH, Washington, DC 20560 USA. EM elijah.talamas@ars.usda.gov FU Systematic Entomology Lab, USDA-ARS; U.S. National Science Foundation [DBI-1356381] FX We thank Lubomir Masner, Andy Bennet (CNCI), and Luciana Musetti (OSUC) for the loans of material that made this revision possible. We thank Norman Johnson (OSUC) for developing and maintaining the Hymenoptera Online Database, Specimage, and vSysLab, which underlie the cybertaxonomy conducted here and Joe Cora (OSUC) for providing invaluable database support. Ashton Smith, Trenton Jung, and Pei Luo (USNM) contributed many of the photographs used to illustrate these species. Luke Kresslein (USNM) contributed scanning electron micrographs. We thank Juliet Muriuki, Mzee Hamisi Muhamed Shee, Kazungu Katana, Beatrice Elesani and Mathias Ngonyo for excellent field work. Dr. Miguel Alonso-Zarazaga (MNCN) provided valuable input on etymology. This work was made possible by funding from the Systematic Entomology Lab, USDA-ARS. The USDA does not endorse any commercial product mentioned in this research. USDA is an equal opportunity provider and employer. Istvan Miko was supported by the U.S. National Science Foundation (grant DBI-1356381). NR 9 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1070-9428 EI 1314-2607 J9 J HYMENOPT RES JI J. Hymenopt. Res. PY 2016 VL 49 BP 1 EP 23 DI 10.3897/JHR.49.7714 PG 23 WC Entomology SC Entomology GA DO9XY UT WOS:000378142500001 ER PT S AU Longmore, S Barnes, A Battersby, C Bally, J Kruijssen, JMD Dale, J Henshaw, J Walker, D Rathborne, J Testi, L Ott, J Ginsburg, A AF Longmore, S. Barnes, A. Battersby, C. Bally, J. Kruijssen, J. M. Diederik Dale, J. Henshaw, J. Walker, D. Rathborne, J. Testi, L. Ott, J. Ginsburg, A. BE Simon, R Schaaf, R Stutzki, J TI USING YOUNG MASSIVE STAR CLUSTERS TO UNDERSTAND STAR FORMATION AND FEEDBACK IN HIGH-REDSHIFT-LIKE ENVIRONMENTS SO 6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES SE EAS Publications Series LA English DT Proceedings Paper CT 6th Zermatt ISM Symposium on Conditions and Impact of Star Formation: From Lab to Space CY SEP 07-11, 2015 CL Zermatt, SWITZERLAND SP Deutsch Forschungsgemeinschaft, Int Stifung Hochalpine Forschungstationen Jungfraujoch & Gornergrat, Burgergemeinde Zermatt, Gornegrat Monte Rosa Bahn ID MOLECULAR GAS; GALAXY; G0.253+0.016; PROGENITOR; REVEALS AB The formation environment of stars in massive stellar clusters is similar to the environment of stars forming in galaxies at a red shift of 1 3, at the peak star formation rate density of the Universe. As massive clusters are still forming at the present day at a fraction of the distance to high-redshift galaxies they offer an opportunity to understand the processes controlling star formation and feedback in conditions similar to those in which most stars in the Universe formed. Here we describe a system of massive clusters and their progenitor gas clouds in the centre of the Milky Way, and outline how detailed observations of this system may be able to: (i) help answer some of the fundamental open questions in star formation and (ii) quantify how stellar feedback couples to the surrounding interstellar medium in this high-pressure, high-redshift analogue environment. C1 [Longmore, S.; Barnes, A.; Walker, D.; Rathborne, J.] Liverpool John Moores Univ, Astrophys Res Inst, Liverpool L3 5UX, Merseyside, England. [Battersby, C.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA USA. [Bally, J.] Univ Colorado, Boulder, CO 80309 USA. [Kruijssen, J. M. Diederik] Heidelberg Univ, Astron Rech Inst, Bergheimer Str 58, D-69115 Heidelberg, Germany. [Dale, J.] Excellence Cluster Univ, Munich, Germany. [Rathborne, J.] CSIRO Astron & Space Sci, Narrabri, NSW, Australia. [Testi, L.; Ginsburg, A.] European So Observ, Garching, Germany. [Ott, J.] Natl Radio Astron Observ, Charlottesville, VA USA. RP Longmore, S (reprint author), Liverpool John Moores Univ, Astrophys Res Inst, Liverpool L3 5UX, Merseyside, England. NR 17 TC 0 Z9 0 U1 1 U2 1 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 1633-4760 BN 978-2-7598-2022-1 J9 EAS PUBLICATIONS PY 2016 VL 75-76 BP 43 EP 48 DI 10.1051/eas/1575006 PG 6 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9MS UT WOS:000377836300005 ER PT S AU Koch, PM Tang, YW Ho, PTP Zhang, Q Girart, JM Chen, HRV Lai, SP Li, HB Li, ZY Liu, HB Padovani, M Qiu, K Rao, R Yen, HW Frau, P Chen, HH Ching, TC AF Koch, P. M. Tang, Y. W. Ho, P. T. P. Zhang, Q. Girart, J. M. Chen, H. R. V. Lai, S. P. Li, H. B. Li, Z. Y. Liu, H. B. Padovani, M. Qiu, K. Rao, R. Yen, H. W. Frau, P. Chen, H. H. Ching, T. C. BE Simon, R Schaaf, R Stutzki, J TI LOCAL MAGNETIC FIELD ROLE IN STAR FORMATION SO 6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES SE EAS Publications Series LA English DT Proceedings Paper CT 6th Zermatt ISM Symposium on Conditions and Impact of Star Formation: From Lab to Space CY SEP 07-11, 2015 CL Zermatt, SWITZERLAND SP Deutsch Forschungsgemeinschaft, Int Stifung Hochalpine Forschungstationen Jungfraujoch & Gornergrat, Burgergemeinde Zermatt, Gornegrat Monte Rosa Bahn ID SUBMILLIMETER ARRAY OBSERVATIONS; DUST POLARIZATION; G240.31+0.07; REGIONS; CORE AB We highlight distinct and systematic observational features of magnetic field morphologies in polarized submm dust continuum. We illustrate this with specific examples and show statistical trends from a sample of 50 star-forming regions. C1 [Koch, P. M.; Tang, Y. W.; Ho, P. T. P.; Chen, H. R. V.; Lai, S. P.; Liu, H. B.; Yen, H. W.] Acad Sinica, Inst Astron & Astrophys, Taipei 115, Taiwan. [Ho, P. T. P.] East Asian Observ, 660 N Aohoku Pl,Univ Pk, Hilo, HI 96720 USA. [Zhang, Q.; Chen, H. H.; Ching, T. C.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Girart, J. M.] Inst Ciencies Espai, Fac Ciencies, C5p 2, Bellaterra 08193, Catalonia, Spain. [Chen, H. R. V.; Lai, S. P.; Ching, T. C.] Natl Tsing Hua Univ, Inst Astron, Hsinchu, Taiwan. [Chen, H. R. V.; Lai, S. P.; Ching, T. C.] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan. [Li, H. B.] Chinese Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China. [Li, Z. Y.] Univ Virginia, Dept Astron, Charlottesville, VA 22904 USA. [Padovani, M.] Univ Montpellier, Lab Univers & Particules Montpellier, Montpellier, France. [Padovani, M.] INAF Osservatorio Astrofis Arcetri, Florence, Italy. [Qiu, K.] Nanjing Univ, Sch Astron & Space Sci, Nanjiing 210093, Peoples R China. [Rao, R.] Inst Astron & Astrophys, Acad Sinica, Hilo, HI 96720 USA. [Frau, P.] Observ Astron Nacl, Madrid 28014, Spain. RP Koch, PM (reprint author), Acad Sinica, Inst Astron & Astrophys, Taipei 115, Taiwan. NR 11 TC 0 Z9 0 U1 0 U2 0 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 1633-4760 BN 978-2-7598-2022-1 J9 EAS PUBLICATIONS PY 2016 VL 75-76 BP 159 EP 162 DI 10.1051/eas/1575027 PG 4 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9MS UT WOS:000377836300026 ER PT S AU Mottram, JC van Dishoeck, EF Kristensen, LE Jose-Garcia, IS AF Mottram, J. C. van Dishoeck, E. F. Kristensen, L. E. Jose-Garcia, I. San CA WISH WILL & Cygnus-X Teams BE Simon, R Schaaf, R Stutzki, J TI LIFE IN THE FAST LANE: H2O REVEALS THE UNIVERSAL NATURE OF SHOCKS IN OUTFLOWS SO 6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES SE EAS Publications Series LA English DT Proceedings Paper CT 6th Zermatt ISM Symposium on Conditions and Impact of Star Formation: From Lab to Space CY SEP 07-11, 2015 CL Zermatt, SWITZERLAND SP Deutsch Forschungsgemeinschaft, Int Stifung Hochalpine Forschungstationen Jungfraujoch & Gornergrat, Burgergemeinde Zermatt, Gornegrat Monte Rosa Bahn ID WATER AB Water is an unique tracer of motion in protostars. It has broad and complex line profiles, dominated by the jet/outflow system. We summarise the results of spectrally resolved H2O line profiles observed with Herschel HIFI from the "Water in star-forming regions with Herschel" (WISH, van Dishoeck et al. 2011), "William Herschel Line Legacy" (WILL, Mottram et al. in prep.) and Cygnus-X surveys. In total, more than 100 low-, intermediate and high-mass (LM, IM HM) protostars have been observed with Lbol from 0.1 to 10(5) L-circle dot. On Galactic scales, water traces star formation. C1 [Mottram, J. C.; van Dishoeck, E. F.; Jose-Garcia, I. San] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. [Mottram, J. C.] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany. [van Dishoeck, E. F.] Max Planck Inst Extraterr Phys, Giessenbachstr 2, D-85478 Garching, Germany. [Kristensen, L. E.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Mottram, JC (reprint author), Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands.; Mottram, JC (reprint author), Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany. EM mottram@mpia.de NR 12 TC 0 Z9 0 U1 0 U2 0 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 1633-4760 BN 978-2-7598-2022-1 J9 EAS PUBLICATIONS PY 2016 VL 75-76 BP 195 EP 197 DI 10.1051/eas/1575037 PG 3 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9MS UT WOS:000377836300036 ER PT S AU Rodon, JA Beuther, H Zhang, Q AF Rodon, J. A. Beuther, H. Zhang, Q. BE Simon, R Schaaf, R Stutzki, J TI THE GENTLE CMF OF HIGH-MASS STAR-FORMING REGIONS SO 6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES SE EAS Publications Series LA English DT Proceedings Paper CT 6th Zermatt ISM Symposium on Conditions and Impact of Star Formation: From Lab to Space CY SEP 07-11, 2015 CL Zermatt, SWITZERLAND SP Deutsch Forschungsgemeinschaft, Int Stifung Hochalpine Forschungstationen Jungfraujoch & Gornergrat, Burgergemeinde Zermatt, Gornegrat Monte Rosa Bahn AB We derive the core mass functions (CMFs) of three high mass star forming regions from interferometric mm observations of their dust emission, obtaining power-law slopes beta similar to -2.2 (similar to the Salpeter IMF), beta similar to -1.6, and beta similar to -1.7. The CMF were obtained with the same procedure and the regions are similar in mass and luminosity. The cause for the difference in slopes is uncertain, but our results suggest that the shape of the CMF is not the only constraint for the shape of the IMF. C1 [Rodon, J. A.] European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany. [Beuther, H.] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany. [Zhang, Q.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA USA. RP Rodon, JA (reprint author), European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany. NR 6 TC 0 Z9 0 U1 0 U2 0 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 1633-4760 BN 978-2-7598-2022-1 J9 EAS PUBLICATIONS PY 2016 VL 75-76 BP 209 EP 210 DI 10.1051/eas/1575042 PG 2 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9MS UT WOS:000377836300041 ER PT S AU Tobin, JJ Looney, LW Li, ZY Chandler, CJ Dunham, MM Segura-Cox, D Cox, EG Harris, RJ Melis, C Sadavoy, SI Perez, L Kratter, K AF Tobin, J. J. Looney, L. W. Li, Z. -Y. Chandler, C. J. Dunham, M. M. Segura-Cox, D. Cox, E. G. Harris, R. J. Melis, C. Sadavoy, S. I. Perez, L. Kratter, K. BE Simon, R Schaaf, R Stutzki, J TI REVOLUTIONIZING OUR VIEW OF PROTOSTELLAR MULTIPLICITY AND DISKS: THE VLA NASCENT DISK AND MULTIPLICITY (VANDAM) SURVEY OF THE PERSEUS MOLECULAR CLOUD SO 6TH ZERMATT ISM-SYMPOSIUM: CONDITIONS AND IMPACT OF STAR FORMATION: FROM LAB TO SPACE: IN MEMORY OF CHARLES H. TOWNES SE EAS Publications Series LA English DT Proceedings Paper CT 6th Zermatt ISM Symposium on Conditions and Impact of Star Formation: From Lab to Space CY SEP 07-11, 2015 CL Zermatt, SWITZERLAND SP Deutsch Forschungsgemeinschaft, Int Stifung Hochalpine Forschungstationen Jungfraujoch & Gornergrat, Burgergemeinde Zermatt, Gornegrat Monte Rosa Bahn ID TURBULENT FRAGMENTATION; PROTOSTARS; STAR; SYSTEMS AB There is substantial evidence for disk formation taking place during the early stages of star formation and for most stars being born in multiple systems; however, protostellar multiplicity and disk searches have been hampered by low resolution, sample bias, and variable sensitivity. We have conducted an unbiased, high-sensitivity Karl G. Jansky Very Large Array (VLA) survey toward all known protostars (n = 94) in the Perseus molecular cloud (d similar to 230 pc), with a resolution of similar to 15 AU (0.06") at A = 8 mm. We have detected candidate protostellar disks toward 17 sources (with 12 of those in the Class 0 stage) and we have found substructure on <50 AU scales for three Class 0 disk candidates, possibly evidence for disk fragmentation. We have discovered 16 new multiple systems (or new components) in this survey; the new systems have separations <500 AU and 3 by <30 AU. We also found a bi-modal distribution of separations, with peaks at, similar to 75 AU and, similar to 3000 AU, suggestive of formation through two distinct mechanisms: disk and turbulent fragmentation. The results from this survey demonstrate the necessity and utility of uniform, unbiased surveys of protostellar systems at millimeter and centimeter wavelengths. C1 [Tobin, J. J.] Leiden Observ, Leiden, Netherlands. [Looney, L. W.; Segura-Cox, D.; Cox, E. G.; Harris, R. J.] Univ Illinois, Chicago, IL 60680 USA. [Li, Z. -Y.] Univ Virginia, Charlottesville, VA 22903 USA. [Chandler, C. J.; Perez, L.] Natl Radio Astron Observ, New York, NY USA. [Dunham, M. M.] Harvard Smithsonian Ctr Astrophys, New York, NY USA. [Melis, C.] Univ Calif San Diego, La Jolla, CA 92093 USA. [Sadavoy, S. I.] Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany. [Kratter, K.] Univ Arizona, Tucson, AZ 85721 USA. RP Tobin, JJ (reprint author), Leiden Observ, Leiden, Netherlands. NR 14 TC 0 Z9 0 U1 0 U2 0 PU E D P SCIENCES PI CEDEX A PA 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE SN 1633-4760 BN 978-2-7598-2022-1 J9 EAS PUBLICATIONS PY 2016 VL 75-76 BP 273 EP 276 DI 10.1051/eas/1575054 PG 4 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA BE9MS UT WOS:000377836300053 ER PT J AU Lopez, K Angeli, C Aguilar, C Loaiza, JR De Leon, LF McMillan, WO Miller, MJ AF Lopez, Krisangel Angeli, Cody Aguilar, Celestino Loaiza, Jose R. Fernando De Leon, Luis Owen McMillan, W. Miller, Matthew J. TI Extreme mitogenomic divergence between two syntopic specimens of Arremon aurantiirostris (Aves: Emberizidae) in central Panama suggests possible cryptic species SO MITOCHONDRIAL DNA PART A LA English DT Article DE Mitogenome; neotropical bird; secondary contact ID BIRDS AB We report the complete mitochondrial genome of two specimens of Orange-billed Sparrow Arremon aurantiirostris from Colon Province, in central Panama. The two specimens were collected on the same day, and at the same locality; however, they showed substantial divergence (6.3% average pairwise divergence among coding genes). A survey of ND2 sequence variation across Panama suggests that this divergence is the result of geographic differentiation and secondary contact. This high level of mitochondrial divergence among co-occurring individuals raises the possibility of multiple biological species in Orange-billed Sparrows. Our results are yet another demonstration that much remains to be discovered regarding avian biodiversity in Panama and throughout the Neotropics. C1 [Lopez, Krisangel; Angeli, Cody; Miller, Matthew J.] Villanova Univ, Dept Biol, 800 E Lancaster Ave, Villanova, PA 19085 USA. [Aguilar, Celestino; Loaiza, Jose R.; Fernando De Leon, Luis; Miller, Matthew J.] Inst Invest Cient & Serv Alta Tecnol INDICASAT AI, Panama City, Panama. [Aguilar, Celestino; Owen McMillan, W.; Miller, Matthew J.] Smithsonian Trop Res Inst, Panama City, Panama. RP Lopez, K (reprint author), Villanova Univ, Dept Biol, 800 E Lancaster Ave, Villanova, PA 19085 USA. EM krisangel.lopez@gmail.com OI Miller, Matthew/0000-0002-2939-0239 FU Smithsonian Tropical Research Institute Office of Academic Programs; Villanova University Biology Department FX The authors report no conflict of interest. The authors alone are responsible for the content and writing of the article. This work was funded by the Smithsonian Tropical Research Institute Office of Academic Programs and the Villanova University Biology Department. We thank Panama's Environmental Ministry (MiAmbiente, formerly ANAM) for continued support of scientific collecting, without which, this study would not have been possible. We thank J. Klicka, G. Spellman, J. DeCosta, P. Guitton for collaboration in the field that was responsible for collecting the specimens used in this study. NR 16 TC 0 Z9 0 U1 0 U2 0 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 2-4 PARK SQUARE, MILTON PARK, ABINGDON OR14 4RN, OXON, ENGLAND SN 2470-1394 EI 2470-1408 J9 MITOCHONDRIAL DNA A JI Mitochondrial DNA Part A PY 2016 VL 27 IS 5 BP 3451 EP 3453 DI 10.3109/19401736.2015.1066344 PG 3 WC Genetics & Heredity SC Genetics & Heredity GA DO7IU UT WOS:000377956700151 PM 26367084 ER PT J AU Ho, S Schachat, SR Piel, WH Monteiro, A AF Ho, Sebastian Schachat, Sandra R. Piel, William H. Monteiro, Antonia TI Attack risk for butterflies changes with eyespot number and size SO ROYAL SOCIETY OPEN SCIENCE LA English DT Article DE paper models; predation; nymphalid; Mycalesis; intimidation ID BICYCLUS-ANYNANA; EVOLUTION; DETECTABILITY; INTIMIDATION; PREDATION; SELECTION; DEFENSE; WINGS; EYE AB Butterfly eyespots are known to function in predator deflection and predator intimidation, but it is still unclear what factors cause eyespots to serve one function over the other. Both functions have been demonstrated in different species that varied in eyespot size, eyespot number and wing size, leaving the contribution of each of these factors to butterfly survival unclear. Here, we study how each of these factors contributes to eyespot function by using paper butterfly models, where each factor is varied in turn, and exposing these models to predation in the field. We find that the presence of multiple, small eyespots results in high predation, whereas single large eyespots (larger than 6mm in diameter) results in low predation. These data indicate that single large eyespots intimidate predators, whereas multiple small eyespots produce a conspicuous, but non-intimidating signal to predators. We propose that eyespots may gain an intimidation function by increasing in size. Our measurements of eyespot size in 255 nymphalid butterfly species show that large eyespots are relatively rare and occur predominantly on ventral wing surfaces. By mapping eyespot size on the phylogeny of the family Nymphalidae, we show that these large eyespots, with a potential intimidation function, are dispersed throughout multiple nymphalid lineages, indicating that phylogeny is not a strong predictor of eyespot size. C1 [Ho, Sebastian; Piel, William H.; Monteiro, Antonia] Natl Univ Singapore, Dept Biol Sci, Singapore 117548, Singapore. [Schachat, Sandra R.] Mississippi State Univ, Dept Biochem Mol Biol Entomol & Plant Pathol, Mississippi State, MS 39762 USA. [Schachat, Sandra R.] Smithsonian Inst, Dept Paleobiol, POB 37012,MRC 121, Washington, DC 20013 USA. [Piel, William H.; Monteiro, Antonia] Yale NUS Coll, Singapore, Singapore. RP Monteiro, A (reprint author), Natl Univ Singapore, Dept Biol Sci, Singapore 117548, Singapore.; Monteiro, A (reprint author), Yale NUS Coll, Singapore, Singapore. EM antonia.monteiro@nus.edu.sg OI Schachat, Sandra/0000-0003-3237-5619 FU Department of Biological Sciences; Singapore Ministry of Education [MOE2014-T2-1-146]; National Science Foundation Graduate Research Fellowship Program [DGE-1125191] FX We thank the Department of Biological Sciences and the Singapore Ministry of Education grant no. MOE2014-T2-1-146 for support. S.R.S. is supported by the National Science Foundation Graduate Research Fellowship Program under grant no. DGE-1125191. NR 44 TC 3 Z9 3 U1 10 U2 10 PU ROYAL SOC PI LONDON PA 6-9 CARLTON HOUSE TERRACE, LONDON SW1Y 5AG, ENGLAND SN 2054-5703 J9 ROY SOC OPEN SCI JI R. Soc. Open Sci. PD JAN PY 2016 VL 3 IS 1 AR 150614 DI 10.1098/rsos.150614 PG 13 WC Multidisciplinary Sciences SC Science & Technology - Other Topics GA DO7NF UT WOS:000377968600031 PM 26909190 ER PT J AU Tornabene, L Robertson, DR Baldwin, CC AF Tornabene, Luke Robertson, D. Ross Baldwin, Carole C. TI Varicus lacerta, a new species of goby (Teleostei, Gobiidae, Gobiosomatini, Nes subgroup) from a mesophotic reef in the southern Caribbean SO ZOOKEYS LA English DT Article DE Systematics; molecular phylogeny; deep reefs; submersible; Curacao; Psilotris ID WESTERN ATLANTIC; 7-SPINED GOBIES; GENUS; SPECIATION; PSILOTRIS; PISCES AB We describe a new species of goby, Varicus lacerta sp. n., which was collected from a mesophotic reef at Curacao, southern Caribbean. The new species is the tenth species of Varicus, all of which occur below traditional SCUBA depths in the wider Caribbean area. Its placement in the genus Varicus is supported by a molecular phylogenetic analysis of three nuclear genes and the mitochondrial gene cytochrome b. In addition, the new species has one anal-fin pterygiophore inserted anterior to the first haemal spine, which distinguishes Varicus species from most species in the closely related and morphologically similar genus Psilotris. Varicus lacerta sp. n. is distinguished from all other named species of Varicus by the absence of scales, having highly branched, feather-like pelvic-fin rays, and in its live coloration. We provide the cytochrome c oxidase I DNA barcode of the holotype and compare color patterns of all species of Varicus and Psilotris for which color photographs or illustrations are available. This study is one of several recent studies demonstrating the utility of manned submersibles in exploring the diversity of poorly studied but species-rich deep-reef habitats. C1 [Tornabene, Luke; Baldwin, Carole C.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Div Fishes, POB 37012, Washington, DC 20013 USA. [Robertson, D. Ross] Smithsonian Trop Res Inst, Balboa, Panama. RP Tornabene, L (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Div Fishes, POB 37012, Washington, DC 20013 USA. EM Luke.Tornabene@gmail.com FU Smithsonian Peter Buck Fellowship; Consortium for Understanding and Sustaining a Biodiverse Planet; Competitive Grants for the Promotion of Science program; Herbert R. and Evelyn Axelrod Endowment Fund for systematic ichthyology; Prince Albert II of Monaco Foundation FX We thank Thomas Devine for assistance in the field and with DNA barcoding the holotype specimen; Matthew DeSaix for his help with molecular work; Jeffrey T. Williams and Diane Pitassy for cataloging material, and Sandra Raredon for photographing the preserved holotype and assisting with radiographs. We are grateful for the help of Cristina Castillo, Adriaan 'Dutch' Schrier, Barry Brown, Bruce Brandt, and the rest of the staff of Substation Curacao for their assistance in the field. The project was funded in part by the Smithsonian Peter Buck Fellowship to LT. Funding for the Smithsonian Institution's Deep Reef Observation Project was provided internally by the Consortium for Understanding and Sustaining a Biodiverse Planet to CCB, the Competitive Grants for the Promotion of Science program to CCB and DRR, the Herbert R. and Evelyn Axelrod Endowment Fund for systematic ichthyology to CCB, and externally by the Prince Albert II of Monaco Foundation. This study is Ocean Heritage Foundation/Curacao Sea Aquarium/Substation Curacao contribution number OHF/CSA/SC#24. NR 25 TC 2 Z9 2 U1 1 U2 3 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 596 BP 143 EP 156 DI 10.3897/zookeys.596.8217 PG 14 WC Zoology SC Zoology GA DO8TC UT WOS:000378055700010 PM 27408581 ER PT J AU Henry, TJ AF Henry, Thomas J. TI A NEW SPECIES OF THE STILT BUG GENUS GAMPSOCORIS FROM SENEGAL AND NEW GENERIC COMBINATION FOR GAMPSOCORIS GOMERANUS (HEMIPTERA: HETEROPTERA: BERYTIDAE) SO ENTOMOLOGICA AMERICANA LA English DT Article DE Insecta; Hemiptera; Gampsocorinae; stilt bugs; distribution; Africa AB The relationships the African genera Gampsoacantha Josifov and Stusak, 1987, Gampsocoris Fuss, 1852, and Micrometacanthus Lindberg, 1985 (Berytidae: Gampsocorinae) are discussed. Gampsocoris gomeranus Wagner, 1965, having a median anterior spine and three basal processes on the pronotum and a short, round antennal segment IV, is transferred to the genus Micrometacanthus (M. gomeranus, new combination). Gampsocoris linnavuorii, new species, from Senegal is diagnosed, described, and illustrated to help distinguish it from all other species of Gampsocoris. A checklist of African Gampsocorinae is given. C1 [Henry, Thomas J.] Smithsonian Inst, Systemat Entomol Lab, USDA ARS, Natl Museum Nat Hist,MRC 0168, Washington, DC 20013 USA. RP Henry, TJ (reprint author), Smithsonian Inst, Systemat Entomol Lab, USDA ARS, Natl Museum Nat Hist,MRC 0168, Washington, DC 20013 USA. EM thomas.henry@ars.usda.gov NR 21 TC 0 Z9 0 U1 1 U2 1 PU NEW YORK ENTOMOLOGICAL SOC INC PI NEW YORK PA C/O AMER MUSEUM NAT HIST 79TH & CENTRAL PARK WEST, NEW YORK, NY 10024 USA SN 1947-5136 EI 1947-5144 J9 ENTOMOL AM-NY JI Entomol. Am. PY 2016 VL 122 IS 1-2 BP 24 EP 30 PG 7 WC Entomology SC Entomology GA DN7SZ UT WOS:000377280300003 ER PT J AU Blundell, R Mehdi, I AF Blundell, Raymond Mehdi, Imran TI Introduction to the Mini-Special-Issue on the 26th International Symposium on Space Terahertz Technology (ISSTT) SO IEEE TRANSACTIONS ON TERAHERTZ SCIENCE AND TECHNOLOGY LA English DT Editorial Material C1 [Blundell, Raymond] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Mehdi, Imran] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA. RP Blundell, R (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. NR 0 TC 0 Z9 0 U1 1 U2 1 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 2156-342X J9 IEEE T THZ SCI TECHN JI IEEE Trans. Terahertz Sci. Technol. PD JAN PY 2016 VL 6 IS 1 SI SI BP 113 EP 114 DI 10.1109/TTHZ.2015.2507759 PG 2 WC Engineering, Electrical & Electronic; Optics; Physics, Applied SC Engineering; Optics; Physics GA DO3LB UT WOS:000377682000015 ER PT J AU Montazeri, S Grimes, PK Tong, CYE Bardin, JC AF Montazeri, Shirin Grimes, Paul K. Tong, Cheuk-Yu Edward Bardin, Joseph C. TI A 220-GHz SIS Mixer Tightly Integrated With a Sub-Hundred-Microwatt SiGe IF Amplifier SO IEEE TRANSACTIONS ON TERAHERTZ SCIENCE AND TECHNOLOGY LA English DT Article; Proceedings Paper CT 26th International Symposium on Space Terahertz Technology (ISSTT) CY MAR 16-18, 2015 CL Smithsonian Astrophys Observ, Cambridge, MA SP Harvard Coll Observ HO Smithsonian Astrophys Observ DE Cryogenic; focal plane array; heterodyne receiver; low-noise amplifier; silicon germanium; superconductor-insulator-superconductor (SIS) mixer ID RECEIVERS AB Future kilopixel-scale heterodyne focal plane arrays based on superconductor-insulator-superconductor (SIS) mixers will require submilliwatt power consumption low-noise amplifiers (LNAs) which are tightly integrated with the mixers. In this paper, an LNA that is optimized for direct connection to a 220-GHz SIS mixer chip and requires less than 100 mu W of dc power is reported. The amplifier design process is described, and measurement results are presented. It is shown that, when pumped at local oscillator frequencies between 214 and 226 GHz, the mixer/amplifier module achieves a double-sideband system noise temperature between 35 and 50 K over the 3.3-6 GHz IF frequency range while requiring just 90 mu W of dc power. Moreover, the potential to further reduce the power consumption is explored and successful operation is demonstrated for LNA power consumption as low as 60 mu W. C1 [Montazeri, Shirin; Bardin, Joseph C.] Univ Massachusetts, Amherst, MA 01003 USA. [Grimes, Paul K.; Tong, Cheuk-Yu Edward] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. RP Bardin, JC (reprint author), Univ Massachusetts, Amherst, MA 01003 USA. EM etong@cfa.harvard.edu; jbardin@engin.umass.edu OI Tong, Edward/0000-0002-7736-4203 NR 23 TC 3 Z9 3 U1 2 U2 2 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 2156-342X J9 IEEE T THZ SCI TECHN JI IEEE Trans. Terahertz Sci. Technol. PD JAN PY 2016 VL 6 IS 1 SI SI BP 133 EP 140 DI 10.1109/TTHZ.2015.2498041 PG 8 WC Engineering, Electrical & Electronic; Optics; Physics, Applied SC Engineering; Optics; Physics GA DO3LB UT WOS:000377682000019 ER PT J AU Zeng, LZ Tong, CE Grimes, PK AF Zeng, Lingzhen Tong, Cheukyu Edward Grimes, Paul K. TI Experimental Verification of the Fundamental Gaussian Beam Properties of Smooth-Walled Feedhorns SO IEEE TRANSACTIONS ON TERAHERTZ SCIENCE AND TECHNOLOGY LA English DT Article; Proceedings Paper CT 26th International Symposium on Space Terahertz Technology (ISSTT) CY MAR 16-18, 2015 CL Smithsonian Astrophys Observ, Cambridge, MA SP Harvard Coll Observ HO Smithsonian Astrophys Observ DE Horn antennas; millimeter-wave measurements; millimeter-wave propagation; near-field radiation pattern ID HORN; MILLIMETER AB We report the measurements of near-field patterns for three smooth-walled feedhorns and a conventional corrugated feedhorn at different wavelengths. The measured vector beam patterns are fitted into fundamental Gaussian beam modes. We verify our measurement by comparing the corrugated horn result with its well-established theoretical pattern. The positions and diameters of the beam waists of all of the measured horns are derived from the fitted fundamental Gaussian beam and are in good agreement with those obtained from numerical calculations. C1 [Zeng, Lingzhen; Tong, Cheukyu Edward; Grimes, Paul K.] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA. RP Zeng, LZ (reprint author), Smithsonian Astrophys Observ, Cambridge, MA 02138 USA. EM lingzhen.zeng@cfa.harvard.edu OI Tong, Edward/0000-0002-7736-4203 NR 16 TC 0 Z9 0 U1 1 U2 1 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 2156-342X J9 IEEE T THZ SCI TECHN JI IEEE Trans. Terahertz Sci. Technol. PD JAN PY 2016 VL 6 IS 1 SI SI BP 163 EP 168 DI 10.1109/TTHZ.2015.2504789 PG 6 WC Engineering, Electrical & Electronic; Optics; Physics, Applied SC Engineering; Optics; Physics GA DO3LB UT WOS:000377682000023 ER PT J AU Philip, S Martin, RV Keller, CA AF Philip, Sajeev Martin, Randall V. Keller, Christoph A. TI Sensitivity of chemistry-transport model simulations to the duration of chemical and transport operators: a case study with GEOS-Chem v10-01 SO GEOSCIENTIFIC MODEL DEVELOPMENT LA English DT Article ID SEA-SALT AEROSOLS; UNITED-STATES; GRID RESOLUTION; TROPOSPHERIC CHEMISTRY; ATMOSPHERIC MODELS; DRY DEPOSITION; NORTH-AMERICA; SMVGEAR-II; OZONE; IMPACT AB Chemistry-transport models involve considerable computational expense. Fine temporal resolution offers accuracy at the expense of computation time. Assessment is needed of the sensitivity of simulation accuracy to the duration of chemical and transport operators. We conduct a series of simulations with the GEOS-Chem chemistry-transport model at different temporal and spatial resolutions to examine the sensitivity of simulated atmospheric composition to operator duration. Subsequently, we compare the species simulated with operator durations from 10 to 60 min as typically used by global chemistry-transport models, and identify the operator durations that optimize both computational expense and simulation accuracy. We find that longer continuous transport operator duration increases concentrations of emitted species such as nitrogen oxides and carbon monoxide since a more homogeneous distribution reduces loss through chemical reactions and dry deposition. The increased concentrations of ozone precursors increase ozone production with longer transport operator duration. Longer chemical operator duration decreases sulfate and ammonium but increases nitrate due to feedbacks with in-cloud sulfur dioxide oxidation and aerosol thermodynamics. The simulation duration decreases by up to a factor of 5 from fine (5 min) to coarse (60 min) operator duration. We assess the change in simulation accuracy with resolution by comparing the root mean square difference in ground-level concentrations of nitrogen oxides, secondary inorganic aerosols, ozone and carbon monoxide with a finer temporal or spatial resolution taken as "truth". Relative simulation error for these species increases by more than a factor of 5 from the shortest (5 min) to longest (60 min) operator duration. Chemical operator duration twice that of the transport operator duration offers more simulation accuracy per unit computation. However, the relative simulation error from coarser spatial resolution generally exceeds that from longer operator duration; e.g., degrading from 2 degrees x 2.5 degrees to 4 degrees x 5 degrees increases error by an order of magnitude. We recommend prioritizing fine spatial resolution before considering different operator durations in offline chemistry-transport models. We encourage chemistry-transport model users to specify in publications the durations of operators due to their effects on simulation accuracy. C1 [Philip, Sajeev; Martin, Randall V.] Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. [Martin, Randall V.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Keller, Christoph A.] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02138 USA. [Keller, Christoph A.] Univ Space Res Assoc, GESTAR, NASA, GMAO, Code 610-1, Greenbelt, MD USA. RP Philip, S (reprint author), Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. EM sj207331@dal.ca RI Martin, Randall/C-1205-2014; Chem, GEOS/C-5595-2014 OI Martin, Randall/0000-0003-2632-8402; FU National Science and Engineering Research Council, Canada; Atlantic Computational Excellence Network FX We thank Colette Heald, Daniel Jacob and Patrick Kim for useful comments at the early stages of this research. We are grateful to three anonymous reviewers for helpful comments. This work was supported by the National Science and Engineering Research Council, Canada, and the Atlantic Computational Excellence Network (http://www.ace-net.ca/). NR 81 TC 1 Z9 1 U1 4 U2 10 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1991-959X EI 1991-9603 J9 GEOSCI MODEL DEV JI Geosci. Model Dev. PY 2016 VL 9 IS 5 BP 1683 EP 1695 DI 10.5194/gmd-9-1683-2016 PG 13 WC Geosciences, Multidisciplinary SC Geology GA DN3BR UT WOS:000376937800003 ER PT J AU Konstantinov, AS AF Konstantinov, Alexander S. TI Possible living fossil in Bolivia: A new genus of flea beetles with modified hind legs (Coleoptera, Chrysomelidae, Galerucinae, Alticini) SO ZOOKEYS LA English DT Article DE Flea beetles; fossil beetles; leaping; structure and function of hind leg; Neotropics ID BALTIC AMBER; EOCENE AB A new genus (Chanealtica) with three new species (C. cuevas, C. ellimon, and C. maxi) from Bolivia is described and illustrated. It is compared with Aphthonoides Jacoby, 1885, Argopistes Motschulsky, 1860, Metroserrapha Bechyne, 1958, Psylliodes Berthold, 1827 and Psyllototus Nadein, 2010. Remarkably, based on the available characters, among all the flea beetles, Chanealtica is mostly similar to an extinct genus Psyllototus. A discussion of diversity and function of the hind leg in flea beetles is provided. C1 [Konstantinov, Alexander S.] Smithsonian Inst, USDA ARS, Natl Museum Nat Hist, Systemat Entomol Lab, MRC 168, Washington, DC 20560 USA. RP Konstantinov, AS (reprint author), Smithsonian Inst, USDA ARS, Natl Museum Nat Hist, Systemat Entomol Lab, MRC 168, Washington, DC 20560 USA. EM alex.konstantinov@ars.usda.gov NR 16 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 592 BP 103 EP 120 DI 10.3897/zookeys.592.8180 PG 18 WC Zoology SC Zoology GA DM6FD UT WOS:000376445100005 PM 27408546 ER PT J AU Croft, B Martin, RV Leaitch, WR Tunved, P Breider, TJ D'Andrea, SD Pierce, JR AF Croft, Betty Martin, Randall V. Leaitch, W. Richard Tunved, Peter Breider, Thomas J. D'Andrea, Stephen D. Pierce, Jeffrey R. TI Processes controlling the annual cycle of Arctic aerosol number and size distributions SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID CLOUD CONDENSATION NUCLEI; OFF-LINE MODEL; BLACK CARBON; CCN CONCENTRATIONS; ASSIMILATED METEOROLOGY; TROPOSPHERIC AEROSOL; MICROPHYSICS MODEL; PARTICLE FORMATION; ORGANIC-COMPOUNDS; ZEPPELIN STATION AB Measurements at high-Arctic sites (Alert, Nunavut, and Mt. Zeppelin, Svalbard) during the years 2011 to 2013 show a strong and similar annual cycle in aerosol number and size distributions. Each year at both sites, the number of aerosols with diameters larger than 20 nm exhibits a minimum in October and two maxima, one in spring associated with a dominant accumulation mode (particles 100 to 500 nm in diameter) and a second in summer associated with a dominant Aitken mode (particles 20 to 100 nm in diameter). Seasonal-mean aerosol effective diameter from measurements ranges from about 180 in summer to 260 nm in winter. This study interprets these annual cycles with the GEOS-Chem-TOMAS global aerosol microphysics model. Important roles are documented for several processes (new-particle formation, coagulation scavenging in clouds, scavenging by precipitation, and transport) in controlling the annual cycle in Arctic aerosol number and size. Our simulations suggest that coagulation scavenging of interstitial aerosols in clouds by aerosols that have activated to form cloud droplets strongly limits the total number of particles with diameters less than 200 nm throughout the year. We find that the minimum in total particle number in October can be explained by diminishing new-particle formation within the Arctic, limited transport of pollution from lower latitudes, and efficient wet removal. Our simulations indicate that the summertime-dominant Aitken mode is associated with efficient wet removal of accumulation-mode aerosols, which limits the condensation sink for condensable vapours. This in turn promotes new-particle formation and growth. The dominant accumulation mode during spring is associated with build up of transported pollution from outside the Arctic coupled with less-efficient wet-removal processes at colder temperatures. We recommend further attention to the key processes of new-particle formation, interstitial coagulation, and wet removal and their delicate interactions and balance in size-resolved aerosol simulations of the Arctic to reduce uncertainties in estimates of aerosol radiative effects on the Arctic climate. C1 [Croft, Betty; Martin, Randall V.; Pierce, Jeffrey R.] Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. [Martin, Randall V.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Leaitch, W. Richard] Environm & Climate Change Canada, Climate Res Directorate, Toronto, ON, Canada. [Tunved, Peter] Stockholm Univ, Dept Environm Sci & Analyt Chem, S-10691 Stockholm, Sweden. [Breider, Thomas J.] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02138 USA. [D'Andrea, Stephen D.; Pierce, Jeffrey R.] Colorado State Univ, Dept Atmospher Sci, Ft Collins, CO 80523 USA. RP Croft, B (reprint author), Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. EM betty.croft@dal.ca RI Pierce, Jeffrey/E-4681-2013; Martin, Randall/C-1205-2014; Chem, GEOS/C-5595-2014 OI Pierce, Jeffrey/0000-0002-4241-838X; Martin, Randall/0000-0003-2632-8402; FU Climate Change and Atmospheric Research Program at NSERC Canada FX The authors acknowledge the financial support provided for NETCARE through the Climate Change and Atmospheric Research Program at NSERC Canada. Thanks to Sangeeta Sharma, Desiree Toom, Andrew Platt, and the Alert operators for supporting the Alert observations. We are also grateful to Ilona Riipinen, Jan Julin, and Tinya Olenius for helpful discussions and for providing the Atmospheric Cluster Dynamics Code (ACDC), applied in our GEOS-Chem-TOMAS simulations. NR 69 TC 6 Z9 6 U1 7 U2 18 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 6 BP 3665 EP 3682 PG 18 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DK1VG UT WOS:000374702300001 ER PT J AU Wheeler, GS Mattison, ED Metz, MA Pratt, PD Purcell, MF AF Wheeler, G. S. Mattison, E. D. Metz, M. A. Pratt, P. D. Purcell, M. F. TI Host range of the defoliator Strepsicrates sp is too broad for biological control of the invasive weed Rhodomyrtus tomentosa SO BIOCONTROL SCIENCE AND TECHNOLOGY LA English DT Article DE Biological control of weeds; rose myrtle; host range determination; Myrtaceae; Tortricidae ID CONTROL AGENT; MYRTACEAE AB In its native range the invasive weed, Rhodomyrtus tomentosa is host to a suite of herbivores. One, Strepsicrates sp. (Lepidoptera: Tortricidae), was collected in China in 2014, introduced under quarantine in Florida, USA, and tested against related species to determine its host range and suitability for biological control. In no-choice tests, neonates fed and completed development to the pupal stage on several species of Myrtaceae, including the target weed R. tomentosa, the exotics Melaleuca quinquenervia, and Eucalyptus camaldulensis, and three native species, Eugenia axillaris, Mosiera longipes and Morella cerifera (Myricaceae). Due to the broad host range exhibited in quarantine testing, this species will not be pursued as a biological control agent of R. tomentosa. C1 [Wheeler, G. S.; Mattison, E. D.] USDA ARS, Invas Plant Res Lab, Ft Lauderdale, FL USA. [Metz, M. A.] USDA ARS, Smithsonian Inst, Systemat Entomol Lab, Washington, DC 20250 USA. [Pratt, P. D.] USDA ARS, Exot & Invas Plant Res Lab, Albany, CA USA. [Purcell, M. F.] USDA ARS, CSIRO Ecosyst Sci, Australian Biol Control Lab, Brisbane, Qld, Australia. RP Wheeler, GS (reprint author), USDA ARS, Invas Plant Res Lab, Ft Lauderdale, FL USA. EM greg.wheeler@ars.usda.gov FU Florida Fish and Wildlife Conservation Commission [08250]; South Florida Water Management District [4600001427]; USDA/ARS [6629050] FX This project was partially funded by Florida Fish and Wildlife Conservation Commission [08250], South Florida Water Management District [4600001427], and USDA/ARS [6629050]. NR 19 TC 0 Z9 0 U1 2 U2 3 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0958-3157 EI 1360-0478 J9 BIOCONTROL SCI TECHN JI Biocontrol Sci. Technol. PY 2016 VL 26 IS 6 BP 861 EP 865 DI 10.1080/09583157.2015.1130799 PG 5 WC Biotechnology & Applied Microbiology; Entomology SC Biotechnology & Applied Microbiology; Entomology GA DJ9SA UT WOS:000374552000010 ER PT J AU Rivera-Correa, M Lamadrid-Feris, F Crawford, AJ AF Rivera-Correa, Mauricio Lamadrid-Feris, Faride Crawford, Andrew J. TI A new small golden frog of the genus Pristimantis (Anura: Craugastoridae) from an Andean cloud forest of Colombia SO AMPHIBIA-REPTILIA LA English DT Article DE advertisement call; Amphibia; Brachycephaloidea; Eastern Cordillera; morphology; South America; Terrarana ID ADVERTISEMENT CALL; PHYLOGENETIC TREES; DNA-SEQUENCES; ELEUTHERODACTYLUS; BRACHYCEPHALIDAE; STRABOMANTIDAE; SYSTEMATICS; DIVERSITY; EVOLUTION; ALIGNMENT AB A new species of Pristimantis is described from an Andean cloud forest at 2650 m in the Cordillera Oriental of Colombia. Pristimantis dorado sp. nov. is similar to and could be closely related to P. acutirostris, but can be readily distinguished from this latter species by the absence of a tympanic annulus, vocal slits, vocal sac and reticulations on concealed surfaces, and by having a metallic gold iris with a brown horizontal streak. The phylogenetic position of the new species is recovered and we provide its advertisement call, which this species manages to emit despite lacking a vocal sac and vocal slits. This discovery reminds us that despite the extensive research on the alpha-taxonomy of Pristimantis in Colombia, fieldwork in high montane forests continues to yield previously unknown species. C1 [Rivera-Correa, Mauricio] Univ Antioquia, Inst Biol, Grp Herpetol Antioquia, Medellin 1226, Colombia. [Rivera-Correa, Mauricio] Univ Antioquia, Secc Oriente, Regionalizac, Km 6 Via Rionegro La Ceja, Carmen De Viboral, Colombia. [Lamadrid-Feris, Faride] Univ Atlantico, Fac Ciencias Basicas, Programa Biol, Barranquilla, Colombia. [Crawford, Andrew J.] Univ Los Andes, Dept Biol Sci, Bogota 4976, Colombia. [Crawford, Andrew J.] Smithsonian Trop Res Inst, Apartado 0843-03092, Panama City, Panama. RP Rivera-Correa, M (reprint author), Univ Antioquia, Inst Biol, Grp Herpetol Antioquia, Medellin 1226, Colombia.; Rivera-Correa, M (reprint author), Univ Antioquia, Secc Oriente, Regionalizac, Km 6 Via Rionegro La Ceja, Carmen De Viboral, Colombia. EM mauriciorivera79@yahoo.com.ar FU Bogota's Aqueduct water company [7-24100-925-2007]; Conservation International - Colombia [7-24100-925-2007]; Ecopetrol [156-09]; Consejo Nacional de Investigaciones Cientificas y Tecnicas de Argentina (CONICET) FX We thank M. Rada, S. Castroviejo, D. Gonzalez, O. Nieto and I. Sanchez for field assistance and A. Munoz-Ortiz for conducting all molecular laboratory work. We are grateful to J. M. Daza (MHUA), J. D. Lynch (ICN) and S. Ron (QCAZ) for allowing access to collections under their care. We are thankful to S. Castroviejo-Fisher for allowing us to use his photographs. Edgar Lehr and Karl-Heinz Jungfer kindly provided suggestions and comments on the manuscript. This biological collection was made with financial support from the technology cooperation agreement No. 7-24100-925-2007 between Bogota's Aqueduct water company and Conservation International - Colombia. Additional samples were obtained and DNA-sequenced under research and collecting permit no. 15 and access to genetic resources permit no. 44 to A.J.C. by the Ministerio de Ambiente, Vivienda y Desarrollo Territorial. Laboratory work was financed by grant no. 156-09 from Ecopetrol. Special thanks to J.V. Rodriguez-Mahecha for supporting the study of the diversity of amphibians in Colombia and to S. Guerra and P. Bejarano for their interest and support to make this article a product of the conservation corridor. Postdoctoral Fellow support for M.R.C. was provided by Consejo Nacional de Investigaciones Cientificas y Tecnicas de Argentina (CONICET). NR 54 TC 1 Z9 1 U1 3 U2 3 PU BRILL ACADEMIC PUBLISHERS PI LEIDEN PA PLANTIJNSTRAAT 2, P O BOX 9000, 2300 PA LEIDEN, NETHERLANDS SN 0173-5373 EI 1568-5381 J9 AMPHIBIA-REPTILIA JI Amphib. Reptil. PY 2016 VL 37 IS 2 BP 153 EP 166 PG 14 WC Zoology SC Zoology GA DL1SL UT WOS:000375412200002 ER PT J AU Luther, DA Phillips, J Derryberry, EP AF Luther, David A. Phillips, Jennifer Derryberry, Elizabeth P. TI Not so sexy in the city: urban birds adjust songs to noise but compromise vocal performance SO BEHAVIORAL ECOLOGY LA English DT Article DE noise pollution; sexual selection; signal trade-off; vocal performance ID WHITE-CROWNED SPARROW; RED-WINGED BLACKBIRDS; ANTHROPOGENIC NOISE; ACOUSTIC COMMUNICATION; CORRELATED EVOLUTION; ROADSIDE HABITATS; TRAFFIC NOISE; HOUSE FINCH; GREAT TITS; SIGNALS AB Anthropogenic noise affects the behavior of a variety of animal taxa around the world. In many taxa, minimum frequencies of acoustic signals increase with ambient noise levels, and males and females respond less strongly to these adjusted signals. Lower response may be due to higher minimum frequencies or to the associated decrease in frequency bandwidth. There is a performance challenge to producing notes rapidly at a wide bandwidth, and any reduction in bandwidth necessarily reduces the performance value. This measure of vocal performance is a trait under sexual selection in many taxa. We investigated the relationship between anthropogenic noise amplitude and male white-crowned sparrow vocal performance in San Francisco, CA. Males on louder territories produced songs at higher minimum frequencies but also with reduced bandwidth and lower vocal performance. These results suggest that behavioral adjustments to anthropogenic noise reduce vocal performance of songs. We conducted playback experiments to test if lower responses to urban songs are due to higher minimum frequencies or to narrower bandwidths. Males responded more strongly to normal than to reduced bandwidth songs, but equally to high-and low-pass filtered songs. Our results therefore suggest that reduced bandwidth and performance-not higher minimum frequency-could be the reason that urban birds are less responsive to songs adjusted for anthropogenic noise. Ultimately, the lower vocal performance of birds on territories with high levels of anthropogenic noise could result in fewer mating opportunities and more challenges in defending their territory. C1 [Luther, David A.] George Mason Univ, Dept Biol, Fairfax, VA 22030 USA. [Luther, David A.] Smithsonian Inst, Natl Zool Pk, Smithsonian Migratory Bird Ctr, Washington, DC 20008 USA. [Phillips, Jennifer; Derryberry, Elizabeth P.] Tulane Univ, Dept Ecol & Evolutionary Biol, New Orleans, LA 70118 USA. RP Luther, DA (reprint author), George Mason Univ, Dept Biol, Fairfax, VA 22030 USA.; Luther, DA (reprint author), Smithsonian Inst, Natl Zool Pk, Smithsonian Migratory Bird Ctr, Washington, DC 20008 USA. EM dluther@gmu.edu FU National Science Foundation Integrative Organismal Systems [1354756] FX Research was funded by National Science Foundation Integrative Organismal Systems (award number 1354756). NR 64 TC 5 Z9 5 U1 16 U2 33 PU OXFORD UNIV PRESS INC PI CARY PA JOURNALS DEPT, 2001 EVANS RD, CARY, NC 27513 USA SN 1045-2249 EI 1465-7279 J9 BEHAV ECOL JI Behav. Ecol. PD JAN-FEB PY 2016 VL 27 IS 1 BP 332 EP 340 DI 10.1093/beheco/arv162 PG 9 WC Behavioral Sciences; Biology; Ecology; Zoology SC Behavioral Sciences; Life Sciences & Biomedicine - Other Topics; Environmental Sciences & Ecology; Zoology GA DK2TW UT WOS:000374768300046 ER PT J AU Chutter, CM Redmond, LJ Cooper, NW Dolan, AC Duffield, D Murphy, MT AF Chutter, Christopher M. Redmond, Lucas J. Cooper, Nathan W. Dolan, Amy C. Duffield, Deborah Murphy, Michael T. TI Paternal behaviour in a socially monogamous but sexually promiscuous passerine bird SO BEHAVIOUR LA English DT Article DE differential allocation; extra-pair paternity; male quality; nesting density; paternal investment; parental behaviour ID MALE PARENTAL CARE; EXTRA-PAIR PATERNITY; EASTERN KINGBIRDS; DIFFERENTIAL ALLOCATION; SAVANNA SPARROWS; REPRODUCTIVE SUCCESS; COLLARED FLYCATCHER; COMMON YELLOWTHROAT; BIPARENTAL CARE; REED BUNTINGS AB We documented parental behaviour and paternity of eastern kingbirds (Tyrannus tyrannus) to test the predictions that paternal care would decline with increasing loss of paternity, increasing nesting density (a proxy for probability of paternity loss), male quality, and number of fertile females available in the population. Extra-pair young were found in 58% of 45 nests for which behaviour was recorded and a higher proportion of young were extra-pair as nesting density increased. Male feeding rate declined with increasing nesting density and male quality, but neither feeding rate nor a composite measure of paternal behaviour varied with number of fertile females or paternity. Although alternative explanations exist, one interpretation of the reduced paternal care at high nesting density was that it was a response to perceived threats of paternity loss. The ultimate basis for the lower paternal effort of higher quality males is unclear but we discuss several possible explanations. C1 [Chutter, Christopher M.; Redmond, Lucas J.; Cooper, Nathan W.; Dolan, Amy C.; Duffield, Deborah; Murphy, Michael T.] Portland State Univ, Dept Biol, Portland, OR 97201 USA. [Chutter, Christopher M.] Minist Adv Educ, 313-4529 West Saanich Rd, Victoria, BC V8Z 3G3, Canada. [Redmond, Lucas J.] Penn State Univ, Schuylkill Campus,200 Univ Dr, Schuylkill Haven, PA 17972 USA. [Cooper, Nathan W.] Natl Zool Pk, Migratory Bird Ctr, Smithsonian Conservat Biol Inst, POB 37012, Washington, DC 20013 USA. [Dolan, Amy C.] Northern State Univ, Dept Biol, MJ224,1200 South Jay St, Aberdeen, SD 57401 USA. RP Murphy, MT (reprint author), Portland State Univ, Dept Biol, Portland, OR 97201 USA. EM murphym@pdx.edu OI Cooper, Nathan/0000-0002-4667-1542 FU National Science Foundation [IOS-0539370]; NSERC [389391-2010]; American Ornithologists' Union; Animal Behaviour Society FX Our work was funded by a National Science Foundation (grant number IOS-0539370; MTM), an NSERC grant (application number 389391-2010; CMC), and additional sources that include the Forbes-Lea Fund of Portland State University, The Frank M. Chapman Fund of the American Museum of Natural History, Student Research Awards from the American Ornithologists' Union, and the Animal Behaviour Society. Without their support this work would not have been possible. We thank all of the members of the various kingbird research teams that have assembled over the years for the diligence and hard work expended in capturing and marking birds, and in collecting the data that are the foundation for our paper. Luis Ruedas allowed us to borrow his canoe year-after-year to conduct surveys along the river. We are also thankful for the cooperation of the staff of Malheur National Wildlife Refuge, and in particular acknowledge the permission granted by Chief Biologists Richard Roy and James Daystyck to work on the refuge. Cal and Alice Elshoff provided great friendship, as did the staff at Malheur Field Station (Duncan Evered and Lyla Messick). Lastly, we thank two anonymous reviewers for helping to improve our presentation. NR 76 TC 0 Z9 0 U1 8 U2 16 PU BRILL ACADEMIC PUBLISHERS PI LEIDEN PA PLANTIJNSTRAAT 2, P O BOX 9000, 2300 PA LEIDEN, NETHERLANDS SN 0005-7959 EI 1568-539X J9 BEHAVIOUR JI Behaviour PY 2016 VL 153 IS 4 BP 443 EP 466 DI 10.1163/1568539X-00003359 PG 24 WC Behavioral Sciences; Zoology SC Behavioral Sciences; Zoology GA DK3RY UT WOS:000374836300004 ER PT J AU Dominguez, M Escalante, I Carrasco-Rueda, F Figuerola-Hernandez, CE Ayup, MM Umana, MN Ramos, D Gonzalez-Zamora, A Brizuela, C Delgado, W Pacheco-Esquivel, J AF Dominguez, Marisol Escalante, Ignacio Carrasco-Rueda, Farah Figuerola-Hernandez, Cielo E. Marta Ayup, Maria Umana, Maria Natalia Ramos, Daniel Gonzalez-Zamora, Arturo Brizuela, Carolina Delgado, Willy Pacheco-Esquivel, Jessica TI Losing legs and walking hard: effects of autotomy and different substrates in the locomotion of harvestmen in the genus Prionostemma SO JOURNAL OF ARACHNOLOGY LA English DT Article DE Costa Rica; Eupnoi; Opiliones; Sclerosomatidae ID LEIOBUNUM-VITTATUM ARACHNIDA; NEOTROPICAL HARVESTMEN; TAIL AUTOTOMY; COSTA-RICA; OPILIONES; REGENERATION; PERFORMANCE; ARTHROPODS; NIGRIPES; SURFACES AB Autotomy, the strategy of voluntarily releasing a leg during an encounter with a potential predator or in agonistic interactions between conspecifics, is common in animals. The potential costs of this behavior have been scarcely studied. In addition, locomotion and substrate-dependent performance might be affected by autotomy. We did a comparative and observational study to investigate whether losing legs affects the escape speed and trajectory of harvestmen in the genus Prionostemma Pocock, 1903 (Eupnoi: Sclerosomatidae) on different substrates: soil (the least roughened), smooth bark and mossy bark (the most roughened) in a tropical premontane forest in Costa Rica. We observed that 71% of the individuals found were missing at least one leg. Harvestmen, regardless of leg condition, walked faster and made fewer turns in their trajectory in the soil. While climbing, they were faster on smooth bark than in moss. On all substrates, autotomized individuals were slower and had a more erratic trajectory than intact ones. The type of missing legs (sensory or locomotor) had no influence on the speed or trajectory. We experimentally induced autotomy and found that walking speed on soil decreases if individuals lose a leg. Our findings confirm that losing legs affects locomotion, and we provide novel insights on how locomotion in these harvestmen depends on surface roughness. Our data suggest that moss could be a type of substrate that requires more elaborate skills in balance, orientation and texture recognition than smooth bark. C1 [Dominguez, Marisol] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Ecol Genet & Evoluc, Buenos Aires, DF, Argentina. [Dominguez, Marisol] Univ Buenos Aires, Fac Ciencias Exactas & Nat, IEGEBA CONICET, Buenos Aires, DF, Argentina. [Escalante, Ignacio] Univ Costa Rica, Escuela Biol, San Jose, Costa Rica. [Carrasco-Rueda, Farah] Smithsonian Inst, Natl Zool Pk, Smithsonian Conservat Biol Inst, Ctr Conservat Educ & Sustainabil, Washington, DC 20008 USA. [Figuerola-Hernandez, Cielo E.] Univ Puerto Rico Rio Piedras, Biol Dept, San Juan, PR 00931 USA. [Marta Ayup, Maria] Univ Nacl Tucuman, Inst Ecol Reg, San Miguel De Tucuman, Argentina. [Umana, Maria Natalia] Michigan State Univ, Dept Plant Biol, E Lansing, MI 48824 USA. [Ramos, Daniel] Univ Laica Eloy Alfaro de Manabi Manta, Manta, Ecuador. [Gonzalez-Zamora, Arturo] Inst Ecol AC, Xalapa, Veracruz, Mexico. [Brizuela, Carolina] Univ Nacl, Escuela Ciencias Biol, San Jose, Costa Rica. [Delgado, Willy] Univ Nacl San Agustin Arequipa, Museo Hist Nat, Arequipa, Peru. [Pacheco-Esquivel, Jessica] Pontificia Univ Catolica Ecuador, Pichincha, Ecuador. [Escalante, Ignacio] Univ Calif Berkeley, Dept Environm Sci Policy & Management, Berkeley, CA 94720 USA. [Carrasco-Rueda, Farah] Univ Florida, Sch Nat Resources & Environm, Gainesville, FL USA. [Gonzalez-Zamora, Arturo] Univ Veracruzana, Inst Invest Biol, Xalapa 91000, Veracruz, Mexico. RP Dominguez, M (reprint author), Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Ecol Genet & Evoluc, Buenos Aires, DF, Argentina.; Dominguez, M (reprint author), Univ Buenos Aires, Fac Ciencias Exactas & Nat, IEGEBA CONICET, Buenos Aires, DF, Argentina. EM soldominguez@ege.fcen.uba.ar FU Organization for Tropical Studies and Las Cruces Biological Station; Biology Department of the UPR at Rio Piedras; Universidad de Antioquia, Colombia; Center For Conservation Education and Sustainability, Smithsonian Conservation Biology Institute; CONCYTEC FX We thank A.G. Farji-Brener, F. Chinchilla, and G. Barrantes for their assistance in the design, analysis and interpretation of this project. E. Triana provided great suggestions to improve the project, as well as field assistance. We thank the Organization for Tropical Studies and Las Cruces Biological Station for providing housing, logistics, transportation and financial support during this project. V.R. Townsend, Jr., Joel Wixson, Elizabeth C. Braun, and two anonymous reviewers provided useful comments to improve this project. The Biology Department of the UPR at Rio Piedras provided financial support to CF. The Universidad de Antioquia, Colombia provided financial support to DG-R, and the Center For Conservation Education and Sustainability, Smithsonian Conservation Biology Institute and CONCYTEC for the financial support to FC-R. NR 33 TC 0 Z9 0 U1 4 U2 5 PU AMER ARACHNOLOGICAL SOC PI COLLEGE PARK PA UNIV MARYLAND, DEPT ENTOMOLOGY, 4112 PLANT SCIENCES BLDG, COLLEGE PARK, MD 20742-4454 USA SN 0161-8202 EI 1937-2396 J9 J ARACHNOL JI J. Arachnol. PY 2016 VL 44 IS 1 BP 76 EP 82 PG 7 WC Entomology SC Entomology GA DK8HM UT WOS:000375167800009 ER PT J AU Cardoso-Martinez, F de la Rosa, JM Diaz-Marrero, AR Darias, J D'Croz, L Jimenez-Anton, MD Corral, MJ Garcia, R Alunda, JM Cueto, M AF Cardoso-Martinez, Faviola de la Rosa, Jose M. Diaz-Marrero, Ana R. Darias, Jose D'Croz, Luis Dolores Jimenez-Anton, M. Jesus Corral, M. Garcia, Rocio Alunda, Jose M. Cueto, Mercedes TI Oxysterols from an octocoral of the genus Gorgonia from the eastern Pacific of Panama SO RSC ADVANCES LA English DT Article ID GROWTH-INHIBITORY ACTIVITY; MARINE NATURAL-PRODUCTS; CORAL NEPHTHEA-ERECTA; SOFT CORAL; POLYHYDROXYLATED STEROIDS; CELL-GROWTH; POLYOXYGENATED STEROIDS; 19-OXYGENATED STEROIDS AB Eighteen new oxysterols have been isolated from a previously undescribed octocoral collected from the eastern Pacific of Panama. Their structures were determined based on spectroscopic evidence. The absolute configuration was established by derivatization with (R)- and (S)-MPA. Antimicrobial and antileishmanial effects were evaluated. C1 [Cardoso-Martinez, Faviola; de la Rosa, Jose M.; Diaz-Marrero, Ana R.; Darias, Jose; Cueto, Mercedes] Inst Prod Nat & Agrobiol CSIC, Avda Astrofis F Sanchez 3, Tenerife 38206, Spain. [D'Croz, Luis] Univ Panama, Dept Biol Marina & Limnol, Panama City, Panama. [D'Croz, Luis] Smithsonian Trop Res Inst, Box 0843-03092, Balboa, Panama. [Dolores Jimenez-Anton, M.; Jesus Corral, M.; Garcia, Rocio; Alunda, Jose M.] Univ Complutense Madrid, Fac Vet, Dept Sanidad Anim, Grp UCM ICPVet 910993, E-28040 Madrid, Spain. [Dolores Jimenez-Anton, M.; Jesus Corral, M.; Garcia, Rocio; Alunda, Jose M.] Hosp 12 Octubre, Inst Invest, Avda Cordoba S-N, E-28041 Madrid, Spain. [Diaz-Marrero, Ana R.] Univ La Laguna, Univ Inst Bioorgan Chem Antonio Gonzalez IUBO CIB, Dept Organ Chem, E-38206 Tenerife, Spain. RP Cueto, M (reprint author), Inst Prod Nat & Agrobiol CSIC, Avda Astrofis F Sanchez 3, Tenerife 38206, Spain. EM mcueto@ipna.csic.es RI Diaz-Marrero, Ana/L-2899-2014 OI Diaz-Marrero, Ana/0000-0002-8886-7519 FU Ministerio de Ciencia e Innovacion [BIO2007-61745, SAF2009-0839]; Programa JAE-Pre (CSIC); IMBRAIN project [FP7-REGPOT-2012-CT2012-31637-IMBRAIN] FX This work was supported by the Ministerio de Ciencia e Innovacion (BIO2007-61745 and SAF2009-0839). F. C. acknowledges financial support from Programa JAE-Pre (CSIC). ARDM acknowledges funding from IMBRAIN project (FP7-REGPOT-2012-CT2012-31637-IMBRAIN). The STRI provided support and facilities. The Government of the Republic of Panama granted permission for the collection of the samples. COST Action CM1307 allowed the establishment of collaborative work. NR 26 TC 1 Z9 1 U1 1 U2 2 PU ROYAL SOC CHEMISTRY PI CAMBRIDGE PA THOMAS GRAHAM HOUSE, SCIENCE PARK, MILTON RD, CAMBRIDGE CB4 0WF, CAMBS, ENGLAND SN 2046-2069 J9 RSC ADV JI RSC Adv. PY 2016 VL 6 IS 45 BP 38579 EP 38591 DI 10.1039/c6ra04521a PG 13 WC Chemistry, Multidisciplinary SC Chemistry GA DK5PT UT WOS:000374972800011 ER PT J AU Haney, E AF Haney, Erin TI Daughters of Zanzibar SO TRANSITION LA English DT Article AB Sailors and Daughters: Early Photography and the Indian Ocean is an online exhibition commissioned by the Smithsonian's National Museum of African Art, as part of their project Connecting the Gems of the Indian Ocean: From Oman to East Africa, supported by a historic gift from the Sultan Qaboos Cultural Center in Washington, DC. The exhibition was curated by Erin Haney, with research assistance by Xavier Courouble, and site designed by Wilcox Design/Green Interactive. View the exhibition at http://indian-ocean.africa.si.edu/ C1 [Haney, Erin] Resolution, London, England. [Haney, Erin] Pioneering Photo Preservat Workshop 3PA, Porto Novo, Benin. [Haney, Erin] Univ Johannesburg, Fac Art Design & Architecture, Johannesburg, South Africa. [Haney, Erin] Smithsonian Inst, Washington, DC 20560 USA. RP Haney, E (reprint author), Resolution, London, England.; Haney, E (reprint author), Univ Johannesburg, Fac Art Design & Architecture, Johannesburg, South Africa.; Haney, E (reprint author), Smithsonian Inst, Washington, DC 20560 USA.; Haney, E (reprint author), George Washington Univ, Washington, DC 20052 USA.; Haney, E (reprint author), Univ Maryland, College Pk, MD 20742 USA. NR 0 TC 0 Z9 0 U1 0 U2 0 PU INDIANA UNIV PRESS PI BLOOMINGTON PA 601 N MORTON STREET, BLOOMINGTON, IN 47404-3797 USA SN 0041-1191 EI 1527-8042 J9 TRANSITION JI Transition PY 2016 IS 119 BP 37 EP 48 DI 10.2979/transition.119.1.06 PG 12 WC Ethnic Studies SC Ethnic Studies GA DK7GK UT WOS:000375093000006 ER PT J AU Miller, CC Jacob, DJ Abad, GG Chance, K AF Miller, Christopher Chan Jacob, Daniel J. Abad, Gonzalo Gonzalez Chance, Kelly TI Hotspot of glyoxal over the Pearl River delta seen from the OMI satellite instrument: implications for emissions of aromatic hydrocarbons SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID VOLATILE ORGANIC-COMPOUNDS; OZONE MONITORING INSTRUMENT; TROPOSPHERIC DEGRADATION; PRIDE-PRD2004 CAMPAIGN; CHEMICAL MECHANISM; SOUTHERN CHINA; HONG-KONG; INTEX-B; REGION; FORMALDEHYDE AB The Pearl River delta (PRD) is a densely populated hub of industrial activity located in southern China. OMI (Ozone Monitoring Instrument) satellite observations reveal a large hotspot of glyoxal (CHOCHO) over the PRD that is almost twice as large as any other in Asia. Formaldehyde (HCHO) and NO2 observed by OMI are also high in the PRD but no more than in other urban/industrial areas of China. The CHOCHO hotspot over the PRD can be explained by industrial paint and solvent emissions of aromatic volatile organic compounds (VOCs), with toluene being a dominant contributor. By contrast, HCHO in the PRD originates mostly from VOCs emitted by combustion (principally vehicles). By applying a plume transport model to wind-segregated OMI data, we show that the CHOCHO and HCHO enhancements over the PRD observed by OMI are consistent with current VOC emission inventories. Prior work using CHOCHO retrievals from the SCIAMACHY satellite instrument suggested that emission inventories for aromatic VOCs in the PRD were too low by a factor of 10-20; we attribute this result in part to bias in the SCIAMACHY data and in part to underestimated CHOCHO yields from oxidation of aromatics. Our work points to the importance of better understanding CHOCHO yields from the oxidation of aromatics in order to interpret space-based CHOCHO observations in polluted environments. C1 [Miller, Christopher Chan; Jacob, Daniel J.] Harvard Univ, Dept Earth & Planetary Sci, 20 Oxford St, Cambridge, MA 02138 USA. [Jacob, Daniel J.] Harvard Univ, Sch Engn & Appl Sci, Cambridge, MA 02138 USA. [Abad, Gonzalo Gonzalez; Chance, Kelly] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Miller, CC (reprint author), Harvard Univ, Dept Earth & Planetary Sci, 20 Oxford St, Cambridge, MA 02138 USA. EM cmiller@fas.harvard.edu OI Gonzalez Abad, Gonzalo/0000-0002-8090-6480 FU NASA Aura Science Team FX This work was supported by the NASA Aura Science Team. NR 54 TC 3 Z9 3 U1 13 U2 22 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 7 BP 4631 EP 4639 DI 10.5194/acp-16-4631-2016 PG 9 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DK1VM UT WOS:000374703000025 ER PT J AU Breedy, O Guzman, HM AF Breedy, Odalisca Guzman, Hector M. TI A revision of the genus Muricea Lamouroux, 1821 (Anthozoa, Octocorallia) in the eastern Pacific. Part II SO ZOOKEYS LA English DT Article DE Alcyonacea; Cnidaria; eastern Pacific; Muricea; plexaurid gorgonian; soft corals; taxonomy ID COELENTERATA; GORGONIIDAE; VERRILL AB The species of the genus Muricea were mainly described from 1846 to 1870. After that very few contributions were published. Although the highest richness of Muricea species is in the eastern Pacific shallow waters, a comprehensive systematic study of the genus does not exist. Recently we started a taxonomic review of the genus in order to validate the status of four species previously included in the genus Eumuricea. Herein we present the second part of the Muricea revision dealing with the species-group characterised by shelf-like calyces instead of tubular-like calyces (the M. squarrosa-group). Original type material was morphologically analysed and illustrated using optical and scanning electron microscopy. Comparative character tables are provided for the genus. The taxonomic status of the species was analysed and established by designating lectotypes, alternatively by recognising a holotype by monotypy. We conclude that the genus Muricea comprises 20 valid species, including the previous four in the M. squarrosa-group. We propose 10 lectotypes, a new combination and three more species groups for the genus based on morphology: the M. fruticosa-group, M. plantaginea-group and M. austera-group. C1 [Breedy, Odalisca] Univ Costa Rica, Escuela Biol, Ctr Invest Estruct Microscop, Ctr Invest Ciencias Mar & Limnol, POB 11501-2060, San Jose, Costa Rica. [Breedy, Odalisca; Guzman, Hector M.] Smithsonian Trop Res Inst, POB 0843-03092, Panama City, Panama. RP Breedy, O (reprint author), Univ Costa Rica, Escuela Biol, Ctr Invest Estruct Microscop, Ctr Invest Ciencias Mar & Limnol, POB 11501-2060, San Jose, Costa Rica.; Breedy, O (reprint author), Smithsonian Trop Res Inst, POB 0843-03092, Panama City, Panama. EM odaliscab@gmail.com FU Smithsonian Tropical Research Institute; Vicerrectoria de Investigacion, Universidad de Costa Rica [808-A9072, 808-B2142, 810-B5159] FX Our appreciation to Stephen Cairns, Leen van Ofwegen and Gary Williams for critical comments and suggestions that improved our manuscript, and Phil Alderslade for his advice solving taxonomic conflicts. We acknowledge the following people and institutions for their generosity in making available the specimens and information used in this study, YPM: Eric Lazo-Wasem and Lourdes Rojas; MCZ: Adam Baldinger; MNHN: Aude Andouche; MNHUK: Andrew Cabrinovic and Tracy Heath; NMNH: Stephen Cairns, Tim Coffer, Chad Walter and Geoff Keel; RMNH: Leen van Ofwegen; SMNH: Karin Sindemark Kronestedt; ZSM: Ole Tendal; Bernhard Ruthensteiner and Eva Lodde; ZMHC: Peter Stiewe and Helma Roggenbuck; CASIZ: Gary Williams; MZUF: Lisa Levi; MZUT: Cecilia Volpi; CASIZ: Gary Williams and Bob Vansyoc; CDRS: Cleve Hickmann; UNAM, Instituto de Ciencias del Mar y Limnologia: Jose Luis Carballo, Rosalinda Abeytia; Stanford University, Hopkins Marine Station, California: Geoffrey Shester; UPCH: Yuri Hooker; INN: Fernando Rivera and Priscilla Martinez; IMARPE: Miguel Romero; CRBMco: Katherine Mejia; UNIANDES-BIOMMAR: Juan Armando Sanchez. We thank the following people for providing photographs for this work: Aude Andouche (MNHN), Walter Larrimore (NMNH), Rosalinda Abeytia (UNAM), DeepSee submersible, Undersea Hunter group, Graham Edgar (University of Tasmania, Australia), Yuri Hooker (UPCH), Fernando Rivera (INN) and Elin Sigvaldadottir, (Department of Invertebrate Zoology, SMNH). We are grateful to Jorge Cortes (CIMAR) for advice and encouragement along this project; Alexander Rodriguez (UCR, CIEMIC) for the composition of the plates; Cristian Mora for laboratory assistance and light microscopic preparations; Ingo Wehrtmann (UCR) for helping with the German language translation; Rita Vargas (MZUCR), Eleazar Ruiz (CIMAR), Carlos Guevara (STRI), and Minor Lara and Maria Marta Chavarria (Area de Conservacion Guanacaste, Costa Rica), for helping in the fieldwork, and Marcelo Mainieri (Universidad de Ciencias Medicas, Costa Rica) for style suggestions. Thanks to the National Parks System of Protected Areas of Costa Rica, and the governments of Panama and Ecuador for allowing visits and collections in their National Parks and reserves. This project was partially sponsored by the Smithsonian Tropical Research Institute and the Vicerrectoria de Investigacion, Universidad de Costa Rica, projects 808-A9072, 808-B2142 and 810-B5159. NR 55 TC 1 Z9 1 U1 0 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 581 BP 1 EP 69 PG 69 WC Zoology SC Zoology GA DK0WJ UT WOS:000374632600001 ER PT J AU Slot, M Garcia, MN Winter, K AF Slot, Martijn Garcia, Milton N. Winter, Klaus TI Temperature response of CO2 exchange in three tropical tree species SO FUNCTIONAL PLANT BIOLOGY LA English DT Article DE carbon balance; gas exchange; global warming; photosynthetic temperature response; stomatal conductance; tropical forest ID RAIN-FOREST; LEAF RESPIRATION; CLIMATE-CHANGE; RUBISCO ACTIVASE; SHADE-TOLERANCE; FICUS-INSIPIDA; PHOTOSYNTHETIC RESPONSES; LIMITED PHOTOSYNTHESIS; EUCALYPTUS-PAUCIFLORA; NET PHOTOSYNTHESIS AB Tropical forests play a critical role in the global carbon cycle, but our limited understanding of the physiological sensitivity of tropical forest trees to environmental factors complicates predictions of tropical carbon fluxes in a changing climate. We determined the short-term temperature response of leaf photosynthesis and respiration of seedlings of three tropical tree species from Panama. For one of the species net CO2 exchange was also measured in situ. Dark respiration of all species increased linearly - not exponentially - over a similar to 30 degrees C temperature range. The early-successional species Ficus insipida Willd. and Ochroma pyramidale (Cav. ex Lam.) Urb. had higher temperature optima for photosynthesis (T-opt) and higher photosynthesis rates at T-opt than the late-successional species Calophyllum longifolium Willd. The decrease in photosynthesis above T-opt could be assigned, in part, to observed temperature-stimulated photorespiration and decreasing stomatal conductance (g(S)), with unmeasured processes such as respiration in the light, Rubisco deactivation, and changing membrane properties probably playing important additional roles, particularly at very high temperatures. As temperature increased above T-opt, g(S) of laboratory-measured leaves first decreased, followed by an increase at temperatures >40-45 degrees C. In contrast, g(S) of canopy leaves of F. insipida in the field continued to decrease with increasing temperature, causing complete suppression of photosynthesis at similar to 45 degrees C, whereas photosynthesis in the laboratory did not reach zero until leaf temperature was similar to 50 degrees C. Models parameterised with laboratory-derived data should be validated against field observations when they are used to predict tropical forest carbon fluxes. C1 [Slot, Martijn; Garcia, Milton N.; Winter, Klaus] Smithsonian Trop Res Inst, Apartado 0843-03092, Balboa, Panama. RP Slot, M (reprint author), Smithsonian Trop Res Inst, Apartado 0843-03092, Balboa, Panama. EM martijnslot78@gmail.com FU Smithsonian Tropical Research Institute FOREST-GEO postdoctoral research fellowship FX MS was supported by a Smithsonian Tropical Research Institute FOREST-GEO postdoctoral research fellowship. We thank Edwin Andrade for operating the canopy crane. Five anonymous reviewers provided valuable comments on an earlier version of this paper. NR 52 TC 5 Z9 5 U1 12 U2 18 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1445-4408 EI 1445-4416 J9 FUNCT PLANT BIOL JI Funct. Plant Biol. PY 2016 VL 43 IS 5 BP 468 EP 478 DI 10.1071/FP15320 PG 11 WC Plant Sciences SC Plant Sciences GA DJ4QD UT WOS:000374191100008 ER PT J AU Garrido, E AF Garrido, Elisa TI Art and science in the Spanish Baroque. Natural history, collectionism and visual culture SO ARCHIVO ESPANOL DE ARTE LA Spanish DT Book Review C1 [Garrido, Elisa] Smithsonian Inst, Washington, DC 20560 USA. RP Garrido, E (reprint author), Smithsonian Inst, Washington, DC 20560 USA. NR 1 TC 0 Z9 0 U1 1 U2 1 PU ARCHIVO ESPANOL DE ARTE PI MADRID PA DUQUE DE MEDINACELI 6, 28014 MADRID, SPAIN SN 0004-0428 EI 1988-8511 J9 ARCH ESPAN ART JI Arch. Esp. Arte PD JAN-MAR PY 2016 VL 89 IS 353 BP 97 EP 97 PG 1 WC Art SC Art GA DI5ZY UT WOS:000373580200009 ER PT J AU Cribbs, JD Cass, C Hazari, Z Sadler, PM Sonnert, G AF Cribbs, Jennifer D. Cass, Cheryl Hazari, Zahra Sadler, Philip M. Sonnert, Gerhard TI Mathematics Identity and Student Persistence in Engineering SO INTERNATIONAL JOURNAL OF ENGINEERING EDUCATION LA English DT Article DE mathematics identity; engineering; higher education; gender ID GENDER-DIFFERENCES; SELF-CONCEPT; HIGH-SCHOOL; SCIENCE; MATH; CHOICE; ACHIEVEMENT; SUCCESS; PERFORMANCE; EXPERIENCES AB Previous research suggests strong connections between students' mathematics background and their persistence in engineering career aspirations. This study expands on that research by examining how mathematics identity impacts the choice of engineering careers for male and female students. Data used in this study were drawn from the Factors Influencing College Success in Mathematics project, a nationally-representative survey garnering responses from 10,437 college calculus students. Results from an exploratory factor analysis validated the mathematics identity framework proposed. Additionally, results from a logistic regression indicate that mathematics interest and recognition in mathematics significantly predict the choice of an engineering career, even after controlling for SAT/ACT mathematics scores and demographic background, such as parental education. Moreover, the interaction between recognition in mathematics and gender is also significant and indicates that being recognized in mathematics has a stronger positive impact on the choice of an engineering career for females than for males. C1 [Cribbs, Jennifer D.] Western Kentucky Univ, Sch Teacher Educ, 1906 Coll Hts Blvd, Bowling Green, KY 42101 USA. [Cass, Cheryl] N Carolina State Univ, Dept Mat Sci & Engn, 911 Partners Way, Raleigh, NC 27606 USA. [Hazari, Zahra] Florida Int Univ, Dept Phys, Dept Teaching & Learning, 11200 SW 8th St, Miami, FL 33199 USA. [Hazari, Zahra] Florida Int Univ, STEM Transformat Inst, 11200 SW 8th St, Miami, FL 33199 USA. [Sadler, Philip M.] Harvard Univ, Dept Astron, Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Sonnert, Gerhard] Harvard Univ, Sci Educ Dept, Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Cribbs, JD (reprint author), Western Kentucky Univ, Sch Teacher Educ, 1906 Coll Hts Blvd, Bowling Green, KY 42101 USA.; Cass, C (reprint author), N Carolina State Univ, Dept Mat Sci & Engn, 911 Partners Way, Raleigh, NC 27606 USA.; Hazari, Z (reprint author), Florida Int Univ, Dept Phys, Dept Teaching & Learning, 11200 SW 8th St, Miami, FL 33199 USA.; Hazari, Z (reprint author), Florida Int Univ, STEM Transformat Inst, 11200 SW 8th St, Miami, FL 33199 USA.; Sadler, PM (reprint author), Harvard Univ, Dept Astron, Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA.; Sonnert, G (reprint author), Harvard Univ, Sci Educ Dept, Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM jennifer.cribbs@wku.edu; cheryl_cass@ncsu.edu; zhazari@fiu.edu; psadler@cfa.harvard.edu; gsonnert@cfa.harvard.edu FU National Science Foundation [0813702] FX This research is part of the Factors Influencing College Success in Mathematics (FICSMath) project funded by the National Science Foundation (0813702). Without the contributions and support of many people, the FICSMath project would not have been possible. We thank the members of the FICSMath team: John Almarode, Devasmita Chakraverty, Kate Dabney, Heather Hill, Jaimie Miller, Matthew Moynihan, Jon Star, Robert Tai, Terry Tivnan, Annette Trenga, Carol Wade, and Charity Watson. We would also like to thank several mathematics educators who provided advice or counsel on this project: Sadie Bragg, David Bressoud, James S. Dietz, Solomon Garfunkel, Daniel Goroff, Ed Joyce, James Lewis, Karen Marrongelle, William McCallum, Ricardo Nemirovsky, and Bob Speiser. Last but not least, we are grateful to the many college calculus professors and their students who gave up a portion of a class to provide data. Any opinions, findings, and conclusions in this article are the authors' and do not necessarily reflect the views of the National Science Foundation. NR 53 TC 0 Z9 0 U1 4 U2 5 PU TEMPUS PUBLICATIONS PI DURRUS, BANTRY PA IJEE , ROSSMORE,, DURRUS, BANTRY, COUNTY CORK 00000, IRELAND SN 0949-149X J9 INT J ENG EDUC JI Int. J. Eng. Educ PY 2016 VL 32 IS 1 BP 163 EP 171 PN A PG 9 WC Education, Scientific Disciplines; Engineering, Multidisciplinary SC Education & Educational Research; Engineering GA DJ5GG UT WOS:000374234200015 ER PT J AU Carrillo-Briceno, JD Argyriou, T Zapata, V Kindlimann, R Jaramillo, C AF Carrillo-Briceno, Jorge D. Argyriou, Thodoris Zapata, Vladimir Kindlimann, Rene Jaramillo, Carlos TI A NEW EARLY MIOCENE (AQUITANIAN) ELASMOBRANCHII ASSEMBLAGE FROM THE LA GUAJIRA PENINSULA, COLOMBIA SO AMEGHINIANA LA English DT Article DE Neogene; Tropical America; Caribbean; Sharks; Rays; Paleobathymetry; Paleoenvironments ID AMERICAN BIOTIC INTERCHANGE; SEA-LEVEL RISE; ALOPIAS-SUPERCILIOSUS; FISH ASSEMBLAGE; SHARK TEETH; NEOGENE; OLIGOCENE; PANAMA; FOSSIL; CHONDRICHTHYES AB Recent field expeditions have led to the discovery of a selachian assemblage from the earliest Miocene (Aquitanian) deposits of the Uitpa Formation in the La Guajira Peninsula, Colombia. This elasmobranch assemblage provides a unique glimpse into the Caribbean bio-diversity at the onset of the Neogene. The assemblage consists of 13 taxa, of which some are reported from Miocene deposits for the very first time. There are also new records of taxa the in southern Caribbean region. The taxonomic composition of the selachian assemblage was used to conduct a paleoenvironmental and paleobathymetric analysis of the lower Uitpa Formation. The maximum likelihood estimation of paleobathymetry suggests that the lower part of the Uitpa Formation was probably accumulated at a water depth of 100 to 200 m. This indicates a rapid increase in relative sea level or basin deepening, providing new insights into the possible causes of marine biota changes in the Cocinetas Basin during the Oligocene/Miocene transition. C1 [Carrillo-Briceno, Jorge D.; Argyriou, Thodoris; Kindlimann, Rene] Univ Zurich, Paleontol Inst & Museum, Karl Schmid Str 4, CH-8006 Zurich, Switzerland. [Zapata, Vladimir] Ecopetrol SA, Edificio Colgas, Bogota 11001000, Colombia. [Jaramillo, Carlos] Smithsonian Trop Res Inst, Ave Gorgas,Ed 235, Balboa 084303092, Ancon, Panama. RP Carrillo-Briceno, JD; Argyriou, T; Kindlimann, R (reprint author), Univ Zurich, Paleontol Inst & Museum, Karl Schmid Str 4, CH-8006 Zurich, Switzerland.; Zapata, V (reprint author), Ecopetrol SA, Edificio Colgas, Bogota 11001000, Colombia.; Jaramillo, C (reprint author), Smithsonian Trop Res Inst, Ave Gorgas,Ed 235, Balboa 084303092, Ancon, Panama. EM jorge.carrillo@pim.uzh.ch; thodoris.argyriou@pim.uzh.ch; vladimir.zapata@ecopetrol.com.co; mad_design@gmx.ch; jaramilloc@si.edu OI Carrillo Briceno, Jorge Domingo/0000-0002-8652-7692 FU SENACYT (National Secretary of Science and Technology of Panama) [PY-NI10-016A]; Swiss National Science Foundation [31003A-149605]; Smithsonian Institution; National Geographic Society; Anders Foundation; Universidad del Norte; National Science Foundation [EAR 0957679] FX This project has been supported by a SENACYT APY-NI10-016A grant (National Secretary of Science and Technology of Panama) and a Swiss National Science Foundation grant 31003A-149605 (to Marcelo Sanchez-Villagra). The Smithsonian Institution, the National Geographic Society, the Anders Foundation, Gregory D. and Jennifer Walston Johnson, Universidad del Norte and the National Science Foundation (Grant EAR 0957679) helped to support this work. Thanks to the Evolutionary Morphology and Palaeobiology group of the Palaeontological Institute and Museum at the University of Zurich, Switzerland, Carlos Jaramillo's lab members (STRI) participant of fieldwork in Alta Guajira (2013-2014), the Wayuu communities of the Alta Guajira and the Colombian National Police together with the Mapuka Museum of Universidad del Norte. Thanks to the Museum fur Naturkunde in Blin, the Museu Paraense Emilio Goeldi, the Natural History Museum of Basel, Paleontological collections of the Alcaldia Bolivariana de Urumaco, Palaeontological Institute and Museum at the University of Zurich and Universidad Nacional Experimental Francisco de Miranda for their valuable assistance and permission to revise fossil collections. Special thanks to J. Ceballos for his help with the microscopic photography and to L. Costeur, L. Londono, M. Gomez, and J. Escobar for their valuable assistance. We greatly appreciate comments and suggestions from A. Lopez Arbarello, C. Pimiento, A. Otero and R. Vullo. NR 161 TC 0 Z9 0 U1 1 U2 3 PU ASOCIACION PALEONTOLOGICA ARGENTINA PI BUENOS AIRES PA MAIPU 645, 1ER PISO, 1006 BUENOS AIRES, ARGENTINA SN 0002-7014 EI 1851-8044 J9 AMEGHINIANA JI Ameghiniana PY 2016 VL 53 IS 2 BP 77 EP 99 DI 10.5710/AMGH.26.10.2015.2931 PG 23 WC Paleontology SC Paleontology GA DI6HD UT WOS:000373598900001 ER PT J AU Davidson, I Scianni, C Hewitt, C Everett, R Holm, E Tamburri, M Ruiz, G AF Davidson, Ian Scianni, Christopher Hewitt, Chad Everett, Richard Holm, Eric Tamburri, Mario Ruiz, Gregory TI Mini-review: Assessing the drivers of ship biofouling management - aligning industry and biosecurity goals SO BIOFOULING LA English DT Review DE Ship biofouling; invasive species; vessel performance; biosecurity; hull surfaces; niche areas ID VESSEL SEA-CHESTS; MARINE BIOINVASIONS; INVASION HISTORY; NORTH-AMERICA; NEW-ZEALAND; ORGANISMS; COATINGS; BARNACLES; VECTOR; IMPACT AB Biofouling exerts a frictional and cost penalty on ships and is a direct cause of invasion by marine species. These negative consequences provide a unifying purpose for the maritime industry and biosecurity managers to prevent biofouling accumulation and transfer, but important gaps exist between these sectors. This mini-review examines the approach to assessments of ship biofouling among sectors (industry, biosecurity and marine science) and the implications for existing and emerging management of biofouling. The primary distinctions between industry and biosecurity in assessment of vessels biofouling revolve around the resolution of biological information collected and the specific wetted surface areas of primary concern to each sector. The morphological characteristics of biofouling and their effects on propulsion dynamics are of primary concern to industry, with an almost exclusive focus on the vertical sides and flat bottom of hulls and an emphasis on antifouling and operational performance. In contrast, the identity, biogeography, and ecology of translocated organisms is of highest concern to invasion researchers and biosecurity managers and policymakers, especially as it relates to species with known histories of invasion elsewhere. Current management practices often provide adequate, although not complete, provision for hull surfaces, but niche areas are well known to enhance biosecurity risk. As regulations to prevent invasions emerge in this arena, there is a growing opportunity for industry, biosecurity and academic stakeholders to collaborate and harmonize efforts to assess and manage biofouling of ships that should lead to more comprehensive biofouling solutions that promote industry goals while reducing biosecurity risk and greenhouse gas emissions. C1 [Davidson, Ian; Ruiz, Gregory] Smithsonian Environm Res Ctr, POB 28, Edgewater, MD 21037 USA. [Scianni, Christopher] Calif State Lands Commiss, Marine Invas Species Program, Sacramento, CA USA. [Hewitt, Chad] Univ Waikato, Sch Sci, Hamilton, New Zealand. [Everett, Richard] US Coast Guard, Environm Stand Div, Washington, DC USA. [Holm, Eric] Naval Surface Warfare Ctr, Carderock Div, West Bethesda, MD USA. [Tamburri, Mario] Univ Maryland, Chesapeake Biol Lab, Ctr Environm Sci, Solomons, MD 20688 USA. RP Davidson, I (reprint author), Smithsonian Environm Res Ctr, POB 28, Edgewater, MD 21037 USA. EM davidsoni@si.edu OI Ruiz, Gregory/0000-0003-2499-441X; Davidson, Ian/0000-0002-8729-6048 FU Maritime Environmental Resource Center (MERC); US Maritime Administration (MARAD); California State Lands Commission (SLC) FX The authors acknowledge funding support from the Maritime Environmental Resource Center (MERC), the US Maritime Administration (MARAD), and the California State Lands Commission (SLC). NR 96 TC 2 Z9 2 U1 12 U2 26 PU TAYLOR & FRANCIS LTD PI ABINGDON PA 4 PARK SQUARE, MILTON PARK, ABINGDON OX14 4RN, OXON, ENGLAND SN 0892-7014 EI 1029-2454 J9 BIOFOULING JI Biofouling PY 2016 VL 32 IS 4 BP 411 EP 428 DI 10.1080/08927014.2016.1149572 PG 18 WC Biotechnology & Applied Microbiology; Marine & Freshwater Biology SC Biotechnology & Applied Microbiology; Marine & Freshwater Biology GA DI2GH UT WOS:000373313200006 PM 26930397 ER PT J AU Kanzaki, N Giblin-Davis, RM Ye, WM Herre, EA Center, BJ AF Kanzaki, Natsumi Giblin-Davis, Robin M. Ye, Weimin Herre, Edward Allen Center, Barbara J. TI Recharacterisation of three Parasitodiplogaster species based on morphological and molecular profiles SO NEMATOLOGY LA English DT Article DE description; Ficus spp.; fig tree; genotyping; morphotyping; Panama; Parasitodiplogaster nymphanema; Parasitodiplogaster obtusinema; Parasitodiplogaster trigonema; taxonomy ID PHYLOGENETIC-RELATIONSHIPS; NEMATODA DIPLOGASTRINA; N. SP; DNA; APHELENCHOIDIDAE; REDESCRIPTION; AUSTRALIA; CITRINEMA; PARASITE; MORACEAE AB Three previously described Parasitodiplogaster spp., P. nymphanema, P. obtusinema and P. trigonema were re-isolated from their type locality, Barro Colorado Island Research Station, Smithsonian Tropical Research Institute, in Panama. The re-isolated materials were morphologically observed to compare with the original descriptions and molecularly characterised by DNA sequences of the near-full-length small subunit and D2-D3 expansion segments of the large subunit of the ribosomal RNA genes. Although the male tail characters, i.e., arrangement of genital papillae and spicule and gubernaculum morphologies, were close to the original descriptions, a compressed stoma with two (right subventral and dorsal) teeth was observed for the first time and confirmed in the newly re-isolated materials. The molecular phylogenetic analysis revealed that the three re-isolated species are close to P. laevigata, P. citrinema and P. popenema, forming the P. laevigata group in the genus, and this group was separated into three subgroups, P. citrinema + P. popenema (subgroup 1), P. nymphanema + P. obtusinema (subgroup 2) and P. laevigata + P. trigonema and three undescribed species (subgroup 3). The P. laevigata group is characterised by a relatively compressed stoma with two (right subventral and dorsal) teeth, arrangement of genital papillae (three or four precloacal and four postcloacal pairs), but distinguishable from each other by stomatal morphology, i.e., the shortest and most compressed being in subgroup 3, widest in subgroup 1, and intermediate in subgroup 2. Furthermore, a large and long spicule and gubernaculum were observed in subgroup 2 as its hypothesised apomorphy. C1 [Kanzaki, Natsumi; Giblin-Davis, Robin M.; Ye, Weimin; Center, Barbara J.] Univ Florida, IFAS, Ft Lauderdale Res & Educ Ctr, 3205 Coll Ave, Davie, FL 33314 USA. [Kanzaki, Natsumi] Forest Pathol Lab Forestry & Forest Prod Res Inst, 1 Matsunosato, Tsukuba, Ibaraki 3058687, Japan. [Herre, Edward Allen] Smithsonian Trop Res Inst, Balboa, Ancon, Panama. [Ye, Weimin] North Carolina Dept Agr & Consumer Serv, Div Agron, Nematode Assay Sect, 4300 Reedy Creek Rd, Raleigh, NC 27607 USA. RP Kanzaki, N (reprint author), Univ Florida, IFAS, Ft Lauderdale Res & Educ Ctr, 3205 Coll Ave, Davie, FL 33314 USA. EM nkanzaki@affrc.go.jp FU National Science Foundation (NSF) Biotic Surveys and Inventories projects [DEB-0450537, DEB-0640807]; USDA National Institute of Food and Agriculture [FLA-FTL-005296]; Japan Society for the Promotion of Science [21770094, 26292178] FX This work was supported in part by National Science Foundation (NSF) Biotic Surveys and Inventories projects (DEB-0450537; DEB-0640807), USDA National Institute of Food and Agriculture, Hatch project FLA-FTL-005296 and Grants-in-Aid for Scientific Research Nos 21770094 and 26292178 from the Japan Society for the Promotion of Science. Special thanks go to Dr Annette Aiello for processing specimens for the collections in Panama. NR 31 TC 2 Z9 2 U1 3 U2 4 PU BRILL ACADEMIC PUBLISHERS PI LEIDEN PA PLANTIJNSTRAAT 2, P O BOX 9000, 2300 PA LEIDEN, NETHERLANDS SN 1388-5545 J9 NEMATOLOGY JI Nematology PY 2016 VL 18 BP 417 EP 437 DI 10.1163/15685411-00002967 PN 4 PG 21 WC Zoology SC Zoology GA DI7XO UT WOS:000373715500003 ER PT J AU Geddes, JA Heald, CL Silva, SJ Martin, RV AF Geddes, Jeffrey A. Heald, Colette L. Silva, Sam J. Martin, Randall V. TI Land cover change impacts on atmospheric chemistry: simulating projected large-scale tree mortality in the United States SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID VOLATILE ORGANIC-COMPOUNDS; BARK BEETLE INFESTATION; OZONE DRY DEPOSITION; AIR-QUALITY; CLIMATE-CHANGE; TROPOSPHERIC CHEMISTRY; MONOTERPENE EMISSIONS; FOREST ECOSYSTEMS; BOREAL FORESTS; AEROSOL AB Land use and land cover changes impact climate and air quality by altering the exchange of trace gases between the Earth's surface and atmosphere. Large-scale tree mortality that is projected to occur across the United States as a result of insect and disease may therefore have unexplored consequences for tropospheric chemistry. We develop a land use module for the GEOS-Chem global chemical transport model to facilitate simulations involving changes to the land surface, and to improve consistency across land-atmosphere exchange processes. The model is used to test the impact of projected national-scale tree mortality risk through 2027 estimated by the 2012 USDA Forest Service National Insect and Disease Risk Assessment. Changes in biogenic emissions alone decrease monthly mean O-3 by up to 0.4 ppb, but reductions in deposition velocity compensate or exceed the effects of emissions yielding a net increase in O-3 of more than 1 ppb in some areas. The O-3 response to the projected change in emissions is affected by the ratio of baseline NOx : VOC concentrations, suggesting that in addition to the degree of land cover change, tree mortality impacts depend on whether a region is NOx-limited or NOx-saturated. Consequently, air quality (as diagnosed by the number of days that 8 h average O-3 exceeds 70 ppb) improves in polluted environments where changes in emissions are more important than changes to dry deposition, but worsens in clean environments where changes to dry deposition are the more important term. The influence of changes in dry deposition demonstrated here underscores the need to evaluate treatments of this physical process in models. Biogenic secondary organic aerosol loadings are significantly affected across the US, decreasing by 5-10% across many regions, and by more than 25% locally. Tree mortality could therefore impact background aerosol loadings by between 0.5 and 2 mu g m(-3). Changes to reactive nitrogen oxide abundance and partitioning are also locally important. The regional effects simulated here are similar in magnitude to other scenarios that consider future biofuel cropping or natural succession, further demonstrating that biosphere-atmosphere exchange should be considered when predicting future air quality and climate. We point to important uncertainties and further development that should be addressed for a more robust understanding of land cover change feedbacks. C1 [Geddes, Jeffrey A.; Martin, Randall V.] Dalhousie Univ, Dept Phys & Atmospher Sci, POB 15000, Halifax, NS B3H 4R2, Canada. [Heald, Colette L.; Silva, Sam J.] MIT, Dept Civil & Environm Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Martin, Randall V.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Geddes, JA (reprint author), Dalhousie Univ, Dept Phys & Atmospher Sci, POB 15000, Halifax, NS B3H 4R2, Canada. EM jeff.geddes@dal.ca RI Martin, Randall/C-1205-2014; Chem, GEOS/C-5595-2014 OI Martin, Randall/0000-0003-2632-8402; FU NSERC; NSF [AGC-1238109]; NSERC CREATE IACPES FX This work was supported by NSERC and NSF (AGC-1238109). JAG was partially supported by a NSERC CREATE IACPES postdoctoral fellowship and travel grant. NR 95 TC 3 Z9 3 U1 3 U2 8 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 4 BP 2323 EP 2340 DI 10.5194/acp-16-2323-2016 PG 18 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DH7KC UT WOS:000372971500030 ER PT J AU Li, C Martin, RV Boys, BL van Donkelaar, A Ruzzante, S AF Li, Chi Martin, Randall V. Boys, Brian L. van Donkelaar, Aaron Ruzzante, Sacha TI Evaluation and application of multi-decadal visibility data for trend analysis of atmospheric haze SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID AEROSOL OPTICAL DEPTH; SULFUR-DIOXIDE EMISSIONS; FINE PARTICULATE MATTER; EASTERN-UNITED-STATES; CLIMATE DATA SERIES; MAXIMAL T-TEST; SOLAR-RADIATION; AIR-POLLUTION; EXPOSURE ASSESSMENT; NITROGEN-OXIDES AB There are few multi-decadal observations of atmospheric aerosols worldwide. This study applies global hourly visibility (Vis) observations at more than 3000 stations to investigate historical trends in atmospheric haze over 1945-1996 for the US, and over 1973-2013 for Europe and eastern Asia. A comprehensive data screening and processing framework is developed and applied to minimize uncertainties and construct monthly statistics of inverse visibility (1/Vis). This data processing includes removal of relatively clean cases with high uncertainty, and change point detection to identify and separate methodological discontinuities such as the introduction of instrumentation. Although the relation between 1/Vis and atmospheric extinction coefficient (b(ext)) varies across different stations, spatially coherent trends of the screened 1/Vis data exhibit consistency with the temporal evolution of collocated aerosol measurements, including the b(ext) trend of -2.4% yr(-1) (95% CI: -3.7, -1.1% yr(-1)) vs. 1/Vis trend of -1.6% yr(-1) (95% CI: -2.4, -0.8% yr(-1)) over the US for 1989-1996, and the fine aerosol mass (PM2.5) trend of -5.8% yr(-1) (95% CI: -7.8, 4.2% yr(-1)) vs. 1/Vis trend of -3.4% yr(-1) (95% CI: -4.4, 2.4% yr(-1)) over Europe for 2006-2013. Regional 1/Vis and Emissions Database for Global Atmospheric Research (EDGAR) sulfur dioxide (SO2) emissions are significantly correlated over the eastern US for 1970-1995 (r = 0.73), over Europe for 1973-2008 (r similar to 0.9) and over China for 1973-2008 (r similar to 0.9). Consistent "reversal points" from increasing to decreasing in SO2 emission data are also captured by the regional 1/Vis time series (e.g., late 1970s for the eastern US, early 1980s for western Europe, late 1980s for eastern Europe, and mid 2000s for China). The consistency of 1/Vis trends with other in situ measurements and emission data demonstrates promise in applying these quality assured 1/Vis data for historical air quality studies. C1 [Li, Chi; Martin, Randall V.; Boys, Brian L.; van Donkelaar, Aaron; Ruzzante, Sacha] Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. [Martin, Randall V.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Ruzzante, Sacha] Queens Univ, Dept Phys Engn Phys & Astron, Kingston, ON, Canada. RP Li, C (reprint author), Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. EM chi.li@dal.ca RI Martin, Randall/C-1205-2014 OI Martin, Randall/0000-0003-2632-8402 FU Natural Science and Engineering Research Council of Canada; Killam Predoctoral Scholarship; ACEnet Research Fellowship; US Environmental Protection Agency; National Park Service FX This work is supported by the Natural Science and Engineering Research Council of Canada. C. Li is partially supported by a Killam Predoctoral Scholarship, and an ACEnet Research Fellowship. We thank two anonymous reviewers for their helpful comments. Special thanks to Jing Li at NASA GISS for instructions and discussion about trend calculation, Xiaolan Wang and Yang Feng at Climate Research Division, Environment Canada for maintaining the RHtest software, and Zifeng Lu at Argonne National Laboratory for guidance in SO2 emission data. This work primarily relies on the visibility data provided by NOAA NCEI. The bext data are from the IMPROVE network. IMPROVE is a collaborative association of state, tribal, and federal agencies, and international partners. US Environmental Protection Agency is the primary funding source, with contracting and research support from the National Park Service. The Air Quality Group at the University of California, Davis is the central analytical laboratory, with ion analysis provided by Research Triangle Institute, and carbon analysis provided by Desert Research Institute. We acknowledge the EMEP measurement networks and the data managers for maintaining the PM2.5 data for validating 1/Vis trends over Europe. We also thank NASA SEDAC and EDGAR for making the emission data used in this study publicly available. NR 100 TC 2 Z9 2 U1 11 U2 23 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 4 BP 2435 EP 2457 DI 10.5194/acp-16-2435-2016 PG 23 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DH7KC UT WOS:000372971500036 ER PT J AU Hammer, MS Martin, RV van Donkelaar, A Buchard, V Torres, O Ridley, DA Spurr, RJD AF Hammer, Melanie S. Martin, Randall V. van Donkelaar, Aaron Buchard, Virginie Torres, Omar Ridley, David A. Spurr, Robert J. D. TI Interpreting the ultraviolet aerosol index observed with the OMI satellite instrument to understand absorption by organic aerosols: implications for atmospheric oxidation and direct radiative effects SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID COMPLEX REFRACTIVE-INDEXES; SINGLE SCATTERING ALBEDO; BROWN CARBON AEROSOL; LIGHT-ABSORPTION; BLACK CARBON; SPECTRAL DEPENDENCE; ANGSTROM EXPONENT; TROPOSPHERIC CHEMISTRY; GLOBAL DISTRIBUTION; PARTICULATE MATTER AB Satellite observations of the ultraviolet aerosol index (UVAI) are sensitive to absorption of solar radiation by aerosols; this absorption affects photolysis frequencies and radiative forcing. We develop a global simulation of the UVAI using the 3-D chemical transport model GEOS-Chem coupled with the Vector Linearized Discrete Ordinate Radiative Transfer model (VLIDORT). The simulation is applied to interpret UVAI observations from the Ozone Monitoring Instrument (OMI) for the year 2007. Simulated and observed values are highly consistent in regions where mineral dust dominates the UVAI, but a large negative bias (0-.32 to -0.97) exists between simulated and observed values in biomass burning regions. We determine effective optical properties for absorbing organic aerosol, known as brown carbon (BrC), and implement them into GEOS-Chem to better represent observed UVAI values over biomass burning regions. The inclusion of absorbing BrC decreases the mean bias between simulated and OMI UVAI values from -0.57 to -0.09 over West Africa in January, from -0.32 to +0.0002 over South Asia in April, from -0.97 to -0.22 over southern Africa in July, and from -0.50 to +0.33 over South America in September. The spectral dependence of absorption after including BrC in the model is broadly consistent with reported observations for biomass burning aerosol, with absorbing ngstrm exponent (AAE) values ranging from 2.9 in the ultraviolet (UV) to 1.3 across the UV-Near IR spectrum. We assess the effect of the additional UV absorption by BrC on atmospheric photochemistry by examining tropospheric hydroxyl radical (OH) concentrations in GEOS-Chem. The inclusion of BrC decreases OH by up to 30% over South America in September, up to 20% over southern Africa in July, and up to 15% over other biomass burning regions. Global annual mean OH concentrations in GEOS-Chem decrease due to the presence of absorbing BrC, increasing the methyl chloroform lifetime from 5.62 to 5.68 years, thus reducing the bias against observed values. We calculate the direct radiative effect (DRE) of BrC using GEOS-Chem coupled with the radiative transfer model RRTMG (GC-RT). Treating organic aerosol as containing more strongly absorbing BrC changes the global annual mean all-sky top of atmosphere (TOA) DRE by +0.03 Wm(-2) and all-sky surface DRE by -0.08 Wm(-2). Regional changes of up to +0.3 Wm(-2) at TOA and down to -1.5 W m(-2) at the surface are found over major biomass burning regions. C1 [Hammer, Melanie S.; Martin, Randall V.; van Donkelaar, Aaron] Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. [Martin, Randall V.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Buchard, Virginie; Torres, Omar] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA. [Buchard, Virginie] Univ Space Res Assoc, GESTAR, Columbia, MD USA. [Ridley, David A.] MIT, Dept Civil & Environm Engn, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Spurr, Robert J. D.] RT Solut Inc, 9 Channing St, Cambridge, MA USA. RP Hammer, MS (reprint author), Dalhousie Univ, Dept Phys & Atmospher Sci, Halifax, NS, Canada. EM melanie.hammer@dal.ca RI Martin, Randall/C-1205-2014; Chem, GEOS/C-5595-2014 OI Martin, Randall/0000-0003-2632-8402; FU Natural Science and Engineering Research Council of Canada FX This work was supported by the Natural Science and Engineering Research Council of Canada. Computational facilities were provided in part by the Atlantic Computational Excellence Network consortium of Compute Canada. We thank Farhan Khan for assistance during the early stages of this work. NR 87 TC 4 Z9 4 U1 3 U2 10 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 4 BP 2507 EP 2523 DI 10.5194/acp-16-2507-2016 PG 17 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DH7KC UT WOS:000372971500040 ER PT J AU Kinsey, JD Kieber, DJ Neale, PJ AF Kinsey, Joanna D. Kieber, David J. Neale, Patrick J. TI Effects of iron limitation and UV radiation on Phaeocystis antarctica growth and dimethylsulfoniopropionate, dimethylsulfoxide and acrylate concentrations SO ENVIRONMENTAL CHEMISTRY LA English DT Article; Proceedings Paper CT 6th International Symposium on Biological and Environmental Chemistry of DMS(P) and Related Compounds CY MAY 26-30, 2014 CL Inst Ciencies Mar, Barcelona, SPAIN SP Spanish Minist Sci & Innovat, CSIC, SCOR HO Inst Ciencies Mar DE acrylic acid; algae; antioxidant; carbon overflow; DMSP; DMSO; DMS; reactive oxygen species; ROS; Ross Sea; Southern Ocean; ultraviolet radiation ID FRAGILARIOPSIS-CYLINDRUS BACILLARIOPHYCEAE; MARINE-PHYTOPLANKTON; SOUTHERN-OCEAN; ROSS SEA; ULTRAVIOLET-RADIATION; PHYSIOLOGICAL-ASPECTS; PRIMARY PRODUCTIVITY; WEIGHTING FUNCTIONS; EMILIANIA-HUXLEYI; NITRATE REDUCTASE AB Environmental context Low iron concentrations and solar ultraviolet radiation can affect the growth of marine algae. We observed reduced growth and substantial increases in dissolved dimethylsulfoxide and cellular acrylate concentrations in low-iron cultures of a prevalent Southern Ocean algal species, Phaeocystis antarctica, with comparatively small increases observed for cellular dimethylsulfoniopropionate concentrations. Exposure of P. antarctica to high levels of ultraviolet and visible light had very little effect on concentrations of these compounds in culture, even under iron-limitation. Our results highlight the importance of iron to P. antarctica. Abstract Iron is a key nutrient regulating primary production in the Southern Ocean. We investigated the effect of iron limitation with and without exposure to ultraviolet radiation (UVR, 290-400nm) on concentrations of dimethylsulfoniopropionate (DMSP), dimethylsulfoxide (DMSO) and acrylate in axenic batch cultures of Phaeocystis antarctica, a dominant algal species in Antarctic waters. Cellular concentrations of DMSP and acrylate, and cell-number normalised dissolved DMSO concentrations were 1.4-, 11.5- and 6.9-fold higher in iron-limited cultures compared to iron-replete cultures, which we propose resulted from (1) increased reactions of DMSP and dimethylsulfide (DMS) with reactive oxygen species to produce DMSO and (2) increased DMSP cleavage under iron limitation to produce acrylate. Short-term exposure (4h) of iron-limited and iron-replete cultures to a range of photosynthetically active radiation (PAR) and UVR+PAR irradiances did not appreciably affect P. antarctica biomass or total DMSP, DMSO or acrylate concentrations, except at high UVR intensities, suggesting that iron limitation was the primary driver regulating growth and changes in concentrations of these compounds in P. antarctica. High millimolar cellular DMSP and acrylate concentrations under both iron-replete and iron-limited conditions indicated that these two compounds served as de facto antioxidants allowing P. antarctica to thrive under high UVR exposure and low iron concentrations. High dissolved acrylate concentrations indicate significant carbon removal possibly as part of an overflow mechanism during unbalanced growth. C1 [Kinsey, Joanna D.; Kieber, David J.] SUNY Coll Environm Sci & Forestry, Dept Chem, 1 Forestry Dr, Syracuse, NY 13210 USA. [Neale, Patrick J.] Smithsonian Environm Res Ctr, 647 Contees Wharf Rd, Edgewater, MD 21037 USA. RP Kieber, DJ (reprint author), SUNY Coll Environm Sci & Forestry, Dept Chem, 1 Forestry Dr, Syracuse, NY 13210 USA. EM djkieber@esf.edu NR 78 TC 2 Z9 2 U1 8 U2 17 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1448-2517 EI 1449-8979 J9 ENVIRON CHEM JI Environ. Chem. PY 2016 VL 13 IS 2 BP 195 EP 211 DI 10.1071/EN14275 PG 17 WC Chemistry, Analytical; Environmental Sciences SC Chemistry; Environmental Sciences & Ecology GA DH8SU UT WOS:000373067500003 ER PT J AU Buffington, ML Forshage, M AF Buffington, Matthew L. Forshage, Mattias TI REDESCRIPTION OF GANASPIS BRASILIENSIS (IHERING, 1905), NEW COMBINATION, (HYMENOPTERA: FIGITIDAE) A NATURAL ENEMY OF THE INVASIVE DROSOPHILA SUZUKII (MATSUMURA, 1931) (DIPTERA: DROSOPHILIDAE) SO PROCEEDINGS OF THE ENTOMOLOGICAL SOCIETY OF WASHINGTON LA English DT Article DE Spotted wing Drosophila; Panama; South Korea; soft fruit; pest fly; biological control ID CYNIPOIDEA; REVISION; GENUS AB The new combination of Ganaspis brasiliensis (Ihering, 1905) is proposed, and the species is redescribed from historical specimens taken in the Neotropical Region as well as more recent specimens reared from Drosophila suzukii Matsumura, 1931 in South Korea. Drosophila suzukii, otherwise known as the spotted-wing Drosophila, is a major pest of soft fruits the world over, and the search for effective natural enemies of this fly are ongoing. Though not parasitoids of D. suzukii, we also propose the following new combinations: Dieucoila brasiliensis (Kieffer, 1909), new combination, and Dieucoila brasiliana (Weld, 1952), new combination. After summarizing all known species of Eucoilinae with the specific epithet 'brasiliensis', we encourage future researchers to avoid this name in order prevent nomenclatural confusion. C1 [Buffington, Matthew L.] Smithsonian Inst, Natl Museum Nat Hist, USDA, Systemat Entomol Lab, 10th & Constitut Ave NW, Washington, DC 20013 USA. [Forshage, Mattias] Nat Hist Riksmuseet, Dept Entomol, Box 50007, SE-10405 Stockholm, Sweden. RP Buffington, ML (reprint author), Smithsonian Inst, Natl Museum Nat Hist, USDA, Systemat Entomol Lab, 10th & Constitut Ave NW, Washington, DC 20013 USA.; Forshage, M (reprint author), Nat Hist Riksmuseet, Dept Entomol, Box 50007, SE-10405 Stockholm, Sweden. EM matt.buffington@ars.usda.gov; Mattias.Forshage@nrm.se FU USDA Systematic Entomology Laboratory FX We gratefully thank Antonio Bionidi and Kent Daane (UC Berkeley) for sending reared specimens for our examination; Claire Villemant and Agniele Touret-Alby (Museum national d'Histoire naturelle, Paris) for loaned us specimens critical to this work; Yves Carton supplied personal information regarding the fieldwork in Guadeloupe. Goran Nordlander (Swedish University of Agricultural Science) provided valuable comments to earlier drafts of this paper. USDA Systematic Entomology Laboratory funded MLB. Mention of trade names or commercial products in this publication is solely for the purpose of providing specific information and does not imply recommendation or endorsement by the USDA. USDA is an equal opportunity provider and employer. NR 20 TC 1 Z9 1 U1 9 U2 12 PU ENTOMOL SOC WASHINGTON PI WASHINGTON PA SMITHSONIAN INSTITUTION DEPT ENTOMOLOGY, WASHINGTON, DC 20560 USA SN 0013-8797 J9 P ENTOMOL SOC WASH JI Proc. Entomol. Soc. Wash. PD JAN PY 2016 VL 118 IS 1 BP 1 EP 13 DI 10.4289/0013-8797.118.1.1 PG 13 WC Entomology SC Entomology GA DI1FU UT WOS:000373242800001 ER PT J AU Buffington, ML Melika, G Davis, M Elkinton, JS AF Buffington, Matthew L. Melika, George Davis, Monica Elkinton, Joseph S. TI THE DESCRIPTION OF ZAPATELLA DAVISAE, NEW SPECIES, (HYMENOPTERA: CYNIPIDAE) A PEST GALL WASP OF BLACK OAK (QUERCUS VELUTINA) IN NEW ENGLAND, USA SO PROCEEDINGS OF THE ENTOMOLOGICAL SOCIETY OF WASHINGTON LA English DT Article DE Cape Cod; Long Island; Martha's Vineyard; oak pest ID PLAGIOTROCHUS-SUBERI HYMENOPTERA; PUJADE-VILLAR; N. AB Many species of gall wasp (Cynipidae) essentially co-exist with their host oak tree species. Occasionally, the association becomes destructive to the tree, as is the case with Zapatella davisae, new species. This species is a twig galler, and as such, in the cases of heavy infestation, cause flagging, leaf clumping, and dieback of branches and twigs. Historical records of other species of Zapatella suggest that members of this genus have a checkered record with respect to damaging their host plants in North America, and these data are summarized here. C1 [Buffington, Matthew L.] Smithsonian Inst, Systemat Entomol Lab, USDA ARS, Natl Museum Nat Hist, 10th & Constitut Ave NW, Washington, DC 20560 USA. [Melika, George] Directorate Plant Protect Soil Conservat & Agrien, Plant Hlth & Mol Biol Lab, Natl Food Chain Safety Off, Budaorsi Str 141-145, H-1118 Budapest, Hungary. [Davis, Monica; Elkinton, Joseph S.] Univ Massachusetts, Dept Environm Conservat, Amherst, MA 01003 USA. RP Melika, G (reprint author), Directorate Plant Protect Soil Conservat & Agrien, Plant Hlth & Mol Biol Lab, Natl Food Chain Safety Off, Budaorsi Str 141-145, H-1118 Budapest, Hungary. EM melikageorge@gmail.com FU Arborjet Inc.; Systematic Entomology Laboratory, ARS-USDA FX GM would like to thank Russell Norton (Cape Cod Cooperative Extension) for sending specimens. MD acknowledges Dan Gilrien for field collections from Long Island sites, and Arborjet Inc. for funding support. MLB was supported by the Systematic Entomology Laboratory, ARS-USDA, and wishes to thank Paul Goldstein (Systematic Entomology Laboratory) for fruitful discussions on this topic. Mention of trade names or commercial products in this publication is solely for the purpose of providing specific information and does not imply recommendation or endorsement by the USDA. USDA is an equal opportunity provider and employer. NR 26 TC 0 Z9 0 U1 2 U2 2 PU ENTOMOL SOC WASHINGTON PI WASHINGTON PA SMITHSONIAN INSTITUTION DEPT ENTOMOLOGY, WASHINGTON, DC 20560 USA SN 0013-8797 J9 P ENTOMOL SOC WASH JI Proc. Entomol. Soc. Wash. PD JAN PY 2016 VL 118 IS 1 BP 14 EP 26 DI 10.4289/0013-8797.118.1.14 PG 13 WC Entomology SC Entomology GA DI1FU UT WOS:000373242800002 ER PT J AU Gagne, RJ AF Gagne, Raymond J. TI ANTHODIPLOSIS EUTROCHII, N. SP (DIPTERA: CECIDOMYIIDAE), THE FLOWER-BUD GALLMAKER OF JOE PYE WEED IN NORTH AMERICA SO PROCEEDINGS OF THE ENTOMOLOGICAL SOCIETY OF WASHINGTON LA English DT Article DE gall midges; Eutrochium; Nearctic; description; life history AB Anthodiplosis eutrochii Gagne, new species (Diptera: Cecidomyiidae: Clinodiplosini), is described. It is responsible for the flower bud gall and only known gall on Eutrochium spp. in eastern North America. Dasineura purpurea Felt is no longer considered the gall maker. Galls are first noticeable at early anthesis in July. Full-grown larvae drop to the soil in August and September. Some adults may emerge in September, but most appear the following year. Anthodiplosis Kieffer, previously known from a single species from Europe, is a genus new to North America. C1 [Gagne, Raymond J.] Smithsonian Inst, Natl Museum Nat Hist, Systemat Entomol Lab, PSI,Agr Res Serv,US Dept Agr, MRC-168,POB 37012, Washington, DC 20013 USA. RP Gagne, RJ (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Systemat Entomol Lab, PSI,Agr Res Serv,US Dept Agr, MRC-168,POB 37012, Washington, DC 20013 USA. EM raymond.gagne@ars.usda.gov NR 20 TC 0 Z9 0 U1 0 U2 0 PU ENTOMOL SOC WASHINGTON PI WASHINGTON PA SMITHSONIAN INSTITUTION DEPT ENTOMOLOGY, WASHINGTON, DC 20560 USA SN 0013-8797 J9 P ENTOMOL SOC WASH JI Proc. Entomol. Soc. Wash. PD JAN PY 2016 VL 118 IS 1 BP 27 EP 36 DI 10.4289/0013-8797.118.1.27 PG 10 WC Entomology SC Entomology GA DI1FU UT WOS:000373242800003 ER PT J AU Kula, RR Harms, NE AF Kula, Robert R. Harms, Nathan E. TI A NEW SPECIES OF CHAENUSA HALIDAY SENSU LATO (HYMENOPTERA: BRACONIDAE) FROM THE NEARCTIC REGION SO PROCEEDINGS OF THE ENTOMOLOGICAL SOCIETY OF WASHINGTON LA English DT Article DE Alysiinae; biological control; Dacnusini; Hydrellia; parasitoid; Sagittaria latifolia; taxonomy ID DISTRIBUTION RECORDS; ALYSIINAE; REVISION; HYDROCHARITACEAE; DIPTERA AB Chaenusa psillosae Kula, new species from the Nearctic Region is described. Specimens upon which the new species is described were reared from an undetermined species of Hydrellia Robineau-Desvoidy infesting Sagittaria latifolia Willd. A key to the New World species of Chaenusa sensu lato is amended to include the new species. C1 [Kula, Robert R.] Smithsonian Inst, Systemat Entomol Lab, Beltsville Agr Res Ctr, Agr Res Serv,US Dept Agr,Natl Museum Nat Hist, POB 37012,MRC-168, Washington, DC 20013 USA. [Harms, Nathan E.] US Army, Engn Res & Dev Ctr, Vicksburg, MS 39180 USA. RP Kula, RR (reprint author), Smithsonian Inst, Systemat Entomol Lab, Beltsville Agr Res Ctr, Agr Res Serv,US Dept Agr,Natl Museum Nat Hist, POB 37012,MRC-168, Washington, DC 20013 USA.; Harms, NE (reprint author), US Army, Engn Res & Dev Ctr, Vicksburg, MS 39180 USA. EM Robert.Kula@ars.usda.gov; Nathan.e.harms@usace.army.mil NR 15 TC 0 Z9 0 U1 0 U2 0 PU ENTOMOL SOC WASHINGTON PI WASHINGTON PA SMITHSONIAN INSTITUTION DEPT ENTOMOLOGY, WASHINGTON, DC 20560 USA SN 0013-8797 J9 P ENTOMOL SOC WASH JI Proc. Entomol. Soc. Wash. PD JAN PY 2016 VL 118 IS 1 BP 101 EP 108 DI 10.4289/0013-8797.118.1.101 PG 8 WC Entomology SC Entomology GA DI1FU UT WOS:000373242800006 ER PT J AU Henry, TJ Gill, BD AF Henry, Thomas J. Gill, Bruce D. TI LEONARD A. KELTON, 1923-2011: BIOGRAPHICAL SKETCH, LIST OF PUBLICATIONS, DESCRIBED TAXA, AND PATRONYMS NAMED IN HIS HONOR OBITUARY SO PROCEEDINGS OF THE ENTOMOLOGICAL SOCIETY OF WASHINGTON LA English DT Biographical-Item C1 [Henry, Thomas J.] ARS, Systemat Entomol Lab, USDA, Natl Museum Nat Hist,Smithsonian Inst, Washington, DC 20013 USA. RP Henry, TJ (reprint author), ARS, Systemat Entomol Lab, USDA, Natl Museum Nat Hist,Smithsonian Inst, Washington, DC 20013 USA. EM thomas.henry@ars.usda.gov; scarab57@xplornet.com NR 1 TC 0 Z9 0 U1 0 U2 0 PU ENTOMOL SOC WASHINGTON PI WASHINGTON PA SMITHSONIAN INSTITUTION DEPT ENTOMOLOGY, WASHINGTON, DC 20560 USA SN 0013-8797 J9 P ENTOMOL SOC WASH JI Proc. Entomol. Soc. Wash. PD JAN PY 2016 VL 118 IS 1 BP 131 EP 139 PG 9 WC Entomology SC Entomology GA DI1FU UT WOS:000373242800009 ER PT J AU Takeda, A Yoshimura, K Saar, SH AF Takeda, Aki Yoshimura, Keiji Saar, Steven H. TI The Hinode/XRT Full-Sun Image Corrections and the Improved Synoptic Composite Image Archive SO SOLAR PHYSICS LA English DT Article DE Corona; Data calibration; Instrumental effects; Instrumentation and data management ID X-RAY TELESCOPE; SOLAR-A MISSION AB The XRT Synoptic Composite Image Archive (SCIA) is a storage and gallery of X-ray full-Sun images obtained through the synoptic program of the X-Ray Telescope (XRT) onboard the Hinode satellite. The archived images provide a quick history of solar activity through the daily and monthly layout pages and long-term data for morphological and quantitative studies of the X-ray corona. This article serves as an introduction to the SCIA, i.e., to the structure of the archive and specification of the data products included therein. We also describe a number of techniques used to improve the quality of the archived images: preparation of composite images to increase intensity dynamic range, removal of dark spots that are due to contaminants on the CCD, and correction of the visible stray light contamination that has been detected on the Ti-poly and C-poly filter images since May 2012. C1 [Takeda, Aki; Yoshimura, Keiji] Montana State Univ, POB 173840, Bozeman, MT 59717 USA. [Saar, Steven H.] Smithsonian Astrophys Observ, 60 Garden St, Cambridge, MA 02138 USA. RP Takeda, A (reprint author), Montana State Univ, POB 173840, Bozeman, MT 59717 USA. EM takeda@solar.physics.montana.edu FU NASA [NNM07AB07C] FX Hinode is a Japanese mission developed and launched by ISAS/JAXA, with NAOJ as domestic partner and NASA and STFC (UK) as international partners. It is operated by these agencies in co-operation with ESA and the NSC (Norway). This work was supported by NASA grant NNM07AB07C for Hinode XRT science. We thank David McKenzie for providing the dust size measurements. We also thank Patrick MacCauley, Adam Kobelski, and Nicole Schanche for their help in characterizing the effects of the light leak, and we thank Antonia Savcheva and Patricia Jibben for the help in developing and testing the spot-correction code. AT thanks Loren Acton for helpful comments and wording advice. NR 10 TC 2 Z9 2 U1 0 U2 1 PU SPRINGER PI DORDRECHT PA VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS SN 0038-0938 EI 1573-093X J9 SOL PHYS JI Sol. Phys. PD JAN PY 2016 VL 291 IS 1 BP 317 EP 333 DI 10.1007/s11207-015-0823-8 PG 17 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DH6CH UT WOS:000372878100018 ER PT J AU Morita, SI Bayless, KM Yeates, DK Wiegmann, BM AF Morita, Shelah I. Bayless, Keith M. Yeates, David K. Wiegmann, Brian M. TI Molecular phylogeny of the horse flies: a framework for renewing tabanid taxonomy SO SYSTEMATIC ENTOMOLOGY LA English DT Article ID SCIONINI DIPTERA TABANIDAE; NUCLEAR GENES; DIVERGENCE TIME; RIBOSOMAL-RNA; EVOLUTION; FLY; INSECTA; INFERENCE; ALIGNMENT; MRBAYES AB Horse flies, family Tabanidae, are the most diverse family-level clade of bloodsucking insects, but their phylogeny has never been thoroughly explored using molecular data. Most adult female Tabanidae feed on nectar and on the blood of various mammals. Traditional horse fly classification tends towards large heterogeneous taxa, which impede much-needed taxonomic work. To guide renewed efforts in the systematics of horse flies and their relatives, we assembled a dataset of 110 exemplar species using nucleotide data from four genes - mitochondrial CO1, and nuclear 28S, CAD and AATS. All commonly recognized tribes in Tabanidae are represented, along with outgroups in Tabanomorpha. The phylogeny is reconstructed using Bayesian inference, and divergence times are estimated using Bayesian relaxed clock methods with time constraints from tabanid fossils. Our results show Athericidae strongly supported as the lineage most closely related to Tabanidae, and Pangoniinae and Tabaninae as monophyletic lineages. However, Chrysopsinae is nonmonophyletic, with strong support for both a nonmonophyletic Bouvieromyiini and for Rhinomyzini as sister to Tabaninae. Only the tribes Philolichini, Chrysopsini, Rhinomyzini and Haematopotini are recovered as monophyletic, although Scionini is monophyletic with exclusion of the peculiar genus Goniops Aldrich. Mycteromyia Philippi and Adersia Austen, two enigmatic genera sometimes placed in separate family-level groups, are recovered inside Pangoniini and Chrysopsini, respectively. Several species-rich genera are not recovered as monophyletic, including Esenbeckia Rondani, Silvius Meigen, Dasybasis Macquart and Tabanus L. Tabanidae likely originated in the Cretaceous, and all major extant groups were present by the early Palaeogene. This newly revised phylogenetic framework for Tabanidae forms the basis for a new assessment of tabanid diversification and provides context for understanding the evolution of trophic specialization in horse flies. C1 [Morita, Shelah I.; Bayless, Keith M.; Wiegmann, Brian M.] N Carolina State Univ, Dept Entomol, Campus Box 7613, Raleigh, NC 27695 USA. [Morita, Shelah I.] Smithsonian Inst, Dept Entomol, Washington, DC 20560 USA. [Yeates, David K.] CSIRO, Australian Natl Insect Collect, Canberra, ACT, Australia. RP Wiegmann, BM (reprint author), N Carolina State Univ, Dept Entomol, Campus Box 7613, Raleigh, NC 27695 USA. EM bwiegman@ncsu.edu RI Yeates, David/A-9917-2008 OI Yeates, David/0000-0001-7729-6143 FU US National Science Foundation [DEB-PEET 0731528]; Department of Entomology, Smithsonian Institution; National Museum of Natural History in Washington DC FX This study was supported by funds from US National Science Foundation Partnerships for Enhancing Expertise in Taxonomy (PEET) project DEB-PEET 0731528 - 'Taxonomic, Phylogenetic and Evolutionary Studies of Horse Flies (Diptera: Tabanidae): An Integrated Approach to Systematics Training' - to BMW, SIM and DKY. We gratefully acknowledge the contribution of technical, informatics and taxonomic expertise of B. K. Cassel, G. E. Kampmeier, B. D. Lessard, M. Turcatel, J. Stoffolano and F. C. Thompson. Specimens were generously contributed by the following collaborators and projects: TIGR (M. Sharkey), M. Irwin, B. Copeland, T. Erwin, A. R. Deans, B. V. Brown, D. Smith, F. D. Parker, G. Svenson, I. S. Winkler, J. LaSalle, J. Skevington, M. Buffington, M. Foldvari, M. Gates, M. Hauser, M. Petersen, M. A. Bertone, M. E. Irwin, R. Kula, R. Harin'Hala, S. Bybee, S. Cameron, T. Erwin, M. Whiting and D. Webb. We also thank the Department of Entomology, Smithsonian Institution, National Museum of Natural History in Washington DC for space and in-kind support for SIM, and J. Schaff and C. Dashiell formerly of the North Carolina State University Genomic Sciences Laboratory. NR 106 TC 3 Z9 3 U1 3 U2 11 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0307-6970 EI 1365-3113 J9 SYST ENTOMOL JI Syst. Entomol. PD JAN PY 2016 VL 41 IS 1 BP 56 EP 72 DI 10.1111/syen.12145 PG 17 WC Evolutionary Biology; Entomology SC Evolutionary Biology; Entomology GA DG4QS UT WOS:000372057800004 ER PT J AU Sohn, JC Regier, JC Mitter, C Adamski, D Landry, JF Heikkila, M Park, KT Harrison, T Mitter, K Zwick, A Kawahara, AY Cho, S Cummings, MP Schmitz, P AF Sohn, Jae-Cheon Regier, Jerome C. Mitter, Charles Adamski, David Landry, Jean-Francois Heikkilae, Maria Park, Kyu-Tek Harrison, Terry Mitter, Kim Zwick, Andreas Kawahara, Akito Y. Cho, Soowon Cummings, Michael P. Schmitz, Patric TI Phylogeny and feeding trait evolution of the mega-diverse Gelechioidea (Lepidoptera: Obtectomera): new insight from 19 nuclear genes SO SYSTEMATIC ENTOMOLOGY LA English DT Article ID MAXIMUM-LIKELIHOOD; BIOLOGICAL-CONTROL; ADVANCED MOTHS; MISSING DATA; GELECHIIDAE; CLASSIFICATION; BUTTERFLIES; RADIATION; MICROLEPIDOPTERA; COSMOPTERIGIDAE AB The Gelechioidea (>18 000 species), one of the largest superfamilies of Lepidoptera, are a major element of terrestrial ecosystems and include important pests and biological model species. Despite much recent progress, our understanding of the classification, phylogeny and evolution of Gelechioidea remains limited. Building on recent molecular studies of this superfamily and a recently revised family/subfamily classification, we provide an independent estimate of among-family relationships, with little overlap in gene sample. We analysed up to five nuclear genes, totalling 6633 bp, for each of 77 gelechioids, plus up to 14 additional genes, for a total of 14 826 bp, in 45 of those taxa and all 19 outgroup taxa. Our maximum-likelihood (ML) analyses, like those of previous authors, strongly support monophyly for most multiply-sampled families and subfamilies, but very weakly support most relationships above the family level. Our tree looks superficially divergent from that of the most recent molecular study of gelechioids, but when the previous tree is re-rooted to accord maximally with ours, the two phylogenies agree entirely on the deepest-level divergences in Gelechioidea, and strongly though incompletely on among-family relationships within the major groups. This concordance between independent studies is evidence that the groupings (or at least the unrooted branching order) are probably accurate, despite the low bootstrap values. After re-rooting, both trees divide the families into three monophyletic groups: a 'Gelechiid Assemblage,' consisting of Gelechiidae and Cosmopterigidae; a 'Scythridid Assemblage,' consisting of Stathmopodidae, Scythrididae, Blastobasidae, Elachistidae, Momphidae, Coleophoridae and Batrachedridae; and a 'Depressariid Assemblage,' consisting of Autostichidae, Xyloryctidae, Lecithoceridae, Oecophoridae, Depressariidae and Lypusidae. Within the largest family, Gelechiidae, our results strongly support the pairing of Anomologinae with Gelechiinae, in accordance with a recent study of this family. Relationships among the other subfamilies, however, conflict moderately to strongly between studies, leaving the intrafamily phylogeny unsettled. Within the 'Scythridid Assemblage,' both trees support an 'SSB clade' consisting of Blastobasidae+(Scythrididae+Stathmopodidae), strongly resolved only in our results. Coleophoridae+Batrachedridae is supported, albeit weakly, in both trees, and only Momphidae differ in position between studies. Within the 'Depressariid Assemblage,' both trees support an 'AXLO' clade consisting of Autostichidae, Xyloryctidae, Lecithoceridae and Oecophoridae. The monophyly of this clade and relationships therein are supported weakly in previous results but strongly in ours. The recently re-defined family Depressariidae is paraphyletic in our tree, but the evidence against depressariid monophyly is very weak. There is moderate support for a core group of Depressariidae consisting, among the seven subfamilies we sampled, of Depressariinae, Aeolanthinae and Hypertrophinae. We show that gelechioids have a higher total number and percentage of species that are saprophagous as larvae than any other apoditrysian superfamily, that saprophagy is concentrated primarily in the 'AXLO clade,' and that the ancestral gelechioid condition was probably feeding on live plants. Among the living-plant feeders, concealed external feeding was probably the ancestral state. The multiple origins of internal feeding of various kinds, including leaf mining (otherwise almost unknown in Apoditrysia), are restricted mostly to the Scythridid and Gelechiid Assemblages. The traits that predispose or permit lineages to adopt these unusual life histories are worthy of study. C1 [Sohn, Jae-Cheon; Regier, Jerome C.; Mitter, Charles; Mitter, Kim] Univ Maryland, Dept Entomol, 4112 Plant Sci Bldg, College Pk, MD 20742 USA. [Sohn, Jae-Cheon; Adamski, David; Heikkilae, Maria] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. [Sohn, Jae-Cheon; Heikkilae, Maria] Smithsonian Inst, Dept Paleobiol, Natl Museum Nat Hist, Washington, DC 20560 USA. [Landry, Jean-Francois] CEF, Agr & Agri Food Canada, Ottawa, ON, Canada. [Park, Kyu-Tek] Natl Acad Sci, Seoul, South Korea. [Harrison, Terry] Univ Illinois, Dept Entomol, Urbana, IL 61801 USA. [Zwick, Andreas] CSIRO Ecosyst Sci, Australian Natl Insect Collect, Canberra, ACT, Australia. [Kawahara, Akito Y.] Univ Florida, Florida Museum Nat Hist, McGuire Ctr Lepidoptera & Biodivers, Gainesville, FL 32611 USA. [Cho, Soowon] Chungbuk Natl Univ, Dept Plant Med, Cheongju, South Korea. [Cummings, Michael P.] Univ Maryland, Lab Mol Evolut, Ctr Bioinformat & Computat Biol, College Pk, MD 20742 USA. [Schmitz, Patric] Univ Hawaii, PEPS, Honolulu, HI 96822 USA. RP Mitter, C (reprint author), Univ Maryland, Dept Entomol, 4112 Plant Sci Bldg, College Pk, MD 20742 USA. EM cmitter@umd.edu RI Zwick, Andreas/A-5735-2015 FU U.S. National Science Foundation's Assembling the Tree of Life program [0531626, 0531769]; U.S. National Science Foundation [DBI-0755048, DEB1355028, DEB-1355023]; Hatch funds of the Maryland Agricultural Experiment Station FX We are indebted to many generous colleagues who provided specimens for this study, including Leif Aarvik, David Agassiz, Joaquin Baixeras, John W. Brown, Timothy P. Friedlander, Jaga Giebultowicz, Peter Hattenschwiler, Ronald Hodges, Bernard Landry, David C. Lees, Marcus J. Matthews, Wolfram Mey, Andrew Mitchell, Ebbe S. Nielsen, Kenji Nishida, Olle Pellmyr and Jadranka Rota. We thank three contributors to the 'UK moths' website (www.ukmoths.org.uk), Tristan Bantock, Ian Kimber, and Mark Lawlor, for providing photos of gelechioid larval feeding, and Ian McMillan for information about Australian Xyloryctidae. The grid-based phylogenetic analyses were made possible by expert support from Adam Bazinet. Financial support was provided by the U.S. National Science Foundation's Assembling the Tree of Life program, award numbers 0531626 and 0531769; U.S. National Science Foundation awards DBI-0755048, DEB1355028 and DEB-1355023; and the Hatch funds of the Maryland Agricultural Experiment Station. Finally, we thank the two anonymous reviewers for their very helpful comments. NR 99 TC 5 Z9 5 U1 2 U2 9 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0307-6970 EI 1365-3113 J9 SYST ENTOMOL JI Syst. Entomol. PD JAN PY 2016 VL 41 IS 1 BP 112 EP 132 DI 10.1111/syen.12143 PG 21 WC Evolutionary Biology; Entomology SC Evolutionary Biology; Entomology GA DG4QS UT WOS:000372057800007 ER PT J AU Winterton, SL Hardy, NB Gaimari, SD Hauser, M Hill, HN Holston, KC Irwin, ME Lambkin, CL Metz, MA Turco, F Webb, D Yang, LL Yeates, DK Wiegmann, BM AF Winterton, Shaun L. Hardy, Nate B. Gaimari, Stephen D. Hauser, Martin Hill, Hilary N. Holston, Kevin C. Irwin, Michael E. Lambkin, Christine L. Metz, Mark A. Turco, Federica Webb, Donald Yang, Longlong Yeates, David K. Wiegmann, Brian M. TI The phylogeny of stiletto flies (Diptera: Therevidae) SO SYSTEMATIC ENTOMOLOGY LA English DT Article ID HIGHER-LEVEL PHYLOGENY; LYNEBORG DIPTERA; AUSTRALIA DIPTERA; ANABARHYNCHUS MACQUART; XESTOMYZINAE DIPTERA; NANEXILA WINTERTON; TAENOGERA KROBER; BONJEANIA IRWIN; ACUPALPA KROBER; GENE-SEQUENCES AB The therevoid clade represents a group of four families (Apsilocephalidae, Evocoidae, Scenopinidae and Therevidae) of lower brachyceran Diptera in the superfamily Asiloidea. The largest of these families is that of the stiletto flies (Therevidae). A large-scale (i.e. supermatrix) phylogeny of Therevidae is presented based on DNA sequence data from seven genetic loci (16S, 18S and 28S ribosomal DNA and four protein-encoding genes: elongation factor 1-alpha, triose phosphate isomerase, short-wavelength rhodopsin and the CPSase region of carbamoyl-phosphate synthase-aspartate transcarbamoylase-dihydroorotase). Results are presented from Bayesian phylogenetic analyses of approximately 8.7 kb of sequence data for 204 taxa representing all subfamilies and genus groups of Therevidae. Our results strongly support the sister-group relationship between Therevidae and Scenopinidae, with Apsilocephalidae as sister to Evocoidae. Previous estimates of stiletto fly phylogeny based on morphology or DNA sequence data, or supertree analysis, have failed to find significant support for relationships among subfamilies. We report for the first time strong support for the placement of the subfamily Phycinae as sister to the remaining Therevidae, originating during the Mid Cretaceous. As in previous studies, the sister-group relationship between the species-rich subfamilies Agapophytinae and Therevinae is strongly supported. Agapophytinae are recovered as monophyletic, inclusive of the Taenogera group. Therevinae comprise the bulk of the species richness in the family and appear to be a relatively recent and rapid radiation originating in the southern hemisphere (Australia+Antarctica+South America) during the Late Cretaceous. Genus groups are defined for all subfamilies based on these results. C1 [Winterton, Shaun L.; Gaimari, Stephen D.; Hauser, Martin] Calif Dept Food & Agr, Calif State Collect Arthropods, 3294 Meadowview Rd, Sacramento, CA 95832 USA. [Hardy, Nate B.] Auburn Univ, Dept Entomol & Plant Pathol, Auburn, AL 36849 USA. [Hill, Hilary N.] US EPA, Washington, DC 20460 USA. [Holston, Kevin C.] Swedish Museum Nat Hist, S-10405 Stockholm, Sweden. [Irwin, Michael E.; Webb, Donald] Illinois Nat Hist Survey, Champaign, IL 61820 USA. [Lambkin, Christine L.; Turco, Federica] Queensland Museum, POB 300, Brisbane, Qld 4101, Australia. [Metz, Mark A.] Smithsonian Inst, Washington, DC 20560 USA. [Yang, Longlong] Ctr Hlth Res, CIIT, Raleigh, NC USA. [Yeates, David K.] CSIRO, Nat Res Collect Australia, Canberra, ACT, Australia. [Wiegmann, Brian M.] N Carolina State Univ, Dept Entomol, Raleigh, NC 27695 USA. RP Winterton, SL (reprint author), Calif Dept Food & Agr, Calif State Collect Arthropods, 3294 Meadowview Rd, Sacramento, CA 95832 USA. EM wintertonshaun@gmail.com RI Yeates, David/A-9917-2008 OI Yeates, David/0000-0001-7729-6143 FU National Science Foundation (NSF) [DEB-0614213, DEB-9521925, DEB-9977958]; Schlinger Foundation; Australian Biological Resources Study [ABRS-209-48, BBR-210-40] FX Funding for this study and those that formed the basis of this work was provided by the National Science Foundation (NSF) (DEB-0614213, DEB-9521925 and DEB-9977958), the Schlinger Foundation and the Australian Biological Resources Study (ABRS-209-48, BBR-210-40). Statements and viewpoints expressed herein do not necessarily reflect the views of the NSF or ABRS. We thank the three anonymous reviewers for their useful comments on the manuscript. NR 107 TC 2 Z9 2 U1 3 U2 4 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0307-6970 EI 1365-3113 J9 SYST ENTOMOL JI Syst. Entomol. PD JAN PY 2016 VL 41 IS 1 BP 144 EP 161 DI 10.1111/syen.12147 PG 18 WC Evolutionary Biology; Entomology SC Evolutionary Biology; Entomology GA DG4QS UT WOS:000372057800009 ER PT J AU Funk, VA Pasini, E Bonifacino, JM Katinas, L AF Funk, Vicki A. Pasini, Eduardo Mauricio Bonifacino, J. Katinas, Liliana TI Home at last: the enigmatic genera Eriachaenium and Adenocaulon (Compositae, Mutisioideae, Mutisieae, Adenocaulinae) SO PHYTOKEYS LA English DT Article DE Asteraceae; dimorphic flowers; endemism; Patagonia; Asia-North America disjunct ID PHYLOGENETIC ANALYSIS; CHROMOSOME NUMBERS; ASTERACEAE; POLLEN; SENECIONEAE; TRIBE AB The genera Eriachaenium and Adenocaulon (Compositae) have distinct but complex histories and both have been placed in a number of tribes across the family. For the first time the two genera are included in a molecular study and the results show that they are best placed in the tribe Mutisieae s.s. and are the only genera in the re-instated subtribe Adenocaulinae. When described, this subtribe contained only Adenocaulon and was found in the Inuleae. The study also confirms one of the conclusions of a recent morphological study that Eriachaenium and Adenocaulon are sister taxa. Past difficulties in tribal assignment are attributed to the distinct and unusual morphology of each genus. Both genera and the subtribe are described and a key to separate the genera is provided. C1 [Funk, Vicki A.; Pasini, Eduardo; Mauricio Bonifacino, J.; Katinas, Liliana] Smithsonian Inst, Dept Bot, NMNH, Washington, DC 20560 USA. [Pasini, Eduardo] Univ Fed Rio Grande do Sul, Programa Posgrad Bot, Ave Bento Goncalves 9500, BR-91501970 Porto Alegre, RS, Brazil. [Mauricio Bonifacino, J.] Univ Republica, Fac Agron, Lab Bot 3, Ave Garzon 780, Montevideo 12900, Uruguay. [Katinas, Liliana] Museo La Plata, Div Plantas Vasculares, Paseo Bosque S-N, RA-1900 La Plata, Buenos Aires, Argentina. RP Funk, VA (reprint author), Smithsonian Inst, Dept Bot, NMNH, Washington, DC 20560 USA. EM funkv@si.edu FU Office of the Undersecretary for Science; Natural History Museum; Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES); PEDEDIBA (Udelar); Facultad de Agronomia (Udelar); CONICET (Argentina) [PIP 0729]; ANPCyT (Argentina) [PICT 1683] FX A number of colleagues helped us during the course of this study and we are very grateful. In particular we thank: Gisela Sancho (LP) for her participation in the 2009 field trip to Patagonia; Raymund Chan, Carol Kelloff and Gabe Johnson (US) for their assistance in the lab; the Laboratory of Analytical Biology at the Museum Support Center (Smithsonian) where the lab work was done; the last two authors thank PEDEDIBA and we all thank the herbaria where we examined the specimens (LP, NY, US). A special thanks to our funding sources: the Pell grant program from the Office of the Undersecretary for Science for funding the field trip and lab work and the Natural History Museum for funding publication costs (Smithsonian Institution); The second author would like to thank Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES) for financial support and for providing an international scholarship to work at the National Museum of Natural History (NMNH) of the Smithsonian Institution. Additional funding supplied by PEDEDIBA and Facultad de Agronomia (Udelar); PIP 0729 from CONICET (Argentina) and PICT 1683 from ANPCyT (Argentina). Finally, we thank the editors of the amazing online databases that we use daily and often forget to mention: International Plant Names Index, JSTOR Global Plants, Index Herbariorum, and Index to chromosome numbers in Asteraceae (IPNI 2012, JSTOR-GP continuously updated, Thiers continuously updated, Watanabe 2015). NR 50 TC 2 Z9 2 U1 0 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 60 BP 1 EP 19 DI 10.3897/phytokeys.60.6795 PG 19 WC Plant Sciences SC Plant Sciences GA DG0QB UT WOS:000371769500001 ER PT J AU Robinson, H Skvarla, JJ Funk, VA AF Robinson, Harold Skvarla, John J. Funk, Vicki A. TI Vernonieae (Asteraceae) of southern Africa: A generic disposition of the species and a study of their pollen SO PHYTOKEYS LA English DT Article DE Asteraceae; Baccharoides; Bothriocline; Botswana; Compositae; Cyanthillium; Distephanus; Erlangea; Ethulia; Gymnanthemum; Hilliardiella; Lesotho; Namibia; Namibithamnus; new combinations; new genera; Oocephala; Orbivestus; Parapolydora; pollen; Polydora; Pseudopegolettia; South Africa; Swaziland; Vernonella; Vernonia; Vernoniastrum; Vernonieae ID GYMNANTHEMINAE VERNONIEAE; CHROMOSOME-NUMBERS; INDIAN COMPOSITAE; GENUS; RESTORATION; CHINA AB Current and previously included members of the Tribe Vernonieae (Asteraceae) of southern Africa are listed in their presently recognized genera with complete synonymies and keys to genera and species. The genus Vernonia, as presently delimited, does not occur in Africa. Genera of the Vernonieae presently recognized from southern Africa are Baccharoides, Bothriocline, Cyanthillium, Distephanus, Erlangea, Ethulia, Gymnanthemum, Hilliardiella, Oocephala, Orbivestus, Parapolydora, Polydora, Vernonella, Vernoniastrum, plus two genera that are named as new: Namibithamnus and Pseudopegolettia. Twelve new combinations are provided and two species, V. potamiphila and V. collinii Klatt., hom. illeg., remain unplaced because of a lack of material. Pollen types are illustrated including previously recognized types: non-lophate, sublophate, tricolporate lophate, and non-colpate triporate lophate. A type previously unknown in the Asteraceae is described here and in a separate paper for Oocephala and Polydora; a non-colpate pantoporate lophate type with pores not strictly equatorial. C1 [Robinson, Harold; Funk, Vicki A.] Smithsonian Inst, Dept Bot, NMNH, MRC 166,POB 37012, Washington, DC 20013 USA. [Skvarla, John J.] Univ Oklahoma, Dept Bot & Microbiol, Norman, OK 73019 USA. [Skvarla, John J.] Univ Oklahoma, Oklahoma Biol Survey, Norman, OK 73019 USA. RP Robinson, H (reprint author), Smithsonian Inst, Dept Bot, NMNH, MRC 166,POB 37012, Washington, DC 20013 USA. EM robinsoh@si.edu NR 59 TC 1 Z9 1 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 60 BP 49 EP 126 DI 10.3897/phytokeys.60.6734 PG 78 WC Plant Sciences SC Plant Sciences GA DG0QB UT WOS:000371769500004 ER PT J AU Beaudrot, L Ahumada, JA O'Brien, T Alvarez-Loayza, P Boekee, K Campos-Arceiz, A Eichberg, D Espinosa, S Fegraus, E Fletcher, C Gajapersad, K Hallam, C Hurtado, J Jansen, PA Kumar, A Larney, E Lima, MGM Mahony, C Martin, EH McWilliam, A Mugerwa, B Ndoundou-Hockemba, M Razafimahaimodison, JC Romero-Saltos, H Rovero, F Salvador, J Santos, F Sheil, D Spironello, WR Willig, MR Winarni, NL Zvoleff, A Andelman, SJ AF Beaudrot, Lydia Ahumada, Jorge A. O'Brien, Timothy Alvarez-Loayza, Patricia Boekee, Kelly Campos-Arceiz, Ahimsa Eichberg, David Espinosa, Santiago Fegraus, Eric Fletcher, Christine Gajapersad, Krisna Hallam, Chris Hurtado, Johanna Jansen, Patrick A. Kumar, Amit Larney, Eileen Moreira Lima, Marcela Guimaraes Mahony, Colin Martin, Emanuel H. McWilliam, Alex Mugerwa, Badru Ndoundou-Hockemba, Mireille Razafimahaimodison, Jean Claude Romero-Saltos, Hugo Rovero, Francesco Salvador, Julia Santos, Fernanda Sheil, Douglas Spironello, Wilson R. Willig, Michael R. Winarni, Nurul L. Zvoleff, Alex Andelman, Sandy J. TI Standardized Assessment of Biodiversity Trends in Tropical Forest Protected Areas: The End Is Not in Sight SO PLOS BIOLOGY LA English DT Article ID BIOLOGICAL DIVERSITY; PROJECTED IMPACTS; MONITORING CHANGE; LAND-USE; CONSERVATION; MAMMALS; TIME; EXTINCTION; OCCUPANCY; DECLINES AB Extinction rates in the Anthropocene are three orders of magnitude higher than background and disproportionately occur in the tropics, home of half the world's species. Despite global efforts to combat tropical species extinctions, lack of high-quality, objective information on tropical biodiversity has hampered quantitative evaluation of conservation strategies. In particular, the scarcity of population-level monitoring in tropical forests has stymied assessment of biodiversity outcomes, such as the status and trends of animal populations in protected areas. Here, we evaluate occupancy trends for 511 populations of terrestrial mammals and birds, representing 244 species from 15 tropical forest protected areas on three continents. For the first time to our knowledge, we use annual surveys from tropical forests worldwide that employ a standardized camera trapping protocol, and we compute data analytics that correct for imperfect detection. We found that occupancy declined in 22%, increased in 17%, and exhibited no change in 22% of populations during the last 3-8 years, while 39% of populations were detected too infrequently to assess occupancy changes. Despite extensive variability in occupancy trends, these 15 tropical protected areas have not exhibited systematic declines in biodiversity (i.e., occupancy, richness, or evenness) at the community level. Our results differ from reports of widespread biodiversity declines based on aggregated secondary data and expert opinion and suggest less extreme deterioration in tropical forest protected areas. We simultaneously fill an important conservation data gap and demonstrate the value of large-scale monitoring infrastructure and powerful analytics, which can be scaled to incorporate additional sites, ecosystems, and monitoring methods. In an era of catastrophic biodiversity loss, robust indicators produced from standardized monitoring infrastructure are critical to accurately assess population outcomes and identify conservation strategies that can avert biodiversity collapse. C1 [Beaudrot, Lydia; Ahumada, Jorge A.; Fegraus, Eric; Zvoleff, Alex; Andelman, Sandy J.] Conservat Int, Moore Ctr Sci, Arlington, VA USA. [O'Brien, Timothy] Wildlife Conservat Soc, Bronx, NY USA. [Alvarez-Loayza, Patricia] Duke Univ, Ctr Trop Conservat, Durham, NC USA. [Boekee, Kelly] Wageningen Univ, Dept Environm Sci, NL-6700 AP Wageningen, Netherlands. [Campos-Arceiz, Ahimsa] Univ Nottingham, Mindset Interdisciplinary Ctr Trop Environm Studi, Sch Geog, Malaysia Campus, Selangor, Malaysia. [Eichberg, David] HP Inc, HP Sustainabil, Palo Alto, CA USA. [Espinosa, Santiago] Pontificia Univ Catolica Ecuador, Escuela Ciencias Biol, Quito, Ecuador. [Fletcher, Christine] Forest Res Inst Malaysia, Kepong, Selangor, Malaysia. [Gajapersad, Krisna] Conservat Int Suriname, Paramaribo, Surinam. [Hallam, Chris] Lao PDR Program, Wildlife Conservat Soc, Viangchan, Laos. [Hurtado, Johanna] Org Trop Studies, La Selva Biol Stn, Puerto Viejo de Sarapiqui, Costa Rica. [Jansen, Patrick A.] Smithsonian Trop Res Inst, Ctr Trop Forest Sci, Panama City, Panama. [Kumar, Amit] Hewlett Packard Enterprise, Enterprise Serv, Palo Alto, CA USA. [Larney, Eileen] Ctr ValBio, Ranomafana, Madagascar. [Larney, Eileen] SUNY Stony Brook, Stony Brook, NY 11794 USA. [Moreira Lima, Marcela Guimaraes; Santos, Fernanda] Fed Univ Para, Museu Paraense Emilio Goeldi, BR-66059 Belem, Para, Brazil. [Mahony, Colin] Hewlett Packard Enterprise Big Data, Palo Alto, CA USA. [Martin, Emanuel H.] Udzungwa Ecol Monitoring Ctr, Udzungwa Mt Natl Pk, Mangula, Tanzania. [Martin, Emanuel H.] Sokoine Univ Agr, Morogoro, Tanzania. [Mugerwa, Badru] MUST, ITFC, Mbarara, Uganda. [Mugerwa, Badru] Univ Western Ontario, Dept Biol, London, ON, Canada. [Mugerwa, Badru] Univ Oxford, Wildlife Conservat Res Unit WildCRU, Oxford, England. [Ndoundou-Hockemba, Mireille] Congo Program, Wildlife Conservat Soc, Brazzaville, Congo. [Romero-Saltos, Hugo] Yachay Tech Univ, Dept Biol, Urcuqui, Imbabura, Ecuador. [Rovero, Francesco] MUSE Museo Sci, Trop Biodivers, Trento, Italy. [Salvador, Julia] Univ Florida, Dept Wildlife Ecol & Conservat, Gainesville, FL USA. [Sheil, Douglas] Norwegian Univ Life Sci NMBU, Dept Ecol & Nat INA Resource Management, As, Norway. [Sheil, Douglas] Ctr Int Forestry Res, Bogor, Indonesia. [Spironello, Wilson R.] Natl Inst Amazonian Res INPA, Manaus, Amazonas, Brazil. [Willig, Michael R.] Univ Connecticut, Dept Ecol & Evolutionary Biol, Storrs, CT USA. [Willig, Michael R.] Univ Connecticut, Ctr Environm Sci & Engn, Storrs, CT USA. [Winarni, Nurul L.] Univ Indonesia, Res Ctr Climate Change, Depok, Indonesia. RP Beaudrot, L; Ahumada, JA (reprint author), Conservat Int, Moore Ctr Sci, Arlington, VA USA. EM beaudrot@umich.edu; jahumada@conservation.org RI Sheil, Douglas/A-3867-2015; OI Sheil, Douglas/0000-0002-1166-6591; Winarni, Nurul Laksmi/0000-0001-6343-3805 FU Gordon and Betty Moore Foundation; Northrop Grumman Foundation; Hewlett Packard Living Progress; Conservation International FX This study was funded by the Gordon and Betty Moore Foundation, Northrop Grumman Foundation and other donors. Hewlett Packard Living Progress, in partnership with Conservation International, contributed funding to enable the bulk of the occupancy modeling and generation of the Wildlife Picture Index through software development and hardware in kind donations. DE and AK from Hewlett Packard Company contributed to the manuscript by providing descriptions of the software and hardware used for the analysis. Apart from this the funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript. NR 84 TC 9 Z9 10 U1 15 U2 32 PU PUBLIC LIBRARY SCIENCE PI SAN FRANCISCO PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA SN 1545-7885 J9 PLOS BIOL JI PLoS. Biol. PD JAN PY 2016 VL 14 IS 1 AR e1002357 DI 10.1371/journal.pbio.1002357 PG 21 WC Biochemistry & Molecular Biology; Biology SC Biochemistry & Molecular Biology; Life Sciences & Biomedicine - Other Topics GA DG2FU UT WOS:000371882900023 PM 26785119 ER PT J AU Benson, RBJ Butler, RJ Alroy, J Mannion, PD Carrano, MT Lloyd, GT AF Benson, Roger B. J. Butler, Richard J. Alroy, John Mannion, Philip D. Carrano, Matthew T. Lloyd, Graeme T. TI Near-Stasis in the Long-Term Diversification of Mesozoic Tetrapods SO PLOS BIOLOGY LA English DT Article ID PHANEROZOIC TAXONOMIC DIVERSITY; NORTH-AMERICAN MAMMALS; FOSSIL RECORD; SPECIES-DIVERSITY; ANGIOSPERM DIVERSIFICATION; CONTINENTAL SCALES; GLOBAL DIVERSITY; SAMPLING BIASES; MASS EXTINCTION; KINETIC-MODEL AB How did evolution generate the extraordinary diversity of vertebrates on land? Zero species are known prior to similar to 380 million years ago, and more than 30,000 are present today. An expansionist model suggests this was achieved by large and unbounded increases, leading to substantially greater diversity in the present than at any time in the geological past. This model contrasts starkly with empirical support for constrained diversification in marine animals, suggesting different macroevolutionary processes on land and in the sea. We quantify patterns of vertebrate standing diversity on land during the Mesozoic-early Paleogene interval, applying sample-standardization to a global fossil dataset containing 27,260 occurrences of 4,898 non-marine tetrapod species. Our results show a highly stable pattern of Mesozoic tetrapod diversity at regional and local levels, underpinned by a weakly positive, but near-zero, long-term net diversification rate over 190 million years. Species diversity of non-flying terrestrial tetrapods less than doubled over this interval, despite the origins of exceptionally diverse extant groups within mammals, squamates, amphibians, and dinosaurs. Therefore, although speciose groups of modern tetrapods have Mesozoic origins, rates of Mesozoic diversification inferred from the fossil record are slow compared to those inferred from molecular phylogenies. If high speciation rates did occur in the Mesozoic, then they seem to have been balanced by extinctions among older clades. An apparent 4-fold expansion of species richness after the Cretaceous/Paleogene (K/Pg) boundary deserves further examination in light of potential taxonomic biases, but is consistent with the hypothesis that global environmental disturbances such as mass extinction events can rapidly adjust limits to diversity by restructuring ecosystems, and suggests that the gradualistic evolutionary diversification of tetrapods was punctuated by brief but dramatic episodes of radiation. C1 [Benson, Roger B. J.] Univ Oxford, Dept Earth Sci, Oxford OX1 3PR, England. [Butler, Richard J.] Univ Birmingham, Sch Geog Earth & Environm Sci, Birmingham, W Midlands, England. [Alroy, John; Lloyd, Graeme T.] Macquarie Univ, Dept Biol Sci, N Ryde, NSW 2109, Australia. [Mannion, Philip D.] Univ London Imperial Coll Sci Technol & Med, Dept Earth Sci & Engn, London, England. [Carrano, Matthew T.] Smithsonian Inst, Dept Paleobiol, Washington, DC 20560 USA. RP Benson, RBJ (reprint author), Univ Oxford, Dept Earth Sci, Oxford OX1 3PR, England. EM roger.benson@earth.ox.ac.uk RI Alroy, John/B-4585-2009; Carrano, Matthew/C-7601-2011; Butler, Richard/A-5239-2011; OI Carrano, Matthew/0000-0003-2129-1612; Butler, Richard/0000-0003-2136-7541; Benson, Roger/0000-0001-8244-6177 FU European Union's Horizon 2020 research and innovation programme (ERC Starting Grant: TERRA) [637483]; Imperial College London Junior Research Fellowship; Leverhulme Trust Early Career Fellowship [ECF-2014- 398 662] FX RJB received funding from the European Union's Horizon 2020 research and innovation programme 2014-2018 under grant agreement 637483 (ERC Starting Grant: TERRA). PDM is supported by an Imperial College London Junior Research Fellowship and Leverhulme Trust Early Career Fellowship (ECF-2014- 398 662). The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript. NR 100 TC 5 Z9 5 U1 10 U2 19 PU PUBLIC LIBRARY SCIENCE PI SAN FRANCISCO PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA SN 1545-7885 J9 PLOS BIOL JI PLoS. Biol. PD JAN PY 2016 VL 14 IS 1 AR e1002359 DI 10.1371/journal.pbio.1002359 PG 27 WC Biochemistry & Molecular Biology; Biology SC Biochemistry & Molecular Biology; Life Sciences & Biomedicine - Other Topics GA DG2FU UT WOS:000371882900025 PM 26807777 ER PT J AU Wallbank, RWR Baxter, SW Pardo-Diaz, C Hanly, JJ Martin, SH Mallet, J Dasmahapatra, KK Salazar, C Joron, M Nadeau, N McMillan, WO Jiggins, CD AF Wallbank, Richard W. R. Baxter, Simon W. Pardo-Diaz, Carolina Hanly, Joseph J. Martin, Simon H. Mallet, James Dasmahapatra, Kanchon K. Salazar, Camilo Joron, Mathieu Nadeau, Nicola McMillan, W. Owen Jiggins, Chris D. TI Evolutionary Novelty in a Butterfly Wing Pattern through Enhancer Shuffling SO PLOS BIOLOGY LA English DT Article ID HELICONIUS-BUTTERFLIES; ADAPTIVE EVOLUTION; COLOR PATTERN; MIMICRY; GENE; DIVERGENCE; DROSOPHILA; STICKLEBACKS; EXPRESSION; UNDERLIES AB An important goal in evolutionary biology is to understand the genetic changes underlying novel morphological structures. We investigated the origins of a complex wing pattern found among Amazonian Heliconius butterflies. Genome sequence data from 142 individuals across 17 species identified narrow regions associated with two distinct red colour pattern elements, dennis and ray. We hypothesise that these modules in non-coding sequence represent distinct cis-regulatory loci that control expression of the transcription factor optix, which in turn controls red pattern variation across Heliconius. Phylogenetic analysis of the two elements demonstrated that they have distinct evolutionary histories and that novel adaptive morphological variation was created by shuffling these cis-regulatory modules through recombination between divergent lineages. In addition, recombination of modules into different combinations within species further contributes to diversity. Analysis of the timing of diversification in these two regions supports the hypothesis of introgression moving regulatory modules between species, rather than shared ancestral variation. The dennis phenotype introgressed into Heliconius melpomene at about the same time that ray originated in this group, while ray introgressed back into H. elevatus much more recently. We show that shuffling of existing enhancer elements both within and between species provides a mechanism for rapid diversification and generation of novel morphological combinations during adaptive radiation. C1 [Wallbank, Richard W. R.; Pardo-Diaz, Carolina; Hanly, Joseph J.; Martin, Simon H.; Jiggins, Chris D.] Univ Cambridge, Dept Zool, Cambridge, England. [Wallbank, Richard W. R.; Pardo-Diaz, Carolina; Hanly, Joseph J.; Mallet, James; Dasmahapatra, Kanchon K.; Salazar, Camilo; Joron, Mathieu; McMillan, W. Owen; Jiggins, Chris D.] Smithsonian Trop Res Inst, Balboa, Ancon, Panama. [Baxter, Simon W.] Univ Adelaide, Sch Biol Sci, Adelaide, SA, Australia. [Pardo-Diaz, Carolina; Salazar, Camilo] Univ Rosario, Fac Nat Sci & Math, Biol Program, Bogota, DC, Colombia. [Mallet, James] Harvard Univ, Organism & Evolutionary Biol, Harvard, MA USA. [Dasmahapatra, Kanchon K.] Univ York, Dept Biol, York YO10 5DD, N Yorkshire, England. [Joron, Mathieu] Museum Natl Hist Nat, CNRS MNHN UPMC EPHE, UMR 7205, Inst Systemat Evolut & Biodiversite,CP50, F-75231 Paris, France. [Joron, Mathieu] Univ Montpellier 3, Univ Montpellier, EPHE,CNRS, Ctr Ecol Fonct & Evolut,UMR 5175, F-34032 Montpellier, France. [Nadeau, Nicola] Univ Sheffield, Dept Anim & Plant Sci, Sheffield S10 2TN, S Yorkshire, England. RP Jiggins, CD (reprint author), Univ Cambridge, Dept Zool, Cambridge, England.; Jiggins, CD (reprint author), Smithsonian Trop Res Inst, Balboa, Ancon, Panama. EM c.jiggins@zoo.cam.ac.uk RI mallet, james/B-5114-2008; Pardo-Diaz, Carolina/C-7936-2016; Nadeau, Nicola/E-1149-2011; Jiggins, Chris/B-9960-2008; OI Pardo-Diaz, Carolina/0000-0002-7259-1183; Nadeau, Nicola/0000-0002-9319-921X; Jiggins, Chris/0000-0002-7809-062X; Dasmahapatra, Kanchon Kumar/0000-0002-2840-7019; Salazar, Camilo/0000-0001-9217-6588 FU Biotechnology and Biological Sciences Research Council [H01439X/1]; European Research Council MimEvol grant; European Research Council Speciation Genetics FX This study was funded by the Biotechnology and Biological Sciences Research Council http://www.bbsrc.ac.uk grant number H01439X/1 to CDJ; the European Research Council MimEvol grant to MJ and the European Research Council Speciation Genetics to CDJ. The funders had no role in study design, data collection and analysis, decision to publish, or preparation of the manuscript. NR 43 TC 11 Z9 11 U1 23 U2 41 PU PUBLIC LIBRARY SCIENCE PI SAN FRANCISCO PA 1160 BATTERY STREET, STE 100, SAN FRANCISCO, CA 94111 USA SN 1545-7885 J9 PLOS BIOL JI PLoS. Biol. PD JAN PY 2016 VL 14 IS 1 AR e1002353 DI 10.1371/journal.pbio.1002353 PG 16 WC Biochemistry & Molecular Biology; Biology SC Biochemistry & Molecular Biology; Life Sciences & Biomedicine - Other Topics GA DG2FU UT WOS:000371882900020 PM 26771987 ER PT J AU Feuillet, C AF Feuillet, Christian TI Two new combinations in Euploca Nutt. (Heliotropiaceae, Boraginales) and a conspectus of the species of the Guiana Shield area SO PHYTOKEYS LA English DT Article DE Boraginales; Brazil; Euploca; Guiana Shield; Guianas; Heliotropiaceae; Venezuela AB Heliotropium foliatum and Tournefortia humilis are transferred to Euploca Nutt. respectively as Euploca foliata comb. n. and Euploca humilis comb. n. A collection from Guyana has been recently identified as Euploca humistrata, a species previously considered a Brazilian endemic. A collection from French Guiana documents for the first time the species in that country. A key to the species of the Guiana Shield area is given. The species of Euploca from the Guiana Shield are listed with synonymy and a brief description: E. filiformis, E. humilis, E. humistrata, E. lagoensis, E. polyphylla, E. procumbens. C1 [Feuillet, Christian] Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, MRC-166,POB 37012, Washington, DC 20013 USA. [Feuillet, Christian] Oregon State Univ, Dept Bot & Plant Pathol, 2082 Cordley Hall, Corvallis, OR 97331 USA. RP Feuillet, C (reprint author), Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, MRC-166,POB 37012, Washington, DC 20013 USA.; Feuillet, C (reprint author), Oregon State Univ, Dept Bot & Plant Pathol, 2082 Cordley Hall, Corvallis, OR 97331 USA. EM feuillec@science.oregonstate.edu NR 69 TC 0 Z9 0 U1 1 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 61 BP 101 EP 124 DI 10.3897/phytokeys.61.6260 PG 24 WC Plant Sciences SC Plant Sciences GA DG0QZ UT WOS:000371772000010 ER PT J AU Morfeld, KA Brown, JL AF Morfeld, Kari A. Brown, Janine L. TI Ovarian acyclicity in zoo African elephants (Loxodonta africana) is associated with high body condition scores and elevated serum insulin and leptin SO REPRODUCTION FERTILITY AND DEVELOPMENT LA English DT Article DE infertility; metabolic hormones; obesity; reproduction ID METABOLIC SYNDROME; MASS INDEX; HORMONE-SECRETION; REPRODUCTIVE CYCLICITY; ASSISTED REPRODUCTION; STIMULATING-HORMONE; INFERTILE WOMEN; NORTH-AMERICA; WEIGHT-LOSS; OBESITY AB The purpose of the present study was to determine whether excessive body fat and altered metabolic hormone concentrations in the circulation were associated with ovarian acyclicity in the world's largest land mammal, the African elephant. We compared body condition, glucose, insulin and leptin concentrations and the glucose-to-insulin ratio (G:I) between cycling (n=23; normal 14-16 week cycles based on serum progestagens for at least 2 years) and non-cycling (n=23; consistent baseline progestagen concentrations for at least 2 years) females. A validated body condition score (BCS) index (five-point scale; 1=thinnest, 5=fattest) was used to assess the degree of fatness of the study elephants. The mean BCS of non-cycling elephants was higher than that of their cycling counterparts. There were differences in concentrations of serum metabolic biomarkers, with non-cycling elephants in the BCS 5 category having higher leptin and insulin concentrations and a lower G:I ratio than cycling BCS 5 females. Using non-cycling' as the outcome variable in regression models, high BCS was a strong predictor of a non-cycling status. This study provides the first evidence that ovarian acyclicity in zoo African elephants is associated with body condition indicative of obesity, as well as elevated, perturbed biomarkers of metabolic status. C1 [Morfeld, Kari A.; Brown, Janine L.] Natl Zool Pk, Smithsonian Conservat Biol Inst, Ctr Species Survival, 1500 Remount Rd, Front Royal, VA 22630 USA. RP Morfeld, KA (reprint author), Natl Zool Pk, Smithsonian Conservat Biol Inst, Ctr Species Survival, 1500 Remount Rd, Front Royal, VA 22630 USA. EM morfeldk@si.edu FU Morris Animal Foundation; George Mason University; Smithsonian Conservation Biology Institute; Lincoln Children's Zoo FX The authors give special thanks to the following zoological facilities that provided photographs and serum samples for this project: Virginia Zoo, San Diego Safari Park, Toledo Zoo, Zoo Atlanta, Zoo Miami, Disney's Animal Kingdom, Lee Richardson Zoo, Kansas City Zoo, Nashville Zoo, Memphis Zoo, Riverbanks Zoo, Seneca Park Zoo, Oakland Zoo, Indianapolis Zoo, Knoxville Zoo and North Carolina Zoo. The authors also thank Dr Jeffery French at the University of Nebraska at Omaha for graciously providing laboratory space and equipment for the metabolic assays. We also thank the Morris Animal Foundation for funding this study. We are grateful to George Mason University, the Smithsonian Conservation Biology Institute, and Lincoln Children's Zoo for support and guidance. We also thank Dr David Wildt for valuable editorial comments. NR 77 TC 1 Z9 1 U1 6 U2 12 PU CSIRO PUBLISHING PI CLAYTON PA UNIPARK, BLDG 1, LEVEL 1, 195 WELLINGTON RD, LOCKED BAG 10, CLAYTON, VIC 3168, AUSTRALIA SN 1031-3613 EI 1448-5990 J9 REPROD FERT DEVELOP JI Reprod. Fertil. Dev. PY 2016 VL 28 IS 5 BP 640 EP 647 DI 10.1071/RD14140 PG 8 WC Developmental Biology; Reproductive Biology; Zoology SC Developmental Biology; Reproductive Biology; Zoology GA DF8RS UT WOS:000371626600011 PM 25375263 ER PT J AU Pryer, KM Huiet, L Li, FW Rothfels, CJ Schuettpelz, E AF Pryer, Kathleen M. Huiet, Layne Li, Fay-Wei Rothfels, Carl J. Schuettpelz, Eric TI Maidenhair Ferns, Adiantum, are Indeed Monophyletic and Sister to Shoestring Ferns, Vittarioids (Pteridaceae) SO SYSTEMATIC BOTANY LA English DT Article DE Epiphytes; gametophytes; molecular phylogeny; rate heterogeneity ID BAYESIAN PHYLOGENETIC INFERENCE; MOLECULAR EVOLUTION; NUCLEOTIDE-SEQUENCES; CHEILANTHOID FERNS; RBCL SEQUENCES; GAMETOPHYTES; CONFIDENCE; SELECTION; ALIGNMENT; LINEAGES AB Across the tree of life, molecular phylogenetic studies often reveal surprising relationships between taxa with radically different morphologies that have long obscured their close affiliations. A spectacular botanical example is Rafflesia, a holoparasite that produces the largest flowers in the world, but that evolved from tiny-flowered ancestors within the Euphorbiaceae. Outside of parasitic lineages, such abrupt transformations are rarely seen. One exception involves the "maidenhair ferns" (Adiantum), which are quintessential ferns: beautifully dissected, terrestrial, and shade loving. The closely related "shoestring ferns" (vittarioids), in contrast, have an extremely simplified morphology, are canopy-dwelling epiphytes, and exhibit greatly accelerated rates of molecular evolution. While Adiantum and the vittarioids together have been shown to form a robust monophyletic group (adiantoids), there remain unanswered questions regarding the monophyly of Adiantum and the evolutionary history of the vittarioids. Here we review recent phylogenetic evidence suggesting support for the monophyly of Adiantum, and analyze new plastid data to confirm this result. We find that Adiantum is monophyletic and sister to the vittarioids. With this robust phylogenetic framework established for the broadest relationships in the adiantoid Glade, we can now focus on understanding the evolutionary processes associated with the extreme morphological, ecological, and genetic transitions that took place within this lineage. C1 [Pryer, Kathleen M.; Huiet, Layne; Li, Fay-Wei] Duke Univ, Dept Biol, Durham, NC 27708 USA. [Li, Fay-Wei; Rothfels, Carl J.] Univ Calif Berkeley, Univ Herbarium, Berkeley, CA 94720 USA. [Schuettpelz, Eric] Univ Calif Berkeley, Dept Integrat Biol, Berkeley, CA 94720 USA. [Pryer, Kathleen M.] Smithsonian Inst, Dept Bot, MRC 166,POB 37012, Washington, DC 20013 USA. RP Pryer, KM (reprint author), Duke Univ, Dept Biol, Durham, NC 27708 USA.; Pryer, KM (reprint author), Smithsonian Inst, Dept Bot, MRC 166,POB 37012, Washington, DC 20013 USA. EM pryer@duke.edu FU National Science Foundation [DEB-1145614, DEB-1405181]; NSF DDIG [DEB-1110652, DEB-1407158] FX The authors thank the herbarium curators and staff of A, COLO, DUKE, GOET, P, TUR, UC, and UTC for access to specimens needed for this study. This research was funded by National Science Foundation grants DEB-1145614 to K. M. P. and L. H. and DEB-1405181 to E. S. as well as NSF DDIG awards DEB-1110652 to K. M. P. and C. J. R. and DEB-1407158 to K. M. P. and F.-W. L. Assistance from T.-T. Kao is gratefully acknowledged, as are the thoughtful comments of M. D. Windham. NR 46 TC 5 Z9 5 U1 4 U2 8 PU AMER SOC PLANT TAXONOMISTS PI LARAMIE PA UNIV WYOMING, DEPT BOTANY 3165, 1000 E UNIVERSITY AVE, LARAMIE, WY 82071 USA SN 0363-6445 EI 1548-2324 J9 SYST BOT JI Syst. Bot. PD JAN-MAR PY 2016 VL 41 IS 1 BP 17 EP 23 DI 10.1600/036364416X690660 PG 7 WC Plant Sciences; Evolutionary Biology SC Plant Sciences; Evolutionary Biology GA DF9AY UT WOS:000371653800004 ER PT J AU Lu, LM Wen, J Chen, ZD AF Lu, Limin Wen, Jun Chen, Zhiduan TI Cayratia cheniana (Vitaceae): An Endangered New Species Endemic to the Limestone Mountains of Ninh Thuan Province, Vietnam SO SYSTEMATIC BOTANY LA English DT Article DE Biodiversity conservation; chloroplast DNA; critically endangered species; habitat loss ID GRAPE FAMILY VITACEAE; PHYLOGENETIC ANALYSIS; BIOGEOGRAPHY; SEQUENCES; EVOLUTION; PLANCH. AB Considerable numbers of species have become extinct before being scientifically described, and the loss of natural habitats is known to be one of the major reasons for biodiversity declines. In this study, an endangered new species, Cayratia cheniana L. M. Lu & J. Wen, endemic to the limestone mountains of Ninh Thuan province of Vietnam is herein described based on both morphological and molecular evidence. With five chloroplast markers, Cayratia cheniana is placed as the first diverged lineage of Cayratia Juss. Morphologically, Cayratia cheniana shares synapomorphies with all other Cayratia s. s. in possessing a membrane enclosing ventral infolds in the seeds and presence of bracts on the lower part of the inflorescence axis. This species can be readily distinguished from other congeners by its tripalmate-trifoliate to bipinnate leaf architecture and stems with shredding bark. C1 [Lu, Limin; Chen, Zhiduan] Chinese Acad Sci, Inst Bot, State Key Lab Systemat & Evolutionary Bot, Beijing 100093, Peoples R China. [Wen, Jun] Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, MRC166, Washington, DC 20013 USA. RP Chen, ZD (reprint author), Chinese Acad Sci, Inst Bot, State Key Lab Systemat & Evolutionary Bot, Beijing 100093, Peoples R China.; Wen, J (reprint author), Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, MRC166, Washington, DC 20013 USA. EM wenj@si.edu; zhiduan@ibcas.ac.cn FU National Natural Science Foundation of China [NNSF 31500179, NNSF 31270268]; External Cooperation Program of BIC, Chinese Academy of Sciences [GJHZ 201321]; CAS International Research & Education Development Program [SAJC201315]; Science and Technology Basic Work [2013FY112100] FX We are grateful to Van Du Nguyen, Jingbo Zhang, and Van Hieu Nguyen for field assistance, Ai-Li Li for the line drawing, Sadaf Habib for taking seed photos, and Russell Barrett for helpful comments on the manuscript. We also thank Dr. Steven R. Manchester, one anonymous reviewer, and the Editor-in-Chief Dr. James F. Smith for their valuable suggestions. This study was supported by the National Natural Science Foundation of China (NNSF 31500179 and NNSF 31270268). Field work in Vietnam was partially supported by the External Cooperation Program of BIC, Chinese Academy of Sciences (Grant No. GJHZ 201321), CAS International Research & Education Development Program (Grant No. SAJC201315), and Science and Technology Basic Work (2013FY112100). NR 40 TC 0 Z9 0 U1 2 U2 2 PU AMER SOC PLANT TAXONOMISTS PI LARAMIE PA UNIV WYOMING, DEPT BOTANY 3165, 1000 E UNIVERSITY AVE, LARAMIE, WY 82071 USA SN 0363-6445 EI 1548-2324 J9 SYST BOT JI Syst. Bot. PD JAN-MAR PY 2016 VL 41 IS 1 BP 49 EP 55 DI 10.1600/036364416X690741 PG 7 WC Plant Sciences; Evolutionary Biology SC Plant Sciences; Evolutionary Biology GA DF9AY UT WOS:000371653800007 ER PT J AU Medeiros, H Forzza, RC Acevedo-Rodriguez, P AF Medeiros, Herison Forzza, Rafaela Campostrini Acevedo-Rodriguez, Pedro TI Wild Relatives of Guarana (Paullinia cupana, Sapindaceae) in Southwestern Brazilian Amazon SO SYSTEMATIC BOTANY LA English DT Article DE Acre; flora; Paullinieae; Sapindales; species distribution; taxonomy ID FLORA AB Paullinia species are generally laticiferous, woody climbers with a pair of watch-spring tendrils at the middle of the inflorescence, stipules, compound leaves with mostly pinnate organization, zygomorphic flowers with white corollas, septifragal capsules, and black or dark brown seeds with a white arillode. Paullinia is a Neotropical genus with approximately 220 species, one of which (P. pinnata) is also naturally found in Africa and Madagascar. Currently, 99 species are listed for Brazil, most of which are found in forest formations. The Amazon and the coastal Atlantic Forest are the two Brazilian biomes that hold the greatest diversity of Paullinia, with 73 and 26 species respectively. Surprisingly, nearly half of the Brazilian species of Paullinia (45 species, five new records for Brazil) are recorded for the Amazonian state of Acre. In the present work, we provide keys and brief species descriptions to identify the species of Paullinia found in the state of Acre. We also provide information on their distributions within Acre, and within their total range. It is noteworthy that about 70% of the species had their distribution restricted to the Amazonian domain and 44% are restricted to southwestern Amazonia, suggesting this region is a center of diversity for the genus. C1 [Medeiros, Herison; Forzza, Rafaela Campostrini] Inst Pesquisas Jardim Bot Rio de Janeiro, Pacheco Leao 915, BR-22460030 Rio De Janeiro, Brazil. [Acevedo-Rodriguez, Pedro] Smithsonian Natl Museum Nat Hist, Dept Bot, POB 37012, Washington, DC 20013 USA. RP Medeiros, H (reprint author), Inst Pesquisas Jardim Bot Rio de Janeiro, Pacheco Leao 915, BR-22460030 Rio De Janeiro, Brazil. EM medeiros.herison@gmail.com RI Forzza, Rafaela/N-9274-2015 FU CAPES (Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior); Beneficial Foundation; JRS Biodiversity Foundation FX This paper is part of the M.Sc. dissertation of the first author, presented to the Programa de Pos-Graduacao em Botanica, Jardim Botanico do Rio de Janeiro. We thank the CAPES (Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior) for the Master's scholarship awarded to the first author. We thank the Beneficial Foundation who funded the Mobilizing Taxonomic Specialists project, and the JRS Biodiversity Foundation for funding the Rescue and Integration of Botanical Data for Conservation in the Southwestern Amazon project for the financial support; the curators of the above-mentioned herbaria for their assistance; Douglas C. Daly, Flavio A. Obermuller, Marcos Silveira, Genise V. Somner, Vidal F. Mansano, Daniela Zappi and Manly M. Gomes for relevant suggestions; Edilson C. Oliveira, experienced plant collector, and the students in the University of Acre's Laboratorio de Botanica e Ecologia Vegetal for their invaluable assistance in the field. Rafaela Forzza is a CNPq Research Fellow. NR 37 TC 0 Z9 0 U1 5 U2 11 PU AMER SOC PLANT TAXONOMISTS PI LARAMIE PA UNIV WYOMING, DEPT BOTANY 3165, 1000 E UNIVERSITY AVE, LARAMIE, WY 82071 USA SN 0363-6445 EI 1548-2324 J9 SYST BOT JI Syst. Bot. PD JAN-MAR PY 2016 VL 41 IS 1 BP 202 EP 228 DI 10.1600/036364416X690606 PG 27 WC Plant Sciences; Evolutionary Biology SC Plant Sciences; Evolutionary Biology GA DF9AY UT WOS:000371653800019 ER PT J AU Tocheri, MW Dommain, R McFarlin, SC Burnett, SE Case, DT Orr, CM Roach, NT Villmoare, B Eriksen, AB Kalthoff, DC Senck, S Assefa, Z Groves, CP Jungers, WL AF Tocheri, Matthew W. Dommain, Rene McFarlin, Shannon C. Burnett, Scott E. Case, D. Troy Orr, Caley M. Roach, Neil T. Villmoare, Brian Eriksen, Amandine B. Kalthoff, Daniela C. Senck, Sascha Assefa, Zelalem Groves, Colin P. Jungers, William L. TI The Evolutionary Origin and Population History of the Grauer Gorilla SO AMERICAN JOURNAL OF PHYSICAL ANTHROPOLOGY LA English DT Article DE eastern gorilla biogeography; founder effect; genetic bottleneck; osseous and non-osseous coalitions; rare skeletal traits ID LAST GLACIAL MAXIMUM; IMPENETRABLE NATIONAL-PARK; WESTERN LOWLAND GORILLAS; SPASTIC FLAT FOOT; GENETIC DIVERSITY; MITOCHONDRIAL-DNA; EAST-AFRICA; GREAT APE; MOUNTAIN GORILLAS; LATE PLEISTOCENE AB Gorillas living in western central Africa (Gorilla gorilla) are morphologically and genetically distinguishable from those living in eastern central Africa (Gorilla beringei). Genomic analyses show eastern gorillas experienced a significant reduction in population size during the Pleistocene subsequent to geographical isolation from their western counterparts. However, how these results relate more specifically to the recent biogeographical and evolutionary history of eastern gorillas remains poorly understood. Here we show that two rare morphological traits are present in the hands and feet of both eastern gorilla subspecies at strikingly high frequencies (>60% in G. b. graueri; similar to 28% in G. b. beringei) in comparison with western gorillas (<1%). The intrageneric distribution of these rare traits suggests that they became common among eastern gorillas after diverging from their western relatives during the early to middle Pleistocene. The extremely high frequencies observed among grauer gorillas-which currently occupy a geographic range more than ten times the size of that of mountain gorillas-imply that grauers originated relatively recently from a small founding population of eastern gorillas. Current paleoenvironmental, geological, and biogeographical evidence supports the hypothesis that a small group of eastern gorillas likely dispersed westward from the Virungas into present-day grauer range in the highlands just north of Lake Kivu, either immediately before or directly after the Younger Dryas interval. We propose that as the lowland forests of central Africa expanded rapidly during the early Holocene, they became connected with the expanding highland forests along the Albertine Rift and enabled the descendants of this small group to widely disperse. The descendant populations significantly expanded their geographic range and population numbers relative to the gorillas of the Virunga Mountains and the Bwindi-Impenetrable Forest, ultimately resulting in the grauer gorilla subspecies recognized today. This founder-effect hypothesis offers some optimism for modern conservation efforts to save critically endangered eastern gorillas from extinction. (c) 2016 American Association of Physical Anthropologists C1 [Tocheri, Matthew W.] Lakehead Univ, Dept Anthropol, Thunder Bay, ON P7B 5E1, Canada. [Tocheri, Matthew W.; Dommain, Rene; Assefa, Zelalem] Smithsonian Inst, Natl Museum Nat Hist, Human Origins Program, Washington, DC 20013 USA. [McFarlin, Shannon C.] George Washington Univ, Dept Anthropol, Washington, DC 20052 USA. [McFarlin, Shannon C.] George Washington Univ, Ctr Adv Study Hominid Paleobiol, Washington, DC 20052 USA. [McFarlin, Shannon C.] Smithsonian Inst, Natl Museum Nat Hist, Div Mammals, Washington, DC 20013 USA. [Burnett, Scott E.] Eckerd Coll, Dept Anthropol, St Petersburg, FL 33711 USA. [Case, D. Troy] N Carolina State Univ, Dept Sociol & Anthropol, Raleigh, NC 27695 USA. [Orr, Caley M.] Univ Colorado, Sch Med, Dept Cell & Dev Biol, Aurora, CO 80045 USA. [Roach, Neil T.] Harvard Univ, Dept Human Evolutionary Biol, Cambridge, MA 02138 USA. [Roach, Neil T.] Amer Museum Nat Hist, Div Anthropol, New York, NY 10024 USA. [Villmoare, Brian] Univ Nevada, Dept Anthropol, Las Vegas, NV 89154 USA. [Villmoare, Brian] UCL, Dept Anthropol, London WC1H 0BW, England. [Eriksen, Amandine B.] SUNY Buffalo, Dept Anthropol, Buffalo, NY 14260 USA. [Kalthoff, Daniela C.] Swedish Museum Nat Hist, Dept Zool, S-10405 Stockholm, Sweden. [Senck, Sascha] Univ Appl Sci Upper Austria, Fak Tech & Umweltwissensch, A-4600 Wels, Austria. [Groves, Colin P.] Australian Natl Univ, Sch Archaeol & Anthropol, GPO Box 4, Canberra, ACT 0200, Australia. [Jungers, William L.] SUNY Stony Brook, Med Ctr, Dept Anat Sci, Stony Brook, NY 11794 USA. [Jungers, William L.] Assoc Vahatra, BP 3972, Madagascar, Madagascar. RP Tocheri, MW (reprint author), Lakehead Univ, Dept Anthropol, Thunder Bay, ON P7B 5E1, Canada. EM tocherim@gmail.com OI Tocheri, Matthew/0000-0001-7600-8998 FU Wenner-Gren Foundation [7822]; Smithsonian Institution's Scholarly Studies Grant Program; Canada Research Chairs Program; National Science Foundation [BCS-0852866, BCS-0964944]; National Geographic Society Committee for Research and Exploration [8486-08]; Leakey Foundation; George Washington University Center; Institute Facilitating Fund FX Grant sponsor: Wenner-Gren Foundation; Grant number: 7822; Grant sponsor: Smithsonian Institution's Scholarly Studies Grant Program; Grant sponsor: Canada Research Chairs Program; Grant sponsor: National Science Foundation; Grant number: BCS-0852866 and BCS-0964944; Grant sponsor: National Geographic Society Committee for Research and Exploration; Grant number: 8486-08; Grant sponsor: The Leakey Foundation; Grant sponsor: The George Washington University Center and Institute Facilitating Fund. NR 173 TC 1 Z9 1 U1 13 U2 18 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0002-9483 EI 1096-8644 J9 AM J PHYS ANTHROPOL JI Am. J. Phys. Anthropol. PD JAN PY 2016 VL 159 SU 61 BP 4 EP 18 DI 10.1002/ajpa.22900 PG 15 WC Anthropology; Evolutionary Biology SC Anthropology; Evolutionary Biology GA DF3PU UT WOS:000371257900002 ER PT J AU Pobiner, B AF Pobiner, Briana TI Accepting, Understanding, Teaching, and Learning (Human) Evolution: Obstacles and Opportunities SO AMERICAN JOURNAL OF PHYSICAL ANTHROPOLOGY LA English DT Article DE human evolution; evolution education; evolution misconceptions; science denial; outreach ID HIGH-SCHOOL BIOLOGY; NATURAL-SELECTION; COLLEGE-STUDENTS; SCIENCE-EDUCATION; TREE-THINKING; CONCEPTUAL CHANGE; PUBLIC-SCHOOLS; UNITED-STATES; TEACHERS CONCEPTIONS; UNIVERSITY-STUDENTS AB Questions about our origin as a species are universal and compelling. Evolution-and in particular human evolution-is a subject that generates intense interest across the world, evidenced by the fact that fossil and DNA discoveries grace the covers of major science journals and magazines as well as other popular print and online media. However, virtually all national polls indicate that the majority of Americans strongly reject biological evolution as a fact-based, well-tested, and robust understanding of the history of life. In the popular mind, no topic in all of science is more contentious or polarizing than evolution and media sources often only serve to magnify this polarization by covering challenges to the teaching of evolution. In the realm of teaching, debates about evolution have shaped textbooks, curricula, standards, and policy. Challenges to accepting and understanding evolution include mistrust and denial of science, cognitive obstacles and misconceptions, language and terminology, and a religious worldview, among others. Teachers, who are on the front lines of these challenges, must be armed with the tools and techniques to teach evolution in formal education settings across grades K-16 in a straightforward, thorough, and sensitive way. Despite the potentially controversial topic of human evolution, growing research is demonstrating that a pedagogical focus on human examples is an effective and engaging way to teach core concepts of evolutionary biology. (c) 2016 American Association of Physical Anthropologists C1 [Pobiner, Briana] Natl Museum Nat Hist, Smithsonian Inst, Dept Anthropol, Human Origins Program, Washington, DC 20560 USA. RP Pobiner, B (reprint author), MRC 112 Smithsonians Natl Museum Nat Hist, Dept Anthropol, Human Origins Program, 10th St & Constitut Ave, Washington, DC 20560 USA. EM pobinerb@si.edu FU National Science Foundation [1119468] FX I thank Robin Bernstein for the invitation to write this paper and for the thoughtful comments and suggestions by Trudy Turner (Editor), Shara Bailey (Associate Editor), and the two reviewers. I am grateful to many people who continue to stimulate my thinking and interest in this area, including (but not exclusive to): Paul Beardsley, Connie Bertka, Jennifer Clark, Holly Dunsworth, Amanda Glaze, T. Ryan Gregory, Norman Johnson, Jay Labov, David Long, Louise Mead, Lee Meadows, Rick Potts, Melissa Wilson Sayres, Caitlin Schrein, Judy Scotchmoor, Eugenie Scott, Jim Smith, Anna Thanukos, Bill Watson, Jory Weintraub, my other friends and colleagues at the National Museum of Natural History, and all the not-yetspecifically- named members of the "Communicating the Relevance of Human Evolution" working group at the National Evolutionary Synthesis Center (NESCent). This paper included links and references to material based upon work supported by the National Science Foundation under Grant No. 1119468 for the "Teaching Evolution through Human Examples" project, and I thank all the teachers and students who helped us field test the materials developed by the project. I also thank Bobby Kaplan and especially Anna Ragni for editorial and bibliographic assistance with this paper. NR 373 TC 0 Z9 0 U1 17 U2 41 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0002-9483 EI 1096-8644 J9 AM J PHYS ANTHROPOL JI Am. J. Phys. Anthropol. PD JAN PY 2016 VL 159 SU 61 BP 232 EP 274 DI 10.1002/ajpa.22910 PG 43 WC Anthropology; Evolutionary Biology SC Anthropology; Evolutionary Biology GA DF3PU UT WOS:000371257900012 ER PT J AU Jeong, U Kim, J Ahn, C Torres, O Liu, X Bhartia, PK Spurr, RJD Haffner, D Chance, K Holben, BN AF Jeong, U. Kim, J. Ahn, C. Torres, O. Liu, X. Bhartia, P. K. Spurr, R. J. D. Haffner, D. Chance, K. Holben, B. N. TI An optimal-estimation-based aerosol retrieval algorithm using OMI near-UV observations SO ATMOSPHERIC CHEMISTRY AND PHYSICS LA English DT Article ID OZONE-MONITORING INSTRUMENT; SKY RADIANCE MEASUREMENTS; OPTICAL-PROPERTIES; PARTICLE NONSPHERICITY; TROPOSPHERIC AEROSOLS; SPECTRAL REFLECTANCE; SATELLITE; AERONET; ABSORPTION; MODELS AB An optimal-estimation(OE)-based aerosol retrieval algorithm using the OMI (Ozone Monitoring Instrument) near-ultraviolet observation was developed in this study. The OE-based algorithm has the merit of providing useful estimates of errors simultaneously with the inversion products. Furthermore, instead of using the traditional look-up tables for inversion, it performs online radiative transfer calculations with the VLIDORT (linearized pseudo-spherical vector discrete ordinate radiative transfer code) to eliminate interpolation errors and improve stability. The measurements and inversion products of the Distributed Regional Aerosol Gridded Observation Network campaign in northeast Asia (DRAGON NE-Asia 2012) were used to validate the retrieved aerosol optical thickness (AOT) and single scattering albedo (SSA). The retrieved AOT and SSA at 388 nm have a correlation with the Aerosol Robotic Network (AERONET) products that is comparable to or better than the correlation with the operational product during the campaign. The OE-based estimated error represented the variance of actual biases of AOT at 388 nm between the retrieval and AERONET measurements better than the operational error estimates. The forward model parameter errors were analyzed separately for both AOT and SSA retrievals. The surface reflectance at 388 nm, the imaginary part of the refractive index at 354 nm, and the number fine-mode fraction (FMF) were found to be the most important parameters affecting the retrieval accuracy of AOT, while FMF was the most important parameter for the SSA retrieval. The additional information provided with the retrievals, including the estimated error and degrees of freedom, is expected to be valuable for relevant studies. Detailed advantages of using the OE method were described and discussed in this paper. C1 [Jeong, U.; Kim, J.] Yonsei Univ, Dept Atmospher Sci, Seoul 120749, South Korea. [Ahn, C.] Sci Syst & Applicat Inc, Lanham, MD USA. [Torres, O.; Bhartia, P. K.; Haffner, D.; Holben, B. N.] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA. [Liu, X.; Chance, K.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Spurr, R. J. D.] RT Solut Inc, 9 Channing St, Cambridge, MA USA. RP Kim, J (reprint author), Yonsei Univ, Dept Atmospher Sci, Seoul 120749, South Korea. EM jkim2@yonsei.ac.kr RI Liu, Xiong/P-7186-2014 OI Liu, Xiong/0000-0003-2939-574X FU GEMS program of the Ministry of Environment, Korea; Eco Innovation Program of KEITI [2012000160002] FX This research was supported by the GEMS program of the Ministry of Environment, Korea, and the Eco Innovation Program of KEITI (2012000160002). The authors also acknowledge the KNMI and NASA/GSFC for providing OMI and AERONET data, respectively. Authors also acknowledge all the P. I.s and staff for the contribution to the DRAGON-NE Asia campaign. NR 59 TC 2 Z9 2 U1 0 U2 1 PU COPERNICUS GESELLSCHAFT MBH PI GOTTINGEN PA BAHNHOFSALLEE 1E, GOTTINGEN, 37081, GERMANY SN 1680-7316 EI 1680-7324 J9 ATMOS CHEM PHYS JI Atmos. Chem. Phys. PY 2016 VL 16 IS 1 BP 177 EP 193 DI 10.5194/acp-16-177-2016 PG 17 WC Meteorology & Atmospheric Sciences SC Meteorology & Atmospheric Sciences GA DF3YG UT WOS:000371283900012 ER PT J AU Jimenez, H Dumas, P Mouillot, D Bigot, L Ferraris, J AF Jimenez, Haizea Dumas, Pascal Mouillot, David Bigot, Lionel Ferraris, Jocelyne TI Harvesting effects on functional structure and composition of tropical invertebrate assemblages SO ICES JOURNAL OF MARINE SCIENCE LA English DT Article DE BTA; marine protected areas; shellfishing; species composition; tropical benthos ID CORAL-REEF ECOSYSTEMS; UPPER RHONE RIVER; COMMUNITY STRUCTURE; BIOLOGICAL TRAITS; SPECIES TRAITS; COASTAL ECOSYSTEMS; BENTHIC MACROINVERTEBRATES; HUMAN EXPLOITATION; PROTECTED AREAS; MARINE BENTHOS AB Anthropogenic disturbances affect ecosystem structure and functioning. The quantification of their impacts on highly diverse and structurally complex ecosystems, such as coral reefs, is challenging. These communities are facing rising fishing pressure, particularly on Pacific Islands such as New Caledonia. The main objective was to quantify harvesting effects on invertebrate assemblages across two contrasting habitats (soft-and hard-bottom), by comparing communities in marine protected areas (MPAs) with non-MPAs using 10 biological and ecological traits. Patterns of trait composition were compared with those of species composition by non-metric multidimensional scaling and permutational analysis of variance analyses. Traits most responsible for differences between MPAs and non-MPAs were determined using SIMPER analysis, and predictions on shellfishing effects were discussed. A total of 248 species were recorded in hard-bottom communities, mainly characterized by mobile epifauna living on corals, crawling, and possessing a shell (molluscs) or a cuticle (crabs and echinoderms). Soft-bottom habitats contained 166 species, dominated by burrowing and sedentary species, especially shelled (largely bivalves) and worm-like organisms. Clear differences in species and trait composition between MPA and non-MPAs were highlighted in both habitats. Harvesting activities have community-wide effects that change the functional composition of invertebrate assemblages, in particular in terms of living habits and mobility. The observed shifts in benthic communities can affect the functioning of tropical coastal ecosystems and need to be included in small-scale fisheries management in poorly known tropical environments. C1 [Jimenez, Haizea; Dumas, Pascal] IRD, UMR ENTROPIE, Lab Excellence LabEx CORAIL, 101 Promenade Roger Laroque,BP A5, Noumea 98848, New Caledonia. [Jimenez, Haizea] Smithsonian Environm Res Ctr, 3150 Paradise Dr, Tiburon, CA 94920 USA. [Mouillot, David] Univ Montpellier, UMR IRD CNRS UM IFREMER 9190, MARBEC, F-34095 Montpellier, France. [Mouillot, David] James Cook Univ, Australian Res Council, Ctr Excellence Coral Reef Studies, Townsville, Qld 4811, Australia. [Bigot, Lionel] Univ La Reunion, UMR ENTROPIE, Lab Excellence LabEx CORAIL, Ave Rene Cassin,BP 7151, F-97715 St Denis, France. [Ferraris, Jocelyne] Univ Perpignan, IRD, UMR ENTROPIE, Lab Excellence LabEx CORAIL, Via Domitia,52 Ave Paul Alduy, F-66860 Perpignan 9, France. RP Jimenez, H (reprint author), IRD, UMR ENTROPIE, Lab Excellence LabEx CORAIL, 101 Promenade Roger Laroque,BP A5, Noumea 98848, New Caledonia.; Jimenez, H (reprint author), Smithsonian Environm Res Ctr, 3150 Paradise Dr, Tiburon, CA 94920 USA. EM haizea.jimenez@gmail.com OI Dumas, Pascal/0000-0001-7369-8989 FU CRISP program; PAMPA program; GAIUS program; Eusko Jaurlaritza/Gobierno Vasco FX This research was supported by the CRISP, PAMPA, and GAIUS programmes and by a PhD grant from Eusko Jaurlaritza/Gobierno Vasco. NR 75 TC 1 Z9 1 U1 4 U2 18 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 1054-3139 EI 1095-9289 J9 ICES J MAR SCI JI ICES J. Mar. Sci. PD JAN-FEB PY 2016 VL 73 IS 2 BP 420 EP 428 DI 10.1093/icesjms/fsv179 PG 9 WC Fisheries; Marine & Freshwater Biology; Oceanography SC Fisheries; Marine & Freshwater Biology; Oceanography GA DF2AN UT WOS:000371141600023 ER PT J AU Didham, RK Leather, SR Basset, Y AF Didham, Raphael K. Leather, Simon R. Basset, Yves TI Circle the bandwagons - challenges mount against the theoretical foundations of applied functional trait and ecosystem service research SO INSECT CONSERVATION AND DIVERSITY LA English DT Editorial Material ID COMMUNITY ECOLOGY; CONSERVATION; INSECTS; SCIENCE; SCALE C1 [Didham, Raphael K.] Univ Western Australia, Sch Anim Biol, Crawley, WA, Australia. [Didham, Raphael K.] Ctr Environm & Life Sci, CSIRO Land & Water, Floreat, WA, Australia. [Leather, Simon R.] Harper Adams Univ, Dept Crop & Environm Sci, Newport, Shrops, England. [Basset, Yves] Smithsonian Trop Res Inst, Panama City, Panama. RP Didham, RK (reprint author), Univ Western Australia, Sch Anim Biol, Crawley, WA, Australia.; Didham, RK (reprint author), Ctr Environm & Life Sci, CSIRO Land & Water, Floreat, WA, Australia. RI Basset, Yves/B-6642-2014; Didham, Raphael/B-5953-2011 NR 25 TC 1 Z9 1 U1 0 U2 9 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1752-458X EI 1752-4598 J9 INSECT CONSERV DIVER JI Insect. Conserv. Divers. PD JAN PY 2016 VL 9 IS 1 BP 1 EP 3 DI 10.1111/icad.12150 PG 3 WC Biodiversity Conservation; Entomology SC Biodiversity & Conservation; Entomology GA DF3DB UT WOS:000371222800001 ER PT J AU Luhring, TM Connette, GM Schalk, CM AF Luhring, Thomas M. Connette, Grant M. Schalk, Christopher M. TI Trap characteristics and species morphology explain size-biased sampling of two salamander species SO AMPHIBIA-REPTILIA LA English DT Article DE Amphiuma means; body size; detection probability; inventory; passive trapping; population monitoring; sampling bias; Siren lacertina ID SIREN SIREN-LACERTINA; AMPHIUMA-MEANS; FUNNEL TRAPS; BODY-SIZE; GREATER SIREN; AQUATIC SALAMANDERS; CAPTURE RATES; BIRD COUNTS; DIMORPHISM; EFFICIENCY AB Demographic studies often depend on sampling techniques providing representative samples from populations. However, the sequence of events leading up to a successful capture or detection is susceptible to biases introduced through individual-level behaviour or physiology. Passive sampling techniques may be especially prone to sampling bias caused by size-related phenomena (e.g., physical limitations on trap entrance). We tested for size-biased sampling among five types of passive traps using a 9-year data set for two species of aquatic salamanders that have a 20 and 61 fold change in length over their ontogeny (Amphiuma means, Siren lacertina). Size-biased trapping was evident for both species, with body size distributions (body length mean and SD) of captured individuals differing among sampling techniques. Because our two species differed in girth at similar lengths, we were able to show that size biases (in length) were most likely caused by girth limitations on trap entry rates, and potentially by differences in retention rates. Accounting for the biases of sampling techniques may be critical when assessing current population status and demographic change. C1 [Luhring, Thomas M.; Schalk, Christopher M.] Univ Georgia, Savannah River Ecol Lab, Aiken, SC 29802 USA. [Luhring, Thomas M.] Univ Nebraska, Biol Sci, 410 Manter Hall, Lincoln, NE 68588 USA. [Connette, Grant M.] Natl Zool Pk, Smithsonian Conservat Biol Inst, Conservat Ecol Ctr, 1500 Remount Rd, Front Royal, VA 22630 USA. [Schalk, Christopher M.] Texas A&M Univ, Biodivers Res & Teaching Collect, Dept Wildlife & Fisheries Sci, 210 Nagle Hall, College Stn, TX 77843 USA. RP Luhring, TM (reprint author), Univ Georgia, Savannah River Ecol Lab, Aiken, SC 29802 USA.; Luhring, TM (reprint author), Univ Nebraska, Biol Sci, 410 Manter Hall, Lincoln, NE 68588 USA. EM tomluhring@gmail.com FU National Science Foundation [DBI-0453493]; American Museum of Natural History's Theodore Roosevelt Memorial Fund; University of Missouri; Savannah River Ecology Laboratory [DE-FC09-96SR18-546] FX We thank all of the people that have helped with sampling efforts at Dry Bay over the past 9 years. Special thanks are due to K. Buhlmann, B. Crawford, J. Greene, B. Morris, P. Nicodemo, S. Poppy, L. Smith, and J.W. Gibbons for their help and support with these efforts. Animals were collected under South Carolina Department of Natural Resources Scientific Collection permit G-08-07, and procedures used were approved by the University of Georgia (AUP approval #2006-10069). We thank R. McLaughlin for his helpful review of the article. This work was supported by the National Science Foundation (DBI-0453493), the American Museum of Natural History's Theodore Roosevelt Memorial Fund (awarded to TML), The University of Missouri's Life Sciences Fellowship and TWA Fellowship (awarded to TML), the Savannah River Ecology Laboratory under Financial Assistance Award DE-FC09-96SR18-546 between the University of Georgia and the US Department of Energy. We also thank K. O'Donnell for helpful suggestions for the conceptual model. NR 51 TC 0 Z9 0 U1 1 U2 2 PU BRILL ACADEMIC PUBLISHERS PI LEIDEN PA PLANTIJNSTRAAT 2, P O BOX 9000, 2300 PA LEIDEN, NETHERLANDS SN 0173-5373 EI 1568-5381 J9 AMPHIBIA-REPTILIA JI Amphib. Reptil. PY 2016 VL 37 IS 1 BP 79 EP 89 DI 10.1163/15685381-00003034 PG 11 WC Zoology SC Zoology GA DE9JT UT WOS:000370953600008 ER PT S AU Costa, DP Schwarz, L Robinson, P Schick, RS Morris, PA Condit, R Crocker, DE Kilpatrick, AM AF Costa, Daniel P. Schwarz, Lisa Robinson, Patrick Schick, Robert S. Morris, Patricia A. Condit, Richard Crocker, Daniel E. Kilpatrick, A. Marm BE Popper, AN Hawkins, A TI A Bioenergetics Approach to Understanding the Population Consequences of Disturbance: Elephant Seals as a Model System SO EFFECTS OF NOISE ON AQUATIC LIFE II SE Advances in Experimental Medicine and Biology LA English DT Article; Proceedings Paper CT 3rd International Conference on the Effects of Noise on Aquatic Life CY AUG, 2013 CL Budapest, HUNGARY SP Fisheries Joint Management Comm, Natl Oceanog & Atmospher Adm, Natl Sci Fdn, NAVFAC, Off Naval Res, Off Naval Res Global, Acoust Soc Amer, Aquat Noise Trust, Discovery Sound Sea, Co Biologists, Univ Maryland, Coll Chem & Life Sci, Ctr Comparat & Evolutionary Biol Hearing DE Population consequences of acoustic disturbance; Acoustic disturbance; Behavior; Sea lion; Demography ID BEHAVIOR AB Using long-term empirical data, we developed a complete population consequences of acoustic disturbance (PCAD) model and application for northern elephant seals. We assumed that the animals would not successfully forage while in a 100-km-diameter disturbance region within their foraging and transit paths. The decrease in lipid gain due to exposure was then translated to changes in birth rate and pup survival. Given their large foraging range, elephant seals were resilient to such a disturbance, showing no population-level effects. However, similar track analysis showed that given their more coastal nature, California sea lions were within a 25-km-diameter region of disturbance more often. C1 [Costa, Daniel P.; Schwarz, Lisa; Robinson, Patrick; Morris, Patricia A.; Kilpatrick, A. Marm] Univ Calif Santa Cruz, Dept Ecol & Evolutionary Biol, Santa Cruz, CA 95060 USA. [Schick, Robert S.] Univ St Andrews, Ctr Res Ecol & Environm Modelling, St Andrews KY16 9LZ, Fife, Scotland. [Condit, Richard] Smithsonian Trop Res Inst, Ctr Trop Forest Sci, Panama Unit 0948, APO, AA 34002 USA. [Crocker, Daniel E.] Sonoma State Univ, Dept Biol, Rohnert Pk, CA 94928 USA. RP Costa, DP (reprint author), Univ Calif Santa Cruz, Dept Ecol & Evolutionary Biol, Santa Cruz, CA 95060 USA. EM costa@ucsc.edu; schwarz@biology.ucsc.edu; robinson@biology.ucsc.edu; rss5@st-andrews.ac.uk; pamorris@ucsc.edu; conditr@gmail.com; crocker@sonoma.edu; akilpatr@ucsc.edu FU Office of Naval Research [N00014-08-1-1195]; Exploration and Production (E&P) Sound and Marine Life Joint Industry Programme of the International Association of Oil and Gas Producers; ExxonMobil company; Shell oil company; Ida Benson Lynn Chair in Ocean Health FX This paper was developed in association with the Office of Naval Research-supported population consequences of acoustic disturbance/population consequences of disturbance (PCAD/PCOD) committee and was supported by Office of Naval Research Grant N00014-08-1-1195, the Exploration and Production (E&P) Sound and Marine Life Joint Industry Programme of the International Association of Oil and Gas Producers, ExxonMobil and Shell oil companies, and the Ida Benson Lynn Chair in Ocean Health. We also acknowledge the University of California Natural Reserve System and the rangers of Ano Nuevo Reserve. NR 15 TC 1 Z9 1 U1 2 U2 8 PU SPRINGER-VERLAG BERLIN PI BERLIN PA HEIDELBERGER PLATZ 3, D-14197 BERLIN, GERMANY SN 0065-2598 BN 978-1-4939-2981-8; 978-1-4939-2980-1 J9 ADV EXP MED BIOL JI Adv.Exp.Med.Biol. PY 2016 VL 875 BP 161 EP 169 DI 10.1007/978-1-4939-2981-8_19 PG 9 WC Environmental Sciences; Marine & Freshwater Biology SC Environmental Sciences & Ecology; Marine & Freshwater Biology GA BE2TA UT WOS:000370000900020 PM 26610956 ER PT S AU Ketten, DR Arruda, J Cramer, S Yamato, M AF Ketten, D. R. Arruda, J. Cramer, S. Yamato, M. BE Popper, AN Hawkins, A TI Great Ears: Low-Frequency Sensitivity Correlates in Land and Marine Leviathans SO EFFECTS OF NOISE ON AQUATIC LIFE II SE Advances in Experimental Medicine and Biology LA English DT Article; Proceedings Paper CT 3rd International Conference on the Effects of Noise on Aquatic Life CY AUG, 2013 CL Budapest, HUNGARY SP Fisheries Joint Management Comm, Natl Oceanog & Atmospher Adm, Natl Sci Fdn, NAVFAC, Off Naval Res, Off Naval Res Global, Acoust Soc Amer, Aquat Noise Trust, Discovery Sound Sea, Co Biologists, Univ Maryland, Coll Chem & Life Sci, Ctr Comparat & Evolutionary Biol Hearing DE Low frequency; Hearing; Whales; Impacts ID COCHLEA; COILING; LENGTH; CALLS AB Like elephants, baleen whales produce low-frequency (LF) and even infrasonic (IF) signals, suggesting they may be particularly susceptible to underwater anthropogenic sound impacts. Analyses of computerized tomography scans and histologies of the ears in five baleen whale and two elephant species revealed that LF thresholds correlate with basilar membrane thickness/width and cochlear radii ratios. These factors are consistent with high-mass, low-stiffness membranes and broad spiral curvatures, suggesting that Mysticeti and Proboscidea evolved common inner ear adaptations over similar time scales for processing IF/LF sounds despite operating in different media. C1 [Ketten, D. R.; Arruda, J.; Cramer, S.] Woods Hole Oceanog Inst, Dept Biol, Woods Hole, MA 02543 USA. [Ketten, D. R.] Harvard Univ, Sch Med, Boston, MA 02114 USA. [Ketten, D. R.] Curtin Univ, Perth, WA 6845, Australia. [Arruda, J.] Massachusetts Eye & Ear Infirm, Boston, MA 02114 USA. [Yamato, M.] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20004 USA. RP Ketten, DR (reprint author), Woods Hole Oceanog Inst, Dept Biol, Woods Hole, MA 02543 USA.; Ketten, DR (reprint author), Harvard Univ, Sch Med, Boston, MA 02114 USA.; Ketten, DR (reprint author), Curtin Univ, Perth, WA 6845, Australia. EM dketten@whoi.edu; jarruda@whoi.edu; scramer@whoi.edu; YamatoM@si.edu FU Office of Naval Research; National Institutes of Health (NIH); International Association of Oil and Gas Producers (OGP) Joint Industry Programme; National Institute of Deafness and Communication Disorders (NIDCD), NIH FX This work was supported by the Office of Naval Research, the National Institutes of Health (NIH), the International Association of Oil and Gas Producers (OGP) Joint Industry Programme, and the National Institute of Deafness and Communication Disorders (NIDCD), NIH. We are grateful to Jennifer O'Malley, Barbara Burgess, and Diane DeLeo Jones for assistance with the histology and to Clarinda Northrup, the Cape Cod Stranding Network, and the International Fund for Animal Welfare (IFAW) for providing specimens. Above all, we acknowledge the mentorship and inspiration of our colleague Hezy Shoshani, who was a giant among his beloved leviathans and colleagues. He died in defense of his life's work and is sorely missed. NR 16 TC 1 Z9 1 U1 7 U2 10 PU SPRINGER-VERLAG BERLIN PI BERLIN PA HEIDELBERGER PLATZ 3, D-14197 BERLIN, GERMANY SN 0065-2598 BN 978-1-4939-2981-8; 978-1-4939-2980-1 J9 ADV EXP MED BIOL JI Adv.Exp.Med.Biol. PY 2016 VL 875 BP 529 EP 538 DI 10.1007/978-1-4939-2981-8_64 PG 10 WC Environmental Sciences; Marine & Freshwater Biology SC Environmental Sciences & Ecology; Marine & Freshwater Biology GA BE2TA UT WOS:000370000900065 PM 26611001 ER PT J AU He, ZH Kays, R Zhang, Z Ning, GH Huang, C Han, TX Millspaugh, J Forrester, T McShea, W AF He, Zhihai Kays, Roland Zhang, Zhi Ning, Guanghan Huang, Chen Han, Tony X. Millspaugh, Josh Forrester, Tavis McShea, William TI Visual Informatics Tools for Supporting Large-Scale Collaborative Wildlife Monitoring with Citizen Scientists SO IEEE CIRCUITS AND SYSTEMS MAGAZINE LA English DT Article ID SENSOR NETWORKS; VIDEO; TRACKING; SYSTEM; CRITTERCAM; BEHAVIOR; DESIGN; MODELS; DEER AB Collaborative wildlife monitoring and tracking at large scales will help us understand the complex dynamics of wildlife systems, evaluate the impact of human actions and environmental changes on wildlife species, and answer many important ecological and evolutionary research questions. To support collaborative wildlife monitoring and research, we need to develop integrated camera-sensor networking systems, deploy them at large scales, and develop advanced computational and informatics tools to analyze and manage the massive wildlife monitoring data. In this paper, we will cover various aspects of the design of such systems, including (1) long-lived integrated camera-sensor system design, (2) image processing and computer vision algorithms for animal detection, segmentation, tracking, species classification, and biometric feature extraction, (3) cloud-based data management, (4) crowd-sourcing based image annotation with citizen scientists, and (5) applications to wildlife and ecological research. C1 [He, Zhihai] Univ Missouri, Dept Elect & Comp Engn, Columbia, MO 65211 USA. [Kays, Roland] N Carolina State Univ, Raleigh, NC 27695 USA. [Kays, Roland] NC Museum Nat Sci, Biodivers Lab, Raleigh, NC USA. [Zhang, Zhi; Ning, Guanghan; Huang, Chen] Univ Missouri, Columbia, MO 65211 USA. [Han, Tony X.] Univ Missouri, Elect & Comp Engn, Columbia, MO 65211 USA. [Millspaugh, Josh] Univ Missouri, Sch Nat Resources, Wildlife Management, Columbia, MO 65211 USA. [Millspaugh, Josh] Univ Missouri, Sch Nat Resources, Columbia, MO 65211 USA. [Forrester, Tavis; McShea, William] Smithsonian Inst, Washington, DC 20560 USA. RP He, ZH (reprint author), Univ Missouri, Dept Elect & Comp Engn, Columbia, MO 65211 USA. NR 51 TC 1 Z9 1 U1 4 U2 6 PU IEEE-INST ELECTRICAL ELECTRONICS ENGINEERS INC PI PISCATAWAY PA 445 HOES LANE, PISCATAWAY, NJ 08855-4141 USA SN 1531-636X EI 1558-0830 J9 IEEE CIRC SYST MAG JI IEEE Circuits Syst. Mag. PY 2016 VL 16 IS 1 BP 73 EP 86 DI 10.1109/MCAS.2015.2510200 PG 14 WC Engineering, Electrical & Electronic SC Engineering GA DE9CS UT WOS:000370933600006 ER PT J AU Gary, SP Jian, LK Broiles, TW Stevens, ML Podesta, JJ Kasper, JC AF Gary, S. Peter Jian, Lan K. Broiles, Thomas W. Stevens, Michael L. Podesta, John J. Kasper, Justin C. TI Ion-driven instabilities in the solar wind: Wind observations of 19 March 2005 SO JOURNAL OF GEOPHYSICAL RESEARCH-SPACE PHYSICS LA English DT Article DE solar wind; instabilities ID PROTON TEMPERATURE ANISOTROPY; ELECTROMAGNETIC INSTABILITIES; MAGNETOSONIC INSTABILITY; CYCLOTRON WAVES; PLASMA; BEAM; CONSTRAINT; SPACECRAFT; STABILITY; STREAMS AB Intervals of enhanced magnetic fluctuations have been frequently observed in the solar wind. But it remains an open question as to whether these waves are generated at the Sun and then transported outward by the solar wind or generated locally in the interplanetary medium. Magnetic field and plasma measurements from the Wind spacecraft under slow solar wind conditions on 19 March 2005 demonstrate seven events of enhanced magnetic fluctuations at spacecraft-frame frequencies somewhat above the proton cyclotron frequency and propagation approximately parallel or antiparallel to the background magnetic field B-o. The proton velocity distributions during these events are characterized by two components: a more dense, slower core and a less dense, faster beam. Observed plasma parameters are used in a kinetic linear dispersion equation analysis for electromagnetic fluctuations at k x B-o=0; for two events the most unstable mode is the Alfven-cyclotron instability driven by a proton component temperature anisotropy T/T-||>1 (where the subscripts denote directions relative to B-o), and for three events the most unstable mode is the right-hand polarized magnetosonic instability driven primarily by ion component relative flows. Thus, both types of ion anisotropies and both types of instabilities are likely to be local sources of these enhanced fluctuation events in the solar wind. C1 [Gary, S. Peter; Podesta, John J.] Space Sci Inst, Boulder, CO USA. [Jian, Lan K.] Univ Maryland, Goddard Planetary Heliophys Inst, College Pk, MD 20742 USA. [Jian, Lan K.] NASA, Goddard Space Flight Ctr, Greenbelt, MD USA. [Broiles, Thomas W.] Southwest Res Inst, San Antonio, TX USA. [Stevens, Michael L.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Kasper, Justin C.] Univ Michigan, Dept Atmospher Ocean & Space Sci, Ann Arbor, MI 48109 USA. RP Gary, SP (reprint author), Space Sci Inst, Boulder, CO USA. EM pgary@lanl.gov RI Jian, Lan/B-4053-2010; OI Jian, Lan/0000-0002-6849-5527; Broiles, Thomas/0000-0001-6910-2724 FU NASA [NNX15AB75G, NNX13AI65G] FX The research efforts of S.P.G., L.K.J., and T.W.B. were supported by the NASA Living with a Star project NNX15AB75G entitled "Understanding Wave-Particle Interactions between Solar Wind Plasma Waves and Heavy Ions." L.K.J.'s work was also supported by NASA award NNX13AI65G. The observational data for magnetic fields used herein are available at NASA National Space Science Data Center (NSSDC). The observations of plasma parameters are available from Michael Stevens, and the dispersion relations computed from linear theory are available from S. Peter Gary. NR 40 TC 7 Z9 7 U1 2 U2 2 PU AMER GEOPHYSICAL UNION PI WASHINGTON PA 2000 FLORIDA AVE NW, WASHINGTON, DC 20009 USA SN 2169-9380 EI 2169-9402 J9 J GEOPHYS RES-SPACE JI J. Geophys. Res-Space Phys. PD JAN PY 2016 VL 121 IS 1 BP 30 EP 41 DI 10.1002/2015JA021935 PG 12 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DF2CJ UT WOS:000371146900003 PM 27818854 ER PT S AU Tonitto, C Gurwick, NP Woodbury, PB AF Tonitto, Christina Gurwick, Noel P. Woodbury, Peter B. BE DelGrosso, SJ Ahuja, LR Parton, WJ TI Quantifying Greenhouse Gas Emissions from Agricultural and Forest Landscapes for Policy Development and Verification SO SYNTHESIS AND MODELING OF GREENHOUSE GAS EMISSIONS AND CARBON STORAGE IN AGRICULTURAL AND FOREST SYSTEMS TO GUIDE MITIGATION AND ADAPTATION SE Advances in Agricultural Systems Modeling-Transdisciplinary Research Synthesis and Applications LA English DT Article; Book Chapter ID SOIL ORGANIC-MATTER; NITROUS-OXIDE EMISSIONS; CENTRAL GREAT-PLAINS; MATHEMATICAL-MODEL ECOSYS; MISSISSIPPI RIVER-BASIN; CO2 ENRICHMENT FACE; ROW-CROP FIELD; DRAINED ILLINOIS AGROECOSYSTEMS; TERRESTRIAL CARBON STORAGE; HARVESTED WOOD PRODUCTS AB The emergence of policies to reduce greenhouse gas (GHG) emissions motivated a rapid shift in ecosystem modeling, especially concerning agricultural and forest management effects on nitrous oxide (N2O) emissions and soil carbon (C). First, we review models for estimating GHG fluxes in agricultural and forest landscapes. Second, we investigate the interplay of models with institutions that develop and implement climate change policy. Limited GHG flux observations constrain our understanding of process controls, especially with respect to N2O flux. Even when simulation models explicitly include N2O flux, this capability is infrequently applied or validated. In the policy arena, tools used to estimate aboveground forest biomass C rely on robust inventory data. Such data are scarce outside of the industrialized world. Compared with biomass C, soil C storage in both forest and agricultural systems is difficult to quantify. Widely used estimates depend on critical assumptions such as the extent to which erosion contributes to C loss from fields and the mechanisms by which C is stabilized in soil, both of which are the subject of serious debate. As evidenced by at least one instance we explore, institutions dedicated to policy development and implementation can rapidly achieve a nuanced understanding of these limitations, given sufficient engagement of the research community. Our review illuminates challenges that affect land-based GHG mitigation initiatives as a result of current knowledge gaps, institutional capacity, and decision-making frameworks. We suggest key points that should be communicated to model users and raise questions that could be fruitfully addressed by model developers and consumers of modeled estimates. C1 [Tonitto, Christina] Cornell Univ, Cornell Int Inst Food Agr & Dev, Mann Lib B75, Ithaca, NY 14853 USA. [Gurwick, Noel P.] Smithsonian Environm Res Ctr, 647 Contees Wharf Rd, Edgewater, MD 21037 USA. [Woodbury, Peter B.] Cornell Univ, Sect Soil & Crop Sci, Sch Integrat Plant Sci, 1017 Bradfield Hall,306 Tower Rd, Ithaca, NY 14853 USA. RP Tonitto, C (reprint author), Cornell Univ, Cornell Int Inst Food Agr & Dev, Mann Lib B75, Ithaca, NY 14853 USA. EM ctonitto@cornell.edu; noel.gurwick@gmail.com; peterwoodbury@cornell.edu NR 356 TC 2 Z9 2 U1 2 U2 9 PU AMER SOC AGRONOMY PI MADISON PA 677 SOUTH SEGOE RD, MADISON, WI 53711 USA SN 2163-2774 BN 978-0-89118-346-4; 978-0-89118-345-7 J9 ADV AGR SYST MODEL PY 2016 VL 6 BP 229 EP 304 DI 10.2134/advagricsystmodel6.2013.0007 D2 10.2134/advagricsystmodel6 PG 76 WC Agronomy; Environmental Sciences; Forestry SC Agriculture; Environmental Sciences & Ecology; Forestry GA BE3JL UT WOS:000370803600012 ER PT J AU Post, JE Thomas, E Heaney, PJ AF Post, Jeffrey E. Thomas, Ellen Heaney, Peter J. TI Jianshuiite in oceanic manganese nodules at the Paleocene-Eocene boundary SO AMERICAN MINERALOGIST LA English DT Article DE Jianshuiite; birnessite; paleocene-eocene thermal maximum (PETM); X-ray diffraction ID X-RAY-DIFFRACTION; THERMAL MAXIMUM; FERROMANGANESE NODULES; CRYSTAL-STRUCTURE; CS-EXCHANGE; DEEP-SEA; CHALCOPHANITE; SEDIMENTS; BIRNESSITE; MECHANISMS AB Synchrotron powder X-ray diffraction and scanning electron microscopy examinations of manganese oxide concretions/nodules (similar to 0.3-1.0 mm diameter) from ODP Site 1262 on Walvis Ridge in the Southeastern Atlantic Ocean revealed that they consist primarily of the layered Mn oxide phase jianshuiite [(Mg,Mn,Ca)Mn(3+)07 center dot 3H(2)O]. The nodules are from an interval with severe carbonate dissolution that represents the Paleocene/Eocene (P/E) thermal maximum (-55.8 Ma). Most nodules from the middle of the carbonate dissolution interval contain internal open space, and consist almost entirely of euhedral plate -like jianshuiite crystals, 2-4 pm in diameter and similar to 0.1-0.5 pm thick. Backscattered electron images and energy -dispersive X-ray analyses revealed stacks of interleaved Al -rich and Al poor jianshuiite crystals in some nodules. The crystals in other nodules contain predominantly Mg (with trace K and Al) in addition to Mn and 0, making them near "end -member" jianshuiite. Rietveld refinements in space group R3 confirmed the isostructural relationship between jianshuiite and chalcophanite, with Mg occupying the interlayer position above and below the vacant sites in the Mn/O octahedral sheet, and coordinated to 3 octahedral layer O atoms (1.94 angstrom) and 3 interlayer water 0 atoms (2.13 angstrom). Final refined occupancy factors suggest that small quantities of Ni and possibly Mn2+ are located on the Mg site. The transient appearance of the Mg -rich birnessite-like phase jianshuiite, probably abiotically produced, must indicate an exceptional transient change in the chemistry of the pore fluids within deep ocean sediments directly following the P/E boundary, possibly as a result of decreasing oxygen levels and pH, followed by a return to pre -event conditions. C1 [Post, Jeffrey E.] Smithsonian Inst, Dept Mineral Sci, POB 37012, Washington, DC 20013 USA. [Thomas, Ellen] Yale Univ, Dept Geol & Geophys, POB 208109, New Haven, CT 06520 USA. [Thomas, Ellen] Wesleyan Univ, Dept Earth & Environm Sci, 265 Church St, Middletown, CT 06459 USA. [Heaney, Peter J.] Penn State Univ, Dept Geosci, University Pk, PA 16802 USA. RP Post, JE (reprint author), Smithsonian Inst, Dept Mineral Sci, POB 37012, Washington, DC 20013 USA. EM postj@si.edu FU NSF [EAR07-45374, EAR11-47728, OCE 1232413]; U.S. Department of Energy, Division of Materials Sciences and Division of Chemical Sciences [DE-AC02-98CH10886] FX Funding for this research was provided by NSF grants EAR07-45374 and EAR11-47728 to Heaney and Post, and NSF grant OCE 1232413 to Thomas. Thanks go to Peter Eng and Joanne Stubbs at APS beamline 13-BM-C for their assistance with the X-ray diffraction experiment, to Joop Varekamp at Wesleyan University for first noticing the crystalline Mn oxides using the electron microscope facilities at the University of Oregon (Eugene, Oregon), and to Isabella Raffi at the Universita degli Studi G_dAnnunzio, Chieti e Pescara (Italy) for identification of calcareous nannofossils. This research was carried out at the Advanced Photon Source, Argonne National Laboratory, which is supported by the U.S. Department of Energy, Division of Materials Sciences and Division of Chemical Sciences, under Contract No. DE-AC02-98CH10886. Samples were provided by the International Ocean Discovery Program. NR 45 TC 3 Z9 3 U1 2 U2 9 PU MINERALOGICAL SOC AMER PI CHANTILLY PA 3635 CONCORDE PKWY STE 500, CHANTILLY, VA 20151-1125 USA SN 0003-004X EI 1945-3027 J9 AM MINERAL JI Am. Miner. PD JAN-FEB PY 2016 VL 101 IS 1-2 BP 407 EP 414 DI 10.2138/am-2016-5347 PG 8 WC Geochemistry & Geophysics; Mineralogy SC Geochemistry & Geophysics; Mineralogy GA DD8YT UT WOS:000370213500038 ER PT J AU de Barros, S Vanzella, E Amorin, R Castellano, M Siana, B Grazian, A Suh, H Balestra, I Vignali, C Verhamme, A Zamorani, G Mignoli, M Hasinger, G Comastri, A Pentericci, L Perez-Montero, E Fontana, A Giavalisco, M Gilli, R AF de Barros, S. Vanzella, E. Amorin, R. Castellano, M. Siana, B. Grazian, A. Suh, H. Balestra, I. Vignali, C. Verhamme, A. Zamorani, G. Mignoli, M. Hasinger, G. Comastri, A. Pentericci, L. Perez-Montero, E. Fontana, A. Giavalisco, M. Gilli, R. TI An extreme [O III] emitter at z=3.2: a low metallicity Lyman continuum source SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE galaxies: high-redshift; galaxies: evolution; galaxies: ISM; galaxies: starburst ID STAR-FORMING GALAXIES; HUBBLE-SPACE-TELESCOPE; LY-ALPHA EMISSION; ACTIVE GALACTIC NUCLEI; HIGH-REDSHIFT GALAXIES; SIMILAR-TO 2-3; SPECTROSCOPIC PARALLEL SURVEY; EXTRAGALACTIC LEGACY SURVEY; FRAME ULTRAVIOLET-SPECTRA; SURVEY. SURVEY DESIGN AB Aims. Cosmic reionization is an important process occurring in the early epochs of the Universe. However, because of observational limitations due to the opacity of the intergalactic medium to Lyman continuum photons, the nature of ionizing sources is still not well constrained. While high-redshift star-forming galaxies are thought to he the main contributors to the ionizing background at z > 6, it is impossible to directly detect their ionizing emission. Therefore, looking at intermediate redshift analogues (z similar to 2-4) can provide useful hints about cosmic reionization. Methods. We investigate the physical properties of one of the best Lyman continuum emitter candidate at z = 3.212 found in the GOODS-S/CANDELS field with photometric coverage from the U to the MIPS 24 mu m band and VIMOS/VI:17 and.MOSEIRE/Keck spectroscopy. These observations allow us to derive physical properties such as stellar mass, star formation rate, age of the stellar population, dust attenuation, metallicity, and ionization parameter, and to determine how these parameters are related to the Lyman continuum emission. Results. Investigation of the UV spectrum confirms a direct spectroscopic detection of the Lyman continuum emission with S /N > 5. Non-zero Lya flux at the systemic redshift and high Lyman-alpha escape fraction (f(esc))LYa) >= 0.78) suggest a low H I column density. The weak C and Si low-ionization absorption lines are also consistent with a low covering fraction along the line of sight. The subsolar abundances are consistent with a young and extreme starbiu-st. The [O HI]lambda lambda 14959, 5007+H beta equivalent width (EW) is one of the largest reported for a galaxy at z > 3 (EW(O [III)lambda lambda 4959, 5007 + H beta) 1600 A. rest-frame; 6700 A observed-frame) and the near-infrared spectrum shows that this is mainly due to an extremely strong [O III] emission. The large observed [0 HMO Ill ratio (>10) and high ionization parameter are consistent with prediction from photoionization models in the case of a density-bounded nebula scenario. Furthermore, the EW([O III] lambda lambda 4959,5007+beta) is comparable to recent measurements reported at z 7-9, in the reionization epoch. We also investigate the possibility of an AGN contribution to explain the ionizing emission but most of the AGN identification diagnostics suggest that stellar emission dominates instead. Conclusions. This source is currently the first high -z example of a Lyman continuum emitter exhibiting indirect and direct evidences of a Lyman continuum leakage and having physical properties consistent with theoretical expectation from Lyman continuum emission from a density-hounded nebula. A low Ell column density, low covering fraction, compact star formation activity, and a possible interaction/merging of two systems may contribute to the Lyman continuum photon leakage. C1 [de Barros, S.; Vanzella, E.; Vignali, C.; Zamorani, G.; Mignoli, M.; Comastri, A.; Gilli, R.] Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy. [Amorin, R.; Castellano, M.; Grazian, A.; Pentericci, L.] Osserv Astron Roma, INAF, Via Frascati 33, I-00040 Monte Porzio Catone, Italy. [Siana, B.] Univ Calif Riverside, Dept Phys & Astron, Riverside, CA 92507 USA. [Suh, H.; Fontana, A.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Balestra, I.] Osserv Astron Trieste, INAF, Via GB Tiepolo 11, I-34131 Trieste, Italy. [Vignali, C.] Univ Bologna, Dipartimento Fis & Astron, Viale Berti Pichat 6-2, I-40127 Bologna, Italy. [Verhamme, A.] Univ Geneva, Observ Geneva, Ch Maillettes 51, CH-1290 Versoix, Switzerland. [Hasinger, G.] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA. [Perez-Montero, E.] CSIC, Inst Astrofis Andalucia, Apartado Correos 3004, E-18080 Granada, Spain. [Giavalisco, M.] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA. RP de Barros, S (reprint author), Osservatorio Astron Bologna, INAF, Via Ranzani 1, I-40127 Bologna, Italy. EM stephane.debarros@oabo.inaf.it OI Amorin, Ricardo O./0000-0001-5758-1000; Zamorani, Giovanni/0000-0002-2318-301X; Perez Montero, E/0000-0003-3985-4882 FU PRIN-INAF FX We thank the referee for suggestions that clarify the text and the analysis. We thank M. Tosi, F. Annibali, M. Brusa and H. Atek for useful discussions. We acknowledge the financial contribution from PRIN-INAF 2012. This work has made use of the Rainbow Cosmological Surveys Database, which is operated by the Universidad Complutense de Madrid (UCM), partnered with the University of California Observatories at Santa Cruz (UCO/Lick, UCSC). NR 136 TC 20 Z9 20 U1 2 U2 2 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A51 DI 10.1051/0004-6361/20157046 PG 13 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300058 ER PT J AU Diaz, RF Segransan, D Udry, S Lovis, C Pepe, F Dumusque, X Marmier, M Alonso, R Benz, W Bouchy, F Net, ACF Cameron, AC Deleuil, M Figueira, P Gillon, M Lo Curto, G Mayor, M Mordasini, C Motalebi, F Moutou, C Pollacco, D Pompei, E Queloz, D Santos, N Wyttenbach, A AF Diaz, R. F. Segransan, D. Udry, S. Lovis, C. Pepe, F. Dumusque, X. Marmier, M. Alonso, R. Benz, W. Bouchy, F. Net, A. Co Ffi Cameron, A. Collier Deleuil, M. Figueira, P. Gillon, M. Lo Curto, G. Mayor, M. Mordasini, C. Motalebi, F. Moutou, C. Pollacco, D. Pompei, E. Queloz, D. Santos, N. Wyttenbach, A. TI The HARPS search for southern extra-solar planets XXXVIII. Bayesian re-analysis of three systems. New super-Earths, unconfirmed signals, and magnetic cycles SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE techniques: radial velocities; methods: data analysis; methods: statistical; planetary systems ID CA-II H; MAIN-SEQUENCE STARS; M-CIRCLE-PLUS; RADIAL-VELOCITY; HABITABLE-ZONE; STELLAR ACTIVITY; CHROMOSPHERIC ACTIVITY; MARGINAL LIKELIHOOD; GIANT PLANET; MASS PLANETS AB We present the analysis of the entire HARPS observations of three stars that host planetary systems: HD1461, HD40307, and HD204313. The data set spans eight years and contains more than 200 nightly averaged velocity measurements for each star. This means that it is sensitive to both long-period and low-mass planets and also to the effects induced by stellar activity cycles. We modelled the data using Keplerian functions that correspond to planetary candidates and included the short-and long-term effects of magnetic activity. A Bayesian approach was taken both for the data modelling, which allowed us to include information from activity proxies such as log (R'(HK)) in the velocity modelling, and for the model selection, which permitted determining the number of significant signals in the system. The Bayesian model comparison overcomes the limitations inherent to the traditional periodogram analysis. We report an additional super-Earth planet in the HD1461 system. Four out of the six planets previously reported for HD40307 are confirmed and characterised. We discuss the remaining two proposed signals. In particular, we show that when the systematic uncertainty associated with the techniques for estimating model probabilities are taken into account, the current data are not conclusive concerning the existence of the habitable-zone candidate HD40307 g. We also fully characterise the Neptune-mass planet that orbits HD204313 in 34.9 days. C1 [Diaz, R. F.; Segransan, D.; Udry, S.; Lovis, C.; Pepe, F.; Dumusque, X.; Marmier, M.; Bouchy, F.; Net, A. Co Ffi; Mayor, M.; Motalebi, F.; Queloz, D.; Wyttenbach, A.] Univ Geneva, Observ Astron, 51 Ch Maillettes, CH-1290 Versoix, Switzerland. [Dumusque, X.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Alonso, R.] Inst Astrofis Canarias, Tenerife 38205, Spain. [Alonso, R.] Univ La Laguna, Dept Astrofis, E-38206 Tenerife, Spain. [Benz, W.; Mordasini, C.] Univ Bern, Inst Phys, Silderstr 5, CH-3012 Bern, Switzerland. [Bouchy, F.; Deleuil, M.; Moutou, C.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France. [Cameron, A. Collier] Univ St Andrews, Sch Phys & Astron, St Andrews KY16 9SS, Fife, Scotland. [Figueira, P.; Santos, N.] Univ Porto, CAUP, Inst Astrofis & Ciencias Espaco, Rua Estrelas, P-4150762 Oporto, Portugal. [Gillon, M.] Univ Liege, Inst Astrophys & Geophys, Allee 6 Aout 17,Bat B5C, B-4000 Liege, Belgium. [Lo Curto, G.; Pompei, E.] European So Observ, 3107 Alonso Cordova,Casilla 19001, Santiago 19, Chile. [Moutou, C.] Canada France Hawaii Telescope Corp, POB 1597, Kamuela, HI 96743 USA. [Pollacco, D.] Univ Warwick, Dept Phys, Coventry CV4 7AL, W Midlands, England. [Queloz, D.] Univ Cambridge, Cavendish Lab, JJ Thomson Ave, Cambridge CB3 0HE, England. [Santos, N.] Univ Porto, Fac Ciencias, Dept Fis & Astron, Rua Campo Alegre, P-4169007 Oporto, Portugal. RP Diaz, RF (reprint author), Univ Geneva, Observ Astron, 51 Ch Maillettes, CH-1290 Versoix, Switzerland. EM Rodrigo.Diaz@unige.ch RI Figueira, Pedro/J-4916-2013; Alonso, Roi/D-8799-2014; OI Figueira, Pedro/0000-0001-8504-283X; Alonso, Roi/0000-0001-8462-8126; Cameron, Andrew/0000-0002-8863-7828; Diaz, Rodrigo/0000-0001-9289-5160 FU Swiss National Science Foundation (SNSF); European Union [313014]; SNSF; Swiss National Science Foundation [BSSIO_155816]; Fundacao para a Ciencia e a Tecnologia (FCT) through Investigador FCT [IF/01037/2013, IF/00169/2012]; POPH/FSE (EC) by FEDER through the program "Programa Operacional de Factores de Competitividade - COMPETE"; Fundacao para a Ciencia e a Tecnologia (FCT) [IF/01037/2013CP1191/CT0001] FX We acknowledge Ewan Cameron (Oxford) for bringing the Perrakis et al. (2014) estimator to our attention and for his help in understanding the limitations of the TPM estimator. This work has been carried out within the frame of the National Centre for Competence in Research "PlanetS" supported by the Swiss National Science Foundation (SNSF). It made use of the Data Analyses Center for Exoplanets - http://dace.unige.ch - a platform of PlanetS. R.F.D. acknowledges funding from the European Union Seventh Framework Programme (FP7/2007-2013) under Grant agreement number 313014 (ETAEARTH). S.U., C.L., D.S., F.P., C.M. and A.W. acknowledge the financial support of the SNSF. CM acknowledges the support of the Swiss National Science Foundation under grant BSSIO_155816 "PlanetsInTime". We thank the University of Geneva for their continuous support to our planet search programmes. M. Gillon is Research Associate at the FNRS. P.F. and N.C.S. acknowledge support by Fundacao para a Ciencia e a Tecnologia (FCT) through Investigador FCT contracts of reference IF/01037/2013 and IF/00169/2012, respectively, and POPH/FSE (EC) by FEDER funding through the program "Programa Operacional de Factores de Competitividade - COMPETE". P.F. further acknowledges support from Fundacao para a Ciencia e a Tecnologia (FCT) in the form of an exploratory project of reference IF/01037/2013CP1191/CT0001. This research has made use of the SIMBAD database and of the VizieR catalogue access tool operated at CDS, France. NR 86 TC 11 Z9 11 U1 1 U2 1 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A134 DI 10.1051/0004-6361/201526729 PG 24 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300141 ER PT J AU Gusdorf, A Gusten, R Menten, KM Flower, DR des Forets, GP Codella, C Csengeri, T Gomez-Ruiz, AI Heyminck, S Jacobs, K Kristensen, LE Leurini, S Requena-Torres, MA Wampfler, SF Wiesemeyer, H Wyrowski, F AF Gusdorf, A. Guesten, R. Menten, K. M. Flower, D. R. des Forets, G. Pineau Codella, C. Csengeri, T. Gomez-Ruiz, A. I. Heyminck, S. Jacobs, K. Kristensen, L. E. Leurini, S. Requena-Torres, M. A. Wampfler, S. F. Wiesemeyer, H. Wyrowski, F. TI Challenging shock models with SOFIA OH observations in the high-mass star-forming region Cepheus A SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE astrochemistry; stars: formation; ISM: jets and outflows; ISM: kinematics and dynamics; infrared: ISM; ISM: individual objects: Cep A ID MOLECULAR OUTFLOW SOURCES; COLOGNE DATABASE; KEY PROGRAM; CLOUDS; HERSCHEL; WAVES; SPECTROSCOPY; EMISSION; WATER; SIO AB Context. OH is a key molecule in H2O chemistry, a valuable tool for probing physical conditions, and an important contributor to the cooling of shock regions around high-mass protostars. OH participates in the re -distribution of energy from the protostar towards the surrounding Interstellar Medium. Aims. Our aim is to assess the origin of the OH emission from the Cepheus A massive star-forming region and to constrain the physical conditions prevailing in the emitting gas. We thus want to probe the processes at work during the formation of massive stars. Methods. We present spectrally resolved observations of OH towards the protostellar outflows region of Cepheus A with the GREAT spectrometer onboard the Stratospheric Observatory for Infrared Astronomy (SOFIA) telescope. Three triplets were observed at 1834.7 GHz, 1837.8 GHz, and 2514.3 GHz (163.4 pm, 163.1 pm between the (II1/2)-I-2 J = 3/2 and J = 1/2 states, and 119.2 pm, a ground transition between the (2)Pi(3/2) J = 5/2 and J = 3/2 states), at angular resolutions of 16.'3, 16.'3, and 11'.'9, respectively. We also present the CO (16-15) spectrum at the same position. We compared the integrated intensities in the redshifted wings to the results of shock models. Results. The two OH triplets near 163 pm are detected in emission, but with blending hyperfine structure unresolved. Their profiles and that of CO (16-15) can be fitted by a combination of two or three Gaussians. The observed 119.2 mu m triplet is seen in absorption, since its blending hyperfine structure is unresolved, but with three line-of-sight components and a blueshifted emission wing consistent with that of the other lines. The OH line wings are similar to those of CO, suggesting that they emanate from the same shocked structure. Conclusions. Under this common origin assumption, the observations fall within the model predictions and within the range of use of our model only if we consider that four shock structures are caught in our beam. Overall, our comparisons suggest that all the observations might be consistently fitted by a J-type shock model with a high pre-shock density (nH > 105 cm(3)), a high shock velocity (upsilon(s) > 25 km s(-1)), and with a filling factor of the order of unity. Such a high pre -shock density is generally found in shocks associated to high-mass protostars, contrary to low -mass ones. C1 [Gusdorf, A.] PSL Res Univ, CNRS, UMR 8112, LERMA,Observ Paris, F-75014 Paris, France. [Gusdorf, A.] Univ Paris 06, Sorbonne Univ, UMR 8112, LERMA, F-75005 Paris, France. [Guesten, R.; Menten, K. M.; Csengeri, T.; Gomez-Ruiz, A. I.; Heyminck, S.; Leurini, S.; Requena-Torres, M. A.; Wiesemeyer, H.; Wyrowski, F.] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany. [Flower, D. R.] Univ Durham, Dept Phys, Durham DH1 3LE, England. [des Forets, G. Pineau] Univ Paris 11, CNRS, UMR 8617, IAS, Batiment 121, F-91405 Orsay, France. [Codella, C.] Osservatorio Astrofis Arcetri, INAF, Largo Enrico Fermi 5, I-50125 Florence, Italy. [Jacobs, K.] Univ Cologne, Inst Phys 1, KOSMA, Zulpicher Str 77, D-50937 Cologne, Germany. [Kristensen, L. E.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Wampfler, S. F.] Univ Copenhagen, Niels Bohr Inst, Ctr Star & Planet Format, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark. [Wampfler, S. F.] Univ Copenhagen, Nat Hist Museum Denmark, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark. RP Gusdorf, A (reprint author), PSL Res Univ, CNRS, UMR 8112, LERMA,Observ Paris, F-75014 Paris, France.; Gusdorf, A (reprint author), Univ Paris 06, Sorbonne Univ, UMR 8112, LERMA, F-75005 Paris, France. EM antoine.gusdorf@lra.ens.fr RI Kristensen, Lars/F-4774-2011; Wampfler, Susanne/D-2270-2015 OI Kristensen, Lars/0000-0003-1159-3721; Wampfler, Susanne/0000-0002-3151-7657 FU NASA [NAS2-97001]; Deutsches SOFIA Institut, under DLR [50 OK 0901]; French Agence Nationale de la Recherche as part of the SCHISM project [ANR-09-BLAN-0231-01]; CNRS programme "Physique et Chimie du Milieu Interstellaire" FX We thank an anonymous referee and M. Walmsley for comments that helped to improve this paper. We thank the SOFIA operations and the GREAT instrument teams, whose support has been essential for the GREAT accomplishments, and the DSI telescope engineering team. Based (in part) on observations made with the NASA/DLR Stratospheric Observatory for Infrared Astronomy. SOFIA Science Mission Operations are conducted jointly by the Universities Space Research Association, Inc., under NASA contract NAS2-97001, and the Deutsches SOFIA Institut, under DLR contract 50 OK 0901. We thank N. Cunningham for providing us with the spectacular image of the region. This work was partly funded by grant ANR-09-BLAN-0231-01 from the French Agence Nationale de la Recherche as part of the SCHISM project. It was also partly supported by the CNRS programme "Physique et Chimie du Milieu Interstellaire". NR 61 TC 1 Z9 1 U1 1 U2 4 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A45 DI 10.1051/0004-6361/201425325 PG 9 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300052 ER PT J AU Hendricks, B Boeche, C Johnson, CI Frank, MJ Koch, A Mateo, M Bailey, JI AF Hendricks, Benjamin Boeche, Corrado Johnson, Christian I. Frank, Matthias J. Koch, Andreas Mateo, Mario Bailey, John I., III TI Evidence for a chemical enrichment coupling of globular clusters and field stars in the Fornax dSph SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE galaxies: clusters: individual: Fornax; globular clusters: individual: H4; galaxies: abundances; galaxies: evolution; galaxies: dwarf; stars: abundances ID DWARF SPHEROIDAL GALAXY; GIANT BRANCH DISTANCES; METAL-POOR STARS; RED CLUMP STARS; ABUNDANCE RATIOS; HOMOGENEOUS PHOTOMETRY; DETAILED ABUNDANCES; STELLAR POPULATIONS; INDIVIDUAL STARS; GALACTIC DISC AB The globular cluster H4, located in the center of the Fornax dwarf spheroidal galaxy, is crucial for understanding the formation and chemical evolution of star clusters in low-mass galactic environments. H4 is peculiar because the cluster is significantly more metalrich than the galaxy's other clusters, is located near the galaxy center, and may also be the youngest cluster in the galaxy. In this study, we present detailed chemical abundances derived from high-resolution (R similar to 28 000) spectroscopy of an isolated H4 member star for comparison with a sample of 22 nearby Fornax field stars. We find the H4 member to be depleted in the alpha-elements Si, Ca, and Ti with [Si/Fe] = -0.35 +/- 0.34, [Ca/Fe] = +0.05 +/- 0.08, and [Ti/Fe] = -0.27 +/- 0.23, resulting in an average [alpha/Fe] = -0.19 +/- 0.14. If this result is representative of the average cluster properties, H4 is the only known system with a low [alpha/Fe] ratio and a moderately low metallicity embedded in an intact birth environment. For the field stars we find a clear sequence, seen as an early depletion in [alpha/Fe] at low metallicities, in good agreement with previous measurements. H4 falls on top of the observed field star [alpha/Fe] sequence and clearly disagrees with the properties of Milky Way halo stars. We therefore conclude that within a galaxy, the chemical enrichment of globular clusters may be closely linked to the enrichment pattern of the field star population. The low [alpha/Fe] ratios of H4 and similar metallicity field stars in Fornax give evidence that slow chemical enrichment environments, such as dwarf galaxies, may be the original hosts of alpha-depleted clusters in the halos of the Milky Way and M31. C1 [Hendricks, Benjamin; Frank, Matthias J.; Koch, Andreas] Heidelberg Univ, Zentrum Astron, Landessternwarte, Konigstuhl 12, D-69117 Heidelberg, Germany. [Boeche, Corrado] Heidelberg Univ, Zentrum Astron, Astron Rechen Inst, Monchhofstr 12-14, D-69120 Heidelberg, Germany. [Johnson, Christian I.] Harvard Smithsonian Ctr Astrophys, 60 Garden St,MS-15, Cambridge, MA 02138 USA. [Mateo, Mario; Bailey, John I., III] Univ Michigan, Dept Astron, 1085 South Univ, Ann Arbor, MI 48109 USA. RP Hendricks, B (reprint author), Heidelberg Univ, Zentrum Astron, Landessternwarte, Konigstuhl 12, D-69117 Heidelberg, Germany. EM ben.hendricks@lsw.uni-heidelberg.de OI Koch, Andreas/0000-0002-9859-4956 FU NASA [NAS5-26555]; National ScienceFoundation; German Research Foundation (DFG) [Ko 4161/1]; DFG [Sonderforschungsbereich SFB 881]; Clay Fellowship FX We thank Charli Sakari, Hans-Gunter Ludwig, and Morgan Fouesneau for helpful discussions. The HST data used in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by NASA and the National ScienceFoundation. B.H., M.F., and A.K. acknowledge the German Research Foundation (DFG) for funding from Emmy-Noether grant Ko 4161/1. This work was in part supported by Sonderforschungsbereich SFB 881 "The Milky Way System" (subproject A5) of the DFG. C.I.J. acknowledges support through the Clay Fellowship administered by the Smithsonian Astrophysical Observatory. NR 81 TC 1 Z9 1 U1 0 U2 0 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A86 DI 10.1051/0004-6361/201526996 PG 17 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300093 ER PT J AU Hussain, GAJ Alvarado-Gomez, JD Grunhut, J Donati, JF Alecian, E Oksala, M Morin, J Fares, R Jardine, M Drake, JJ Cohen, O Matt, S Petit, P Redfield, S Walter, FM AF Hussain, G. A. J. Alvarado-Gomez, J. D. Grunhut, J. Donati, J. -F. Alecian, E. Oksala, M. Morin, J. Fares, R. Jardine, M. Drake, J. J. Cohen, O. Matt, S. Petit, P. Redfield, S. Walter, F. M. TI A spectro-polarimetric study of the planet-hosting G dwarf, HD 147513 SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE stars: activity; stars: magnetic field; stars: solar-type; stars: individual: HD 147513; techniques: polarimetric; techniques: radial velocities ID SOLAR-TYPE STARS; ANGULAR-MOMENTUM EVOLUTION; MAIN-SEQUENCE STARS; URSA-MAJOR GROUP; MAGNETIC-FIELD; ACTIVE STARS; COOL STARS; KINEMATIC GROUPS; ROTATION; EMISSION AB The results from a spectro-polarimetric study of the planet-hosting Sun-like star, HD 147513 (G5V), are presented here. Robust detections of Zeeman signatures at all observed epochs indicate a surface magnetic field, with longitudinal magnetic field strengths varying between 1.0-3.2 G. Radial velocity variations from night to night modulate on a similar timescale to the longitudinal magnetic field measurements. These variations are therefore likely due to the rotational modulation of stellar active regions rather than the much longer timescale of the planetary orbit (P-orb = 528 d). Both the longitudinal magnetic field measurements and radial velocity variations are consistent with a rotation period of 10 +/- 2 days, which are also consistent with the measured chromospheric activity level of the star ('log R-HK' = -4.64). Together, these quantities indicate a low inclination angle, i similar to 18 degrees. We present preliminary magnetic field maps of the star based on the above period and find a simple poloidal large-scale field. Chemical analyses of the star have revealed that it is likely to have undergone a barium-enrichment phase in its evolution because of a higher mass companion. Despite this, our study reveals that the star has a fairly typical activity level for its rotation period and spectral type. Future studies will enable us to explore the long-term evolution of the field, as well as to measure the stellar rotation period, with greater accuracy. C1 [Hussain, G. A. J.; Alvarado-Gomez, J. D.; Grunhut, J.] European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany. [Hussain, G. A. J.; Donati, J. -F.; Petit, P.] Univ Toulouse, Inst Rech Astrophys, UPS OMP, F-31400 Toulouse, France. [Alvarado-Gomez, J. D.] Univ Munich, Univ Sternwarte Munchen, Scheinerstr 1, D-81679 Munich, Germany. [Donati, J. -F.; Petit, P.] CNRS, Inst Rech Astrophys & Planetol, 14 Ave Edouard Belin, F-31400 Toulouse, France. [Alecian, E.] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France. [Alecian, E.] CNRS, IPAG, F-38000 Grenoble, France. [Alecian, E.; Oksala, M.] Univ Paris Diderot, UPMC, Observ Paris, LESIA,CNRS,UMR 8109, 5 Pl Jules Janssen, F-92190 Meudon, France. [Morin, J.] CNRS, LUPM UMR 5299, Pl Eugene Bataillon, F-34095 Montpellier 05, France. [Morin, J.] Univ Montpellier, Pl Eugene Bataillon, F-34095 Montpellier 05, France. [Fares, R.] Osserv Astrofis Catania, INAF, Via Santa Sofia 78, I-95123 Catania, Italy. [Jardine, M.] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland. [Drake, J. J.; Cohen, O.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Matt, S.] Univ Exeter, Dept Phys & Astron, Stocker Rd, Exeter EX4 4QL, Devon, England. [Redfield, S.] Wesleyan Univ, Dept Astron, Van Vleck Observ, 96 Foss Hill Dr, Middletown, CT 06459 USA. [Walter, F. M.] SUNY Stony Brook, Dept Phys & Astron, Stony Brook, NY 11794 USA. RP Hussain, GAJ (reprint author), European So Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany.; Hussain, GAJ (reprint author), Univ Toulouse, Inst Rech Astrophys, UPS OMP, F-31400 Toulouse, France. EM ghussain@eso.org OI Alvarado Gomez, Julian David/0000-0001-5052-3473; Petit, Pascal/0000-0001-7624-9222; Morin, Julien/0000-0002-4996-6901; Redfield, Seth/0000-0003-3786-3486; Cohen, Ofer/0000-0003-3721-0215; Matt, Sean/0000-0001-9590-2274 FU ESO Telescopes at the La Silla Paranal Observatory [089.D-0138]; IDEX initiative at Universite Federale Toulouse Midi-Pyrenees (UFT-MiP) FX Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under the programme ID 089.D-0138 and using spectra downloaded from the ESO Science Archive Facility under the request number GHUSSAIN-162114. We also thank the IDEX initiative at Universite Federale Toulouse Midi-Pyrenees (UFT-MiP) for funding the "STEPS" collaboration through the Chaire d'Attractivite programme, which enables G.A.J.H. to carry out regular research visits to Toulouse. NR 45 TC 3 Z9 3 U1 0 U2 0 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A77 DI 10.1051/0004-6361/201526595 PG 7 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300084 ER PT J AU Mortier, A Faria, JP Santos, NC Rajpaul, V Figueira, P Boisse, I Cameron, AC Dumusque, X Lo Curto, G Lovis, C Mayor, M Melo, C Pepe, F Queloz, D Santerne, A Segransan, D Sousa, SG Sozzetti, A Udry, S AF Mortier, A. Faria, J. P. Santos, N. C. Rajpaul, V. Figueira, P. Boisse, I. Cameron, A. Collier Dumusque, X. Lo Curto, G. Lovis, C. Mayor, M. Melo, C. Pepe, F. Queloz, D. Santerne, A. Segransan, D. Sousa, S. G. Sozzetti, A. Udry, S. TI The HARPS search for southern extra-solar planets XXXIX. HD175607, the most metal-poor G dwarf with an orbiting sub-Neptune SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE planetary systems; stars: individual: HD175607; techniques: radial velocities; stars: solar-type; stars: activity; stars: abundances ID GAUSSIAN PROCESS FRAMEWORK; LOMB-SCARGLE PERIODOGRAM; RADIAL-VELOCITY DATA; CHAIN MONTE-CARLO; STELLAR ACTIVITY; SUPER-EARTHS; SPIN-ORBIT; STARS; METALLICITY; PARAMETERS AB Context. The presence of a small-mass planet (M-p < 0.1 M-Jup) seems, to date, not to depend on metallicity, however, theoretical simulations have shown that stars with subsolar metallicities may be favoured for harbouring smaller planets. A large, dedicated survey of metal-poor stars with the HARPS spectrograph has thus been carried out to search for Neptunes and super-Earths. Aims. In this paper, we present the analysis of HD175607, an old G6 star with metallicity [Fe/H] = -0.62. We gathered 119 radial velocity measurements in 110 nights over a time span of more than nine years. Methods. The radial velocities were analysed using Lomb-Scargle periodograms, a genetic algorithm, a Markov chain Monte Carlo analysis, and a Gaussian processes analysis. The spectra were also used to derive stellar properties. Several activity indicators were analysed to study the effect of stellar activity on the radial velocities. Results. We find evidence for the presence of a small Neptune-mass planet (M-p sin i = 8.98 +/- 1.10 M-circle times) orbiting this star with an orbital period P = 29.01 +/- 0.02 days in a slightly eccentric orbit (e = 0.11 +/- 0.08). The period of this Neptune is close to the estimated rotational period of the star. However, from a detailed analysis of the radial velocities together with the stellar activity, we conclude that the best explanation of the signal is indeed the presence of a planetary companion rather than stellar related. An additional longer period signal (P similar to 1400 d) is present in the data, for which more measurements are needed to constrain its nature and its properties. Conclusions. HD175607 is the most metal-poor FGK dwarf with a detected low-mass planet amongst the currently known planet hosts. This discovery may thus have important consequences for planet formation and evolution theories. C1 [Mortier, A.; Cameron, A. Collier] Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland. [Faria, J. P.; Santos, N. C.; Figueira, P.; Santerne, A.; Sousa, S. G.] Univ Porto, CAUP, Inst Astrofis & Ciencias Espaco, Rua Estrelas, P-4150762 Oporto, Portugal. [Faria, J. P.; Santos, N. C.] Univ Porto, Fac Ciencias, Dept Fis & Astron, P-4099002 Oporto, Portugal. [Rajpaul, V.] Univ Oxford, Dept Phys, Subdept Astrophys, Oxford OX1 3RH, England. [Boisse, I.] Aix Marseille Univ, CNRS, LAM, UMR 7326, F-13388 Marseille, France. [Dumusque, X.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Lo Curto, G.; Melo, C.] European So Observ, Casilla 19001, Santiago 19, Chile. [Lovis, C.; Mayor, M.; Pepe, F.; Queloz, D.; Segransan, D.; Udry, S.] Univ Geneva, Observ Geneve, 51 Ch Maillettes, CH-1290 Sauverny, Switzerland. [Queloz, D.] Univ Cambridge, Inst Astron, Madingley Rd, Cambridge CB3 0HA, England. [Sozzetti, A.] INAF Osservatorio Astron Torino, Via Osservatorio 20, I-10025 Pino Torinese, Italy. RP Mortier, A (reprint author), Univ St Andrews, Sch Phys & Astron, SUPA, St Andrews KY16 9SS, Fife, Scotland. EM am352@st-andrews.ac.uk RI Figueira, Pedro/J-4916-2013; OI Figueira, Pedro/0000-0001-8504-283X; Faria, Joao/0000-0002-6728-244X; Santerne, Alexandre/0000-0002-3586-1316; Cameron, Andrew/0000-0002-8863-7828; Mortier, Annelies/0000-0001-7254-4363 FU European Union [313014, 627202]; FCT [SFRH/BD/93848/2013]; Fundacao para a Ciencia e a Tecnologia (FCT) [UID/FIS/04434/2013]; FCT through Investigador FCT [IF/01037/2013, IF/00169/2012, IF/00028/2014]; POPH/FSE (EC) by FEDER through the programme "Programa Operacional de Factores de Competitividade - COMPETE"; COST Action [TD 1308] FX This work made use of the Simbad Database. The research leading to these results received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement number 313014 (ETAEARTH). JPF acknowledges support from FCT through grant reference SFRH/BD/93848/2013. This work was supported by Fundacao para a Ciencia e a Tecnologia (FCT) through the research grant UID/FIS/04434/2013. P.F., N.C.S., and S.G.S. also acknowledge the support from FCT through Investigador FCT contracts of reference IF/01037/2013, IF/00169/2012, and IF/00028/2014, respectively, and POPH/FSE (EC) by FEDER funding through the programme "Programa Operacional de Factores de Competitividade - COMPETE". This work results within the collaboration of the COST Action TD 1308. A.S. is supported by the European Union under a Marie Curie Intra-European Fellowship for Career Development with reference FP7-PEOPLE-2013-IEF, number 627202. NR 76 TC 6 Z9 6 U1 0 U2 6 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A135 DI 10.1051/0004-6361/201526905 PG 11 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300142 ER PT J AU Moscadelli, L Sanchez-Monge, A Goddi, C Li, JJ Sanna, A Cesaroni, R Pestalozzi, M Molinari, S Reid, MJ AF Moscadelli, L. Sanchez-Monge, A. Goddi, C. Li, J. J. Sanna, A. Cesaroni, R. Pestalozzi, M. Molinari, S. Reid, M. J. TI Outflow structure within 1000 au of high-mass YSOs I. First results from a combined study of maser and radio continuum emission SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE ISM: jets and outflows; ISM: molecules; masers; radio continum: ISM; techniques: interferometric ID STAR-FORMING REGIONS; YOUNG STELLAR OBJECT; HYPERCOMPACT HII-REGIONS; EXTENDED GREEN OBJECTS; GHZ METHANOL MASERS; TRIGONOMETRIC PARALLAXES; MOLECULAR OUTFLOWS; PROPER MOTIONS; SPIRAL ARM; PROTOSTELLAR CANDIDATES AB Context. In high-mass >= M-circle dot) star formation (SF) studies, high -angular resolution is crucial for resolving individual protostellar outflows (and possibly accretion disks) from the complex contribution of nearby (high- and low -mass) young stellar objects (YSO). Previous interferometric studies have focused mainly on single objects. Aims. A sensitive survey at high angular resolution is required to investigate outflow processes in a statistically significant sample of high -mass YSOs and on spatial scales relevant to testing theories. Methods. We selected a sample of 40 high -mass YSOs from water masers observed within the BeSSeL Stuvey. We investigated the 3D) velocity and spatial structures of the molecular component of massive outflows at milli-arcsecond angular resolution using multi-epoch Very Long Baseline Array (VLBA) observations of 22 GIlz water masers. We also characterize the ionized component of the flows using deep images of the radio continuum emission with resolutions of (Y.'2, at 6, 13, and 22 GIlz with the Jansky Very Large Array (JVLA). Results. We report the first results obtained for a subset of 11 objects from the sample. The water maser measurements provide us with a very accurate description of the molecular gas kinematics. This in turn enables us to estimate the momentiun rate of individual outflows, varying in the range 10-3-10' Mc, yr(-1) km s(-1), among the highest values reported in the literature. In all the observed objects, the continuum emission at 13 and 22 GHz has a compact structure, With its position coincident with that of the water masers. The 6 GHz continuum consists of either compact components (mostly well aligned with the 13 and/or 22 GHz sources) or extended emission (either highly elongated or approximately spherical), which can be offset by up to a few arcseconds from the water masers. The unresolved continuum emission associated with the water masers likely points to the YSO location. The comparison of the radio continuum morphology to the maser spatial and 3D velocity distribution shows that five out of eleven high -mass YSOs emit a collimated outflow, with a flow semi -opening angle in the range 10'-30'. The remaining six sources present a more complicated relationship between the geometry of the radio continuum and water maser velocity pattern; therefore, no firm conclusions can be drawn regarding their outflow structure. In two sources, the 6 GlIz continuum emission shows a highly elongated structure with a negative spectral index down to 1.2. We interpret this finding in terms of synchrotron emission from relativistic electrons accelerated in strong shocks, which indicates that non-thermal continuum emission could be common in high -mass protostellar jets. The Lyman continua derived from bolometric luminosities always exceed those obtained from the radio luminosities. Conclusions. These first results suggest that collimated outflows or jets can be common in high -mass YSOs and, in a couple of cases, provide hints that magnetic fields could be important in driving these jets. To draw firmer conclusions, however, we await completion of the analysis for the entire sample of 40 high -mass YSOs. C1 [Moscadelli, L.; Cesaroni, R.] Osservatorio Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy. [Sanchez-Monge, A.] Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany. [Goddi, C.] Radboud Univ Nijmegen, Dept Astrophys, Inst Math Astrophys & Particle Phys, POB 9010, NL-6500 GL Nijmegen, Netherlands. [Goddi, C.] Joint Inst VLBI Europe, Postbus 2, NL-7990 AA Dwingeloo, Netherlands. [Li, J. J.; Sanna, A.] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany. [Li, J. J.] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China. [Pestalozzi, M.; Molinari, S.] Ist Fis Spazio Interplanetario, INAF, Via Fosso Cavaliere 100, I-00133 Rome, Italy. [Reid, M. J.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Moscadelli, L (reprint author), Osservatorio Astrofis Arcetri, INAF, Largo E Fermi 5, I-50125 Florence, Italy. EM mosca@arcetri.astro.it RI Molinari, Sergio/O-4095-2016 OI Molinari, Sergio/0000-0002-9826-7525 FU collaborative research center project - Deutsche Forschungsgemeinschaft (DFG) [SFB 956]; Deutsche Forschungsgemeinschaft (DFG) Priority Program 1573; National Science Foundation of China [11203082, 11133008]; Natural Science Foundation of Jiangsu Province [BK2012494]; Chinese Academy of Sciences [XDB09000000]; Key Laboratory for Radio Astronomy, CAS FX We are grateful to Rick Perley for the precious help in the calibration of the JVLA data. A.S.-M. acknowledges support by the collaborative research center project SFB 956, funded by the Deutsche Forschungsgemeinschaft (DFG). A.S. gratefully acknowledges financial support by the Deutsche Forschungsgemeinschaft (DFG) Priority Program 1573. J.J. Li was supported by the National Science Foundation of China (Grants Nos. 11203082 and 11133008), the Natural Science Foundation of Jiangsu Province (Grants No. BK2012494), the Strategic Priority Research Program of the Chinese Academy of Sciences (Grants No. XDB09000000), and the Key Laboratory for Radio Astronomy, CAS. NR 75 TC 7 Z9 7 U1 3 U2 6 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 DI 10.1051/0004-6361/201526238 PG 41 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300078 ER PT J AU Pinilla, P Klarmann, L Birnstiel, T Benisty, M Dominik, C Dullemond, CP AF Pinilla, P. Klarmann, L. Birnstiel, T. Benisty, M. Dominik, C. Dullemond, C. P. TI A tunnel and a traffic jam: How transition disks maintain a detectable warm dust component despite the presence of a large planet-carved gap SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE protoplanetary disks ID PROTOPLANETARY DISKS; CIRCUMSTELLAR DISKS; SCATTERED-LIGHT; EMBEDDED PLANETS; SEQUENCE STARS; MOLECULAR GAS; SNOW LINE; HD 100546; COAGULATION; DISCS AB Context. Transition disks are circumstellar disks that show evidence of a dust cavity, which may be related to dynamical clearing by embedded planet(s). Most of these objects show signs of significant accretion, indicating that the inner disks are not truly empty, but that gas is still streaming through to the star. A subset of transition disks, sometimes called pre-transition disks, also shows a strong near-infrared excess, interpreted as an optically thick dusty belt located close to the dust sublimation radius within the first astronomical unit. Aims. We study the conditions for the survival and maintenance of such an inner disk in the case where a massive planet opens a gap in the disk. In this scenario, the planet filters out large dust grains that are trapped at the outer edge of the gap, while the inner regions of the disk may or may not be replenished with small grains. Methods. We combined hydrodynamical simulations of planet-disk interactions with dust evolution models that include coagulation and fragmentation of dust grains over a large range of radii and derived observational properties using radiative transfer calculations. We studied the role of the snow line in the survival of the inner disk of transition disks. Results. Inside the snow line, the lack of ice mantles in dust particles decreases the sticking efficiency between grains. As a consequence, particles fragment at lower collision velocities than in regions beyond the snow line. This effect allows small particles to be maintained for up to a few Myr within the first astronomical unit. These particles are closely coupled to the gas and do not drift significantly with respect to the gas. For lower mass planets (1 M-Jup), the pre-transition appearance can be maintained even longer because dust still trickles through the gap created by the planet, moves invisibly and quickly in the form of relatively large grains through the gap, and becomes visible again as it fragments and gets slowed down inside of the snow line. Conclusions. The global study of dust evolution of a disk with an embedded planet, including the changes of the dust aerodynamics near the snow line, can explain the concentration of millimetre-sized particles in the outer disk and the survival of the dust in the inner disk if a large dust trap is present in the outer disk. This behaviour solves the conundrum of the combination of both near-infrared excess and ring-like millimetre emission observed in several transition disks. C1 [Pinilla, P.] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. [Klarmann, L.; Dominik, C.] Univ Amsterdam, Astron Inst Anton Pannekoek, POB 94249, NL-1090 GE Amsterdam, Netherlands. [Birnstiel, T.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Benisty, M.] Univ Grenoble Alpes, IPAG, F-38000 Grenoble, France. [Benisty, M.] CNRS, IPAG, F-38000 Grenoble, France. [Dullemond, C. P.] Heidelberg Univ, Zentrum Astron, Inst Theoret Astrophys, Albert Ueberle Str 2, D-69120 Heidelberg, Germany. RP Pinilla, P (reprint author), Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. EM pinilla@strw.leidenuniv.nl OI Dullemond, Cornelis/0000-0002-7078-5910; Birnstiel, Tilman/0000-0002-1899-8783 FU Koninklijke Nederlandse Akademie van Wetenschappen (KNAW) professor prize; NASA Origins of Solar Systems grant [NNX12AJ04G]; "Programme National de Physique Stellaire" (PNPS) of CNRS/INSU, France FX The authors are very grateful to E. F. van Dishoeck, M. Kama, and C. Espaillat for all their enthusiasm and comments on this paper. We thank M. Min and M. de Juan Ovelar for all the feedback and help during the preparation of this manuscript. P.P. is supported by Koninklijke Nederlandse Akademie van Wetenschappen (KNAW) professor prize to Ewine van Dishoeck. T.B. acknowledges support from NASA Origins of Solar Systems grant NNX12AJ04G. M.B. acknowledges financial support from "Programme National de Physique Stellaire" (PNPS) of CNRS/INSU, France. NR 72 TC 3 Z9 3 U1 0 U2 1 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A35 DI 10.1051/0004-6361/201527131 PG 8 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300042 ER PT J AU Rudolf, N Gunther, HM Schneider, PC Schmitt, JHMM AF Rudolf, N. Guenther, H. M. Schneider, P. C. Schmitt, J. H. M. M. TI Modelling telluric line spectra in the optical and infrared with an application to VLT/X-Shooter spectra SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE atmospheric effects; instrumentation: spectrographs; methods: observational; methods: data analysis ID ATMOSPHERIC TRANSMISSION; HIGH-RESOLUTION; WATER-VAPOR; ABSORPTION; STARS; SPECTROSCOPY; STANDARDS; DATABASE; SEARCH; ATLAS AB Context. Earth's atmosphere imprints a large number of telluric absorption and emission lines on astronomical spectra, especially in the near infrared, that need to be removed before analysing the affected wavelength regions. Aims. These lines are typically removed by comparison to A-or B-type stars used as telluric standards that themselves have strong hydrogen lines, which complicates the removal of telluric lines. We have developed a method to circumvent that problem. Methods. For our IDL software package tellrem we used a recent approach to model telluric absorption features with the line-by-line radiative transfer model (LBLRTM). The broad wavelength coverage of the X-Shooter at VLT allows us to expand their technique by determining the abundances of the most important telluric molecules H2O, O-2, CO2, and CH4 from sufficiently isolated line groups. For individual observations we construct a telluric absorption model for most of the spectral range that is used to remove the telluric absorption from the object spectrum. Results. We remove telluric absorption from both continuum regions and emission lines without systematic residuals for most of the processable spectral range; however, our method increases the statistical errors. The errors of the corrected spectrum typically increase by 10% for S/N similar to 10 and by a factor of two for high-quality data (S/N similar to 100), i.e. the method is accurate on the percent level. Conclusions. Modelling telluric absorption can be an alternative to the observation of standard stars for removing telluric contamination. C1 [Rudolf, N.; Schneider, P. C.; Schmitt, J. H. M. M.] Univ Hamburg, Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany. [Guenther, H. M.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Guenther, H. M.] MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA. [Schneider, P. C.] ESA, Estec, Keplerlaan 1, NL-2201 AZ Noordwijk, Netherlands. RP Rudolf, N (reprint author), Univ Hamburg, Hamburger Sternwarte, Gojenbergsweg 112, D-21029 Hamburg, Germany. EM nrudolf@hs.uni-hamburg.de OI Gunther, Hans Moritz/0000-0003-4243-2840 FU DLR [50OR1002]; DAAD-Doktorandenstipendium; RTG "Extrasolar planets and their host stars" [1351/2] FX N.R. acknowledges support by the DLR under project no. 50OR1002, a "DAAD-Doktorandenstipendium" as well as the RTG 1351/2 "Extrasolar planets and their host stars". This research has made use of NASA's Astrophysics Data System as well as of the SIMBAD database and the VizieR catalogue access tool, operated at CDS, Strasbourg, France. We also want to thank an anonymous referee for exceptionally helpful reports and constructive criticism that helped to substantially improve the paper. NR 26 TC 0 Z9 0 U1 1 U2 1 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A113 DI 10.1051/0004-6361/201322749 PG 9 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300120 ER PT J AU San Jose-Garcia, I Mottram, JC van Dishoeck, EF Kristensen, LE van der Tak, FFS Braine, J Herpin, F Johnstone, D van Kempen, TA Wyrowski, F AF San Jose-Garcia, I. Mottram, J. C. van Dishoeck, E. F. Kristensen, L. E. van der Tak, F. F. S. Braine, J. Herpin, F. Johnstone, D. van Kempen, T. A. Wyrowski, F. TI Linking low- to high-mass young stellar objects with Herschel-HIFI observations of water SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE stars: formation; stars: protostars; ISM: molecules; ISM: kinematics and dynamics; line: profiles ID STAR-FORMING REGIONS; HIGH-J CO; EMBEDDED PROTOSTARS; PACS SPECTROSCOPY; KEY PROGRAM; HH 46; OUTFLOWS; GAS; SHOCKS; EVOLUTION AB Context. Water probes the dynamics in young stellar objects (YSOs) effectively, especially shocks in molecular outflows. It is therefore a key molecule for exploring whether the physical properties of low-mass protostars can be extrapolated to massive YSOs, an important step in understanding the fundamental mechanisms regulating star formation. Aims. As part of the WISH key programme, we investigate excited water line properties as a function of source luminosity, in particular the dynamics and the excitation conditions of shocks along the outflow cavity wall. Methods. Velocity-resolved Herschel-HIFI spectra of the H2O 2(02)-1(11) (988 GHz), 2(11)-2(02) (752 GHz) and 3(12)-3(03) (1097 GHz) lines were analysed, together with (CO)-C-12 J = 10-9 and 16-15, for 52 YSOs with bolometric luminosities ranging from < 1 to > 10(5) L-circle dot. The H2O and (CO)-C-12 line profiles were decomposed into multiple Gaussian components which are related to the different physical structures of the protostellar system. The non-LTE radiative transfer code radex was used to constrain the excitation conditions of the shocks along the outflow cavity. Results. The profiles of the three excited water lines are similar, indicating that they probe the same gas. Two main emission components are seen in all YSOs: a broad component associated with non-dissociative shocks in the outflow cavity wall ("cavity shocks") and a narrow component associated with the quiescent envelope material. More than 60% of the total integrated intensity in the excited water lines comes from the broad cavity shock component, while the remaining emission comes mostly from the envelope for low-mass Class I, intermediate-and high-mass objects, and dissociative "spot shocks" for low-mass Class 0 protostars. The widths of the water lines are surprisingly similar from low-to high-mass YSOs, whereas (CO)-C-12 J = 10-9 line widths increase slightly with Lbol. The excitation analysis of the cavity shock component shows stronger 752 GHz emission for high-mass YSOs, most likely due to pumping by an infrared radiation field. Finally, a strong correlation with slope unity is measured between the logarithms of the total H2O line luminosity, L-H2O, and Lbol, which can be extrapolated to extragalactic sources. This linear correlation, also found for CO, implies that both species primarily trace dense gas directly related to star formation activity. Conclusions. The water emission probed by spectrally unresolved data is largely due to shocks. Broad water and high-J CO lines originate in shocks in the outflow cavity walls for both low-and high-mass YSOs, whereas lower-J CO transitions mostly trace entrained outflow gas. The higher UV field and turbulent motions in high-mass objects compared to their low-mass counterparts may explain the slightly different kinematical properties of (CO)-C-12 J = 10-9 and H2O lines from low-to high-mass YSOs. C1 [San Jose-Garcia, I.; Mottram, J. C.; van Dishoeck, E. F.; van Kempen, T. A.] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. [van Dishoeck, E. F.] Max Planck Inst Extraterr Phys, Giessenbachstr 2, D-85478 Garching, Germany. [Kristensen, L. E.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [van der Tak, F. F. S.] SRON Netherlands Inst Space Res, POB 800, NL-9700 AV Groningen, Netherlands. [van der Tak, F. F. S.] Univ Groningen, Kapteyn Astron Inst, POB 800, NL-9700 AV Groningen, Netherlands. [Braine, J.; Herpin, F.] Univ Bordeaux, Observ Aquitain Sci Univers, 2 Rue Observ,BP 89, F-33270 Floirac, France. [Braine, J.; Herpin, F.] CNRS, LAB, UMR 5804, 2 Rue Observ,BP 89, F-33270 Floirac, France. [Johnstone, D.] Natl Res Council Canada, Herzberg Inst Astrophys, 5071 West Saanich Rd, Victoria, BC V9E 2E7, Canada. [Johnstone, D.] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 1A1, Canada. [Wyrowski, F.] Max Planck Inst Radioastron, Hugel 69, D-53121 Bonn, Germany. RP San Jose-Garcia, I (reprint author), Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. EM sanjose@strw.leidenuniv.nl RI Kristensen, Lars/F-4774-2011 OI Kristensen, Lars/0000-0003-1159-3721 FU European Community [238258]; Space Research Organisation Netherlands (SRON); Netherlands Research School for Astronomy (NOVA); Spinoza grant; A-ERC grant [291141 CHEMPLAN]; Netherlands Organisation for Scientific Research (NWO) [614.001.008] FX The authors are grateful to the anonymous referee for the constructive and thorough reviews, to Sylvie Cabrit for the useful feedbacks that helped to improve the manuscript and to Mihkel Kama for providing data and suggestions to the paper. We would like to thank Umut Yildiz for helping on the data reduction as well as the WISH team for many inspiring discussions. This work is supported by the European Community's Seventh Framework Programme FP7/2007-2013 under grant agreement 238258 (LASSIE) and by the Space Research Organisation Netherlands (SRON). Astrochemistry in Leiden is supported by the Netherlands Research School for Astronomy (NOVA), by a Spinoza grant, A-ERC grant 291141 CHEMPLAN and grant 614.001.008 from the Netherlands Organisation for Scientific Research (NWO). HIFI has been designed and built by a consortium of institutes and university departments from across Europe, Canada and the United States under the leadership of SRON Netherlands Institute for Space Research, Groningen, The Netherlands and with major contributions from Germany, France and the US. Consortium members are: Canada: CSA, U. Waterloo; France: CESR, LAB, LERMA, IRAM; Germany: KOSMA, MPIfR, MPS; Ireland, NUI Maynooth; Italy: ASI, IFSI-INAF, Osservatorio Astrofisico di Arcetri- INAF; Netherlands: SRON, TUD; Poland: CAMK, CBK; Spain: Observatorio Astronomico Nacional (IGN), Centro de Astrobiologia (CSIC-INTA). Sweden: Chalmers University of Technology - MC2, RSS & GARD; Onsala Space Observatory; Swedish National Space Board, Stockholm University - Stockholm Observatory; Switzerland: ETH Zurich, FHNW; USA: Caltech, JPL, NHSC. NR 77 TC 4 Z9 4 U1 1 U2 1 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A103 DI 10.1051/0004-6361/201525708 PG 30 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300110 ER PT J AU van der Marel, N van Dishoeck, EF Bruderer, S Andrews, SM Pontoppidan, KM Herczeg, GJ van Kempen, T Miotello, A AF van der Marel, N. van Dishoeck, E. F. Bruderer, S. Andrews, S. M. Pontoppidan, K. M. Herczeg, G. J. van Kempen, T. Miotello, A. TI Resolved gas cavities in transitional disks inferred from CO isotopologs with ALMA SO ASTRONOMY & ASTROPHYSICS LA English DT Article DE astrochemistry; stars: formation; protoplanetary disks; ISM: molecules ID MAIN-SEQUENCE STARS; 206462 HD 135344B; T-TAURI DISKS; PROTOPLANETARY DISKS; PRETRANSITIONAL DISKS; CIRCUMSTELLAR DISKS; DUST; YOUNG; ACCRETION; EVOLUTION AB Context Transitional disks around young stars with large dust cavities are promising candidates to look for recently formed, embedded planets. Models of planet-disk interaction predict that young planets clear a gap in the gas while trapping dust at larger radii. Other physical mechanisms might also be responsible for cavities. Previous observations have revealed that gas is still present inside these cavities, but the spatial distribution of this gas remains uncertain. Aims. We present high spatial resolution observations with the Atacama Large Millimeter/submillimeter Array (ALMA) of (CO)-C-13 and (CO)-O-18 3-2 or 6-5 lines of four well-studied transitional disks around pre-main-sequence stars with large dust cavities. The line and continuum observations are used to set constraints on the the gas surface density, specifically on the cavity size and density drop inside the cavity. Methods. The physical-chemical model DALI was used to analyze the gas images of SR21, HD 135344B (also known as SAO 206462), DoAr44, and IRS 48. The main parameters of interest are the size, depth and shape of the gas cavity in each of the disks. CO isotope-selective photodissociation is included to properly constrain the surface density in the outer disk from C18O emission. Results. The gas cavities are up to three times smaller than those of the dust in all four disks. Model fits indicate that the surface density inside the gas cavities decreases by a factor of 100 to 10 000 compared with the surface density profile derived from the outer disk. The data can be fit by either introducing one or two drops in the gas surface density or a surface density profile that increases with radius inside the cavity. A comparison with an analytical model of gap depths by planet-disk interaction shows that the disk viscosities are most likely low, between between 10(-3) and 10(-4), for reasonable estimates of planet masses of up to 10 Jupiter masses. Conclusions. The resolved measurements of the gas and dust in transition disk cavities support the predictions of models that describe how planet-disk interactions sculpt gas disk structures and influence the evolution of dust grains. These observed structures strongly suggest the presence of giant planetary companions in transition disk cavities, although at smaller orbital radii than is typically indicated from the dust cavity radii alone. C1 [van der Marel, N.; van Dishoeck, E. F.; van Kempen, T.; Miotello, A.] Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. [van Dishoeck, E. F.; Bruderer, S.] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany. [Andrews, S. M.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Pontoppidan, K. M.] Space Telescope Sci Inst, 3700 San Martin Dr, Baltimore, MD 21218 USA. [Herczeg, G. J.] Peking Univ, Kavli Inst Astron & Astrophys, Yi He Yuan Lu 5, Beijing 100871, Peoples R China. RP van der Marel, N (reprint author), Leiden Univ, Leiden Observ, POB 9513, NL-2300 RA Leiden, Netherlands. EM nmarel@strw.leidenuniv.nl FU Netherlands Research School for Astronomy (NOVA); Royal Netherlands Academy of Arts and Sciences (KNAW) professor prize; European Union A-ERC [291141 CHEMPLAN] FX The authors would like to thank P. Pinilla for useful discussions. Astrochemistry in Leiden is supported by the Netherlands Research School for Astronomy (NOVA), by a Royal Netherlands Academy of Arts and Sciences (KNAW) professor prize, and by the European Union A-ERC grant 291141 CHEMPLAN. This paper makes use of the following ALMA data: ADS/JAO.ALMA/2012.1.00158.S and ADS/JAO.ALMA/2013.1.00100.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. NR 60 TC 25 Z9 25 U1 1 U2 3 PU EDP SCIENCES S A PI LES ULIS CEDEX A PA 17, AVE DU HOGGAR, PA COURTABOEUF, BP 112, F-91944 LES ULIS CEDEX A, FRANCE SN 1432-0746 J9 ASTRON ASTROPHYS JI Astron. Astrophys. PD JAN PY 2016 VL 585 AR A58 DI 10.1051/0004-6361/201526988 PG 14 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DD1VI UT WOS:000369710300065 ER PT J AU Toews, DPL Campagna, L Taylor, SA Balakrishnan, CN Baldassarre, DT Deane-Coe, PE Harvey, MG Hooper, DM Irwin, DE Judy, CD Mason, NA McCormack, JE McCracken, KG Oliveros, CH Safran, RJ Scordato, ESC Stryjewski, KF Tigano, A Uy, JAC Winger, BM AF Toews, David P. L. Campagna, Leonardo Taylor, Scott A. Balakrishnan, Christopher N. Baldassarre, Daniel T. Deane-Coe, Petra E. Harvey, Michael G. Hooper, Daniel M. Irwin, Darren E. Judy, Caroline D. Mason, Nicholas A. McCormack, John E. McCracken, Kevin G. Oliveros, Carl H. Safran, Rebecca J. Scordato, Elizabeth S. C. Stryjewski, Katherine Faust Tigano, Anna Uy, J. Albert C. Winger, Benjamin M. TI Genomic approaches to understanding population divergence and speciation in birds SO AUK LA English DT Review DE evolution; next-generation sequencing; population genomics; transcriptomics ID ZEBRA FINCH GENOME; AVIAN HYBRID ZONE; GENE FLOW; REPRODUCTIVE ISOLATION; DE-NOVO; CHROMOSOMAL REARRANGEMENTS; ULTRACONSERVED ELEMENTS; WILSONIA-PUSILLA; MIGRATORY DIVIDE; SEX-CHROMOSOME AB The widespread application of high-throughput sequencing in studying evolutionary processes and patterns of diversification has led to many important discoveries. However, the barriers to utilizing these technologies and interpreting the resulting data can be daunting for first-time users. We provide an overview and a brief primer of relevant methods (e.g., whole-genome sequencing, reduced-representation sequencing, sequence-capture methods, and RNA sequencing), as well as important steps in the analysis pipelines (e.g., loci clustering, variant calling, wholegenome and transcriptome assembly). We also review a number of applications in which researchers have used these technologies to address questions related to avian systems. We highlight how genomic tools are advancing research by discussing their contributions to 3 important facets of avian evolutionary history. We focus on (1) general inferences about biogeography and biogeographic history, (2) patterns of gene flow and isolation upon secondary contact and hybridization, and (3) quantifying levels of genomic divergence between closely related taxa. We find that in many cases, high-throughput sequencing data confirms previous work from traditional molecular markers, although there are examples in which genome-wide genetic markers provide a different biological interpretation. We also discuss how these new data allow researchers to address entirely novel questions, and conclude by outlining a number of intellectual and methodological challenges as the genomics era moves forward. C1 [Toews, David P. L.; Campagna, Leonardo; Taylor, Scott A.; Deane-Coe, Petra E.; Mason, Nicholas A.] Cornell Lab Ornithol, Fuller Evolutionary Biol Program, Ithaca, NY USA. [Toews, David P. L.; Campagna, Leonardo; Taylor, Scott A.; Mason, Nicholas A.] Cornell Univ, Dept Ecol & Evolutionary Biol, Ithaca, NY USA. [Balakrishnan, Christopher N.; Deane-Coe, Petra E.] E Carolina Univ, Dept Biol, Greenville, NC USA. [Baldassarre, Daniel T.; Uy, J. Albert C.] Univ Miami, Dept Biol, Coral Gables, FL 33124 USA. [Harvey, Michael G.; Judy, Caroline D.] Louisiana State Univ, Dept Biol Sci, Baton Rouge, LA 70803 USA. [Harvey, Michael G.; Judy, Caroline D.] Louisiana State Univ, Museum Nat Sci, Baton Rouge, LA 70803 USA. [Hooper, Daniel M.; Winger, Benjamin M.] Univ Chicago, Comm Evolutionary Biol, Chicago, IL 60637 USA. [Irwin, Darren E.] Univ British Columbia, Dept Zool, Vancouver, BC, Canada. [Irwin, Darren E.] Univ British Columbia, Biodivers Res Ctr, Vancouver, BC V5Z 1M9, Canada. [Judy, Caroline D.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. [McCormack, John E.] Occidental Coll, Moore Lab Zool, Los Angeles, CA 90041 USA. [McCracken, Kevin G.] Univ Miami, Dept Biol, Coral Gables, FL 33124 USA. [Oliveros, Carl H.] Univ Kansas, Dept Ecol & Evolutionary Biol, Lawrence, KS 66045 USA. [Oliveros, Carl H.] Univ Kansas, Biodivers Inst, Lawrence, KS 66045 USA. [Safran, Rebecca J.; Scordato, Elizabeth S. C.] Univ Colorado, Dept Ecol & Evolutionary Biol, Boulder, CO 80309 USA. [Stryjewski, Katherine Faust] Boston Univ, Dept Biol, 5 Cummington St, Boston, MA 02215 USA. [Tigano, Anna] Queens Univ, Dept Biol, Kingston, ON K7L 3N6, Canada. [Winger, Benjamin M.] Field Museum Nat Hist, Integrat Res Ctr, Chicago, IL 60605 USA. RP Toews, DPL (reprint author), Cornell Lab Ornithol, Fuller Evolutionary Biol Program, Ithaca, NY USA.; Toews, DPL (reprint author), Cornell Univ, Dept Ecol & Evolutionary Biol, Ithaca, NY USA. EM toews@cornell.edu OI Uy, J. Albert C./0000-0002-8437-5525; Balakrishnan, Christopher/0000-0002-0788-0659 NR 127 TC 6 Z9 6 U1 28 U2 70 PU AMER ORNITHOLOGISTS UNION PI LAWRENCE PA ORNITHOLOGICAL SOC NORTH AMER PO BOX 1897, LAWRENCE, KS 66044-8897 USA SN 0004-8038 EI 1938-4254 J9 AUK JI AUK PD JAN PY 2016 VL 133 IS 1 BP 13 EP 30 DI 10.1642/AUK-15-51.1 PG 18 WC Ornithology SC Zoology GA DE1WT UT WOS:000370417900002 ER PT J AU Subiaul, F Patterson, EM Barr, R AF Subiaul, Francys Patterson, Eric M. Barr, Rachel TI The cognitive structure of goal emulation during the preschool years SO BRITISH JOURNAL OF DEVELOPMENTAL PSYCHOLOGY LA English DT Article DE action mirroring; intention mirroring; goal emulation; imitation; cognitive structure; cognitive development; social learning; individual learning ID CHIMPANZEES PAN-TROGLODYTES; MULTIPLE IMITATION MECHANISMS; CHILDREN HOMO-SAPIENS; RATIONAL IMITATION; INFANTS IMITATION; SOCIAL COGNITION; MIRROR NEURONS; CULTURE; INTENTIONS; HUMANS AB Humans excel at mirroring both others' actions (imitation) as well as others' goals and intentions (emulation). As most research has focused on imitation, here we focus on how social and asocial learning predict the development of goal emulation. We tested 215 preschool children on two social conditions (imitation, emulation) and two asocial conditions (trial-and-error and recall) using two touch screen tasks. The tasks involved responding to either three different pictures in a specific picture order (Cognitive: appleboycat) or three identical pictures in a specific spatial order (Motor-Spatial: updownright). Generalized linear models demonstrated that during the preschool years, Motor-Spatial emulation is associated with social and asocial learning, while cognitive emulation is associated only with social learning, including motor-spatial emulation and multiple forms of imitation. This result contrasts with those from a previous study using this same data set showing that motor-spatial and cognitive imitation were neither associated with one another nor, generally, predicted by other forms of social or asocial learning. Together, these results suggests that while developmental changes in imitation are associated with multiple - specialized - mechanisms, developmental changes in emulation are associated with age-related changes and a more unitary, domain-general mechanism that receives input from several different cognitive and learning processes, including some that may not necessarily be specialized for social learning. C1 [Subiaul, Francys] George Washington Univ, Dept Speech & Hearing Sci, Washington, DC 20052 USA. [Subiaul, Francys] Ctr Adv Study Human Paleobiol, Dept Anthropol, Washington, DC USA. [Subiaul, Francys] GWU Inst Neurosci, Washington, DC USA. [Subiaul, Francys] Mind Brain Inst, Washington, DC USA. [Subiaul, Francys; Patterson, Eric M.] Natl Museum Nat Hist, Smithsonian Inst, Washington, DC 20560 USA. [Patterson, Eric M.] Georgetown Univ, Dept Biol, Washington, DC 20057 USA. [Barr, Rachel] Georgetown Univ, Dept Psychol, Washington, DC 20057 USA. RP Subiaul, F (reprint author), 2115 G St,NW 204, Washington, DC 20052 USA. EM subiaul@gwu.edu OI Barr, Rachel/0000-0002-5855-9718 FU University Facilitating Funds (GWU); CAREER grant from the National Science Foundation [BCS-0748717] FX We would like to thank the many student volunteers in the Social Cognition Lab of the George Washington University for assisting with recruitment and data collection. Finally, we want to extend our gratitude to the Smithsonian's Institute, National Museum of Natural History, its staff, and visiting children whose participation made this study possible. This study was supported by University Facilitating Funds (GWU) and a CAREER grant from the National Science Foundation to F. Subiaul (BCS-0748717). NR 65 TC 2 Z9 2 U1 1 U2 4 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0261-510X EI 2044-835X J9 BRIT J DEV PSYCHOL JI Br. J. Dev. Psychol. PY 2016 VL 34 IS 1 SI SI BP 132 EP 149 DI 10.1111/bjdp.12111 PG 18 WC Psychology, Developmental SC Psychology GA DE0QJ UT WOS:000370329100010 PM 26338371 ER PT J AU Ray, GC Hufford, GL Overland, JE Krupnik, I McCormick-Ray, J Frey, K Labunski, E AF Ray, G. Carleton Hufford, Gary L. Overland, James E. Krupnik, Igor McCormick-Ray, Jerry Frey, Karen Labunski, Elizabeth TI Decadal Bering Sea seascape change: consequences for Pacific walruses and indigenous hunters SO ECOLOGICAL APPLICATIONS LA English DT Article DE Bering Sea; climate change; Odobenus rosmarus divergens; Pacific walrus; sea ice; seascape; subsistence hunting ID CLIMATE-CHANGE; ICE; ROSMARUS; WIND AB The most significant factors currently affecting the Pacific walrus (Odobenus rosmarus divergens) population are climate change and consequent changes in sea-ice morphology and dynamics. This paper integrates recent physical sea-ice change in the Bering Sea with biological and ecological conditions of walruses in their winter-spring reproductive habitat. Historically, walrus in winter-spring depended on a critical mass of sea-ice habitat to optimize social networking, reproductive fitness, feeding behavior, migration, and energetic efficiency. During 2003-2013, our cross-disciplinary, multiscale analysis from shipboard observations, satellite imagery, and ice-floe tracking, reinforced by information from indigenous subsistence hunters, documented change of sea-ice structure from a plastic continuum to a "mixing bowl" of ice floes moving more independently. This fragmentation of winter habitat preconditions the walrus population toward dispersal mortality and will also negatively affect the availability of resources for indigenous communities. We urge an expanded research and management agenda that integrates walrus natural history and habitat more completely with changing sea-ice morphology and dynamics at multiple scales, while also meeting the needs of local communities. C1 [Ray, G. Carleton; McCormick-Ray, Jerry] Univ Virginia, Dept Environm Sci, Charlottesville, VA 22904 USA. [Hufford, Gary L.] NOAA, Natl Weather Serv, Anchorage, AK USA. [Overland, James E.] NOAA, Pacific Marine Environm Lab, 7600 Sand Point Way Ne, Seattle, WA 98115 USA. [Krupnik, Igor] Smithsonian Inst, Arctic Studies Ctr, Washington, DC 20560 USA. [Frey, Karen] Clark Univ, Dept Geog, Worcester, MA 01610 USA. [Labunski, Elizabeth] US Fish & Wildlife Serv, Anchorage, AK 99503 USA. RP Ray, GC (reprint author), Univ Virginia, Dept Environm Sci, Charlottesville, VA 22904 USA. EM cr@virginia.edu FU North Pacific Research Board; U.S. Marine Mammal Commission: Assessing changing habitats of ice-dependent marine mammals of Beringia [P10-72213]; NOAA Arctic Project of the Climate Program Office; Pacific Marine Environmental Laboratory; U.S. Marine Mammal Commission; Global Biodiversity Fund of the University of Virginia; PMEL [4239] FX The senior author is deeply indebted to Francis H. "Bud" Fay for his expertise, wisdom, and friendship during our long history of associations and discussions concerning Pacific walruses. Others also contributed significantly with respect to natural history and management, notably John J. Burns, formerly of the Alaska Department of Fish and Game, and R.V. Miller of NOAA/NMFS National Marine Mammal Laboratory. We particularly thank Captains Oliver (in 2006) and Lindstrom (in 2007, 2008) of the icebreaker USGC Healy, and the officers, crew, technical personnel, and our companion scientists for assistance. Steve Roberts of the National Center for Atmospheric Research, Boulder, Colorado, made on-board satellite imagery available. Chief Scientist J. M. Grebmeier, and L. W. Cooper (University of Maryland) made research aboard USCGC Healy in 2006 possible. In 2007, we were similarly supported on the Healy by Chief Scientist Raymond Sombrotto (Lamont-Doherty Earth Observatory, Columbia University). In all years, Kathy Kuletz of the U.S. Fish and Wildlife Service, Migratory Bird Management, Anchorage (supported all by the North Pacific Research Board) supported with surveys. In 2007 and 2008, Michael Cameron and colleagues of the NOAA National Marine Mammal Laboratory, Seattle, Washington, provided walrus observations. In 2008, Chadwick Jay and Anthony Fischbach, U.S. Geological Survey, Anchorage, Alaska, provided the same. Brad Benter of the U.S. Fish and Wildlife Service very kindly shared Gambell walrus catch data in Table. Leonard Apangalook, Sr. (deceased), Paul Apangalook, Chester Noongwook, Aaron Iworrigan, Conrad Oozeva, George Noongwook, and other local experts from St. Lawrence Island, Alaska, shared their knowledge on ice associations, behavior, and distributions of walruses and seals on numerous occasions during 2003-2013. We are grateful to the Eskimo Walrus Commission for a thorough discussion of our project at its meeting in Nome, Alaska (December 2003) and for support in presenting preliminary results of our work to indigenous walrus captains in the communities of Gambell and Savoonga, St. Lawrence Island (February 2004). Lyudmila Bogoslovskaya from the Russian Institute of Cultural and Natural Heritage in Moscow, Russia, contributed reports from local hunters of Russian Beringian communities. Robert L Smith, Charlottesville, Virginia, formatted the illustrations. This paper was supported, in part, by contract number P10-72213 of the U.S. Marine Mammal Commission: Assessing changing habitats of ice-dependent marine mammals of Beringia. J. E. Overland was supported by the NOAA Arctic Project of the Climate Program Office; PMEL contribution Number 4239. We also wish to express our thanks for support of publication costs to the Pacific Marine Environmental Laboratory, the U.S. Marine Mammal Commission, and the Global Biodiversity Fund of the University of Virginia. NR 70 TC 2 Z9 2 U1 12 U2 28 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1051-0761 EI 1939-5582 J9 ECOL APPL JI Ecol. Appl. PD JAN PY 2016 VL 26 IS 1 BP 24 EP 41 DI 10.1890/15-0430 PG 18 WC Ecology; Environmental Sciences SC Environmental Sciences & Ecology GA DC8ZY UT WOS:000369511000004 PM 27039507 ER PT J AU Buchanan, B Hamilton, MJ Kilby, JD Gingerich, JAM AF Buchanan, Briggs Hamilton, Marcus J. Kilby, J. David Gingerich, Joseph A. M. TI Lithic networks reveal early regionalization in late Pleistocene North America SO JOURNAL OF ARCHAEOLOGICAL SCIENCE LA English DT Article DE Paleoindian; Clovis; Late Pleistocene; Lithics; Network analysis; Regionalization ID NEUTRON-ACTIVATION ANALYSIS; SOCIAL NETWORKS; CLOVIS; COLONIZATION; DEMOGRAPHY; STONE; SITE; AGE; PALEOECOLOGY; POPULATIONS AB North America was colonized by hunter gatherer populations during the late Pleistocene, and the Clovis culture is the earliest well-documented evidence of this event. Long-standing questions about the colonization process persist, including the extent to which low-density populations maintained contact across the continent and if foraging territories overlapped or were spatially-discrete. Here, we use a network approach to examine the spatial structure of land use associated with the earliest hunter gatherer populations in North America. In particular, we examine the co-occurrence of raw materials used for stone tool manufacture at archaeological sites across the continent. Using a database of 84 Clovis assemblages we show that there are three large isolated, mostly spatially-discrete, lithic exploitation networks across the continent. These regions closely correspond to previously identified differences in Clovis point form, suggesting that Clovis populations were becoming regionally distinct. This process of cultural diversification that begins in the late Pleistocene, continues to develop into the Holocene. (C) 2015 Elsevier Ltd. All rights reserved. C1 [Buchanan, Briggs] Univ Tulsa, Dept Anthropol, Tulsa, OK 74104 USA. [Hamilton, Marcus J.] Santa Fe Inst, Santa Fe, NM 87501 USA. [Hamilton, Marcus J.] Arizona State Univ, Sch Human Evolut & Social Change, Tempe, AZ USA. [Hamilton, Marcus J.] Eastern New Mexico Univ, Dept Anthropol & Appl Archaeol, Portales, NM USA. [Gingerich, Joseph A. M.] N Carolina State Univ, Dept Sociol & Anthropol, Raleigh, NC 27695 USA. [Gingerich, Joseph A. M.] Smithsonian Inst NMNH, Dept Anthropol, Washington, DC USA. RP Buchanan, B (reprint author), Univ Tulsa, Dept Anthropol, Tulsa, OK 74104 USA.; Hamilton, MJ (reprint author), Santa Fe Inst, Santa Fe, NM 87501 USA. EM briggs-buchanan@utulsa.edu; marcusj@santafe.edu FU University of Tulsa Faculty Development Summer Fellowship Program FX We thank Stephen Lycett and two anonymous reviewers for their helpful comments. BB thanks the University of Tulsa Faculty Development Summer Fellowship Program. NR 63 TC 1 Z9 1 U1 4 U2 13 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0305-4403 EI 1095-9238 J9 J ARCHAEOL SCI JI J. Archaeol. Sci. PD JAN PY 2016 VL 65 BP 114 EP 121 DI 10.1016/j.jas.2015.11.003 PG 8 WC Anthropology; Archaeology; Geosciences, Multidisciplinary SC Anthropology; Archaeology; Geology GA DE2LE UT WOS:000370458000011 ER PT J AU Solis, MA Metz, MA AF Solis, M. Alma Metz, Mark A. TI An illustrated guide to the identification of the known species of Diatraea Guilding (Lepidoptera, Crambidae, Crambinae) based on genitalia SO ZOOKEYS LA English DT Article DE Diatraea; sugarcane moths; Poaceae; biofuels; genitalia AB The genus Diatraea Guilding is one of the most economically important groups of moths in the Western Hemisphere. The larvae are stem borers that feed on species of Poaceae, or grasses, such as sugarcane, corn, rice, and sorghum, as well as many other native grasses. Interest in this group has risen considerably since sugarcane and other grasses have been utilized and/or investigated as biofuels. This is the first modern study to treat all 41 valid described species. Most type specimens were examined and we provide a checklist with 19 new synonyms. We provide keys for the identification of most species in this genus based on morphology of the male and female genitalia and modern illustrations of male and female genitalia. We also provide an updated table of species distribution by country. C1 [Solis, M. Alma; Metz, Mark A.] Smithsonian Inst, USDA, ARS, Systemat Entomol Lab,Beltsville Agr Res Ctr,Natl, E 517,MRC 168,POB 37012, Washington, DC 20013 USA. RP Solis, MA; Metz, MA (reprint author), Smithsonian Inst, USDA, ARS, Systemat Entomol Lab,Beltsville Agr Res Ctr,Natl, E 517,MRC 168,POB 37012, Washington, DC 20013 USA. EM alma.solis@ars.usda.gov; mark.metz@ars.usda.gov NR 57 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 565 BP 73 EP 121 DI 10.3897/zookeys.565.6797 PG 49 WC Zoology SC Zoology GA DE0TQ UT WOS:000370338200003 PM 27081337 ER PT J AU Brown, GP Kelehear, C Pizzatto, L Shine, R AF Brown, Gregory P. Kelehear, Crystal Pizzatto, Ligia Shine, Richard TI The impact of lungworm parasites on rates of dispersal of their anuran host, the invasive cane toad SO BIOLOGICAL INVASIONS LA English DT Article DE Anuran; Bufo marinus; Host-parasite; Invasion front; Invasive species ID EXPANDING RANGE-EDGE; BUFO-MARINUS; RHABDIAS-PSEUDOSPHAEROCEPHALA; RHINELLA-MARINA; TROPICAL AUSTRALIA; BIOLOGICAL-CONTROL; TYPHOID MARY; INFECTION; DYNAMICS; FROGS AB Translocation of native-range parasites to control invasive species is effective only if the parasite substantially impairs either the viability or dispersal rate of the invasive host. Lungworms (Rhabdias pseudosphaerocephala) of cane toads (Rhinella marina) were introduced to Australia from the toad's native range, along with the toads, and have been suggested as a potential biocontrol of invasive toads due to various negative impacts on toad viability. We conducted two radio-telemetry studies on a tropical floodplain to specifically assess the parasite's impact on toad dispersal. First, a retrospective correlative analysis of data from field-collected animals showed that toads infected with lungworms moved farther, not less, than uninfected conspecifics. Second, an experimental study (comparing movements of experimentally infected toads vs. uninfected controls) showed that lungworms did not modify rates of toad dispersal. In addition, experimental infection with lungworms did not elicit an immune response substantial enough to influence dispersal behaviour. Thus, we conclude that increasing lungworm densities at the invasion front as an attempt at biocontrol would not slow down the spread of cane toads. C1 [Brown, Gregory P.; Kelehear, Crystal; Pizzatto, Ligia; Shine, Richard] Univ Sydney, Sch Biol Sci, A08, Sydney, NSW 2006, Australia. [Kelehear, Crystal] Smithsonian Trop Res Inst, Apartado 0843-03092, Panama City, Panama. RP Brown, GP (reprint author), Univ Sydney, Sch Biol Sci, A08, Sydney, NSW 2006, Australia. EM gregory.brown@sydney.edu.au RI Brown, Gregory/F-9897-2011 OI Brown, Gregory/0000-0002-2924-9040 FU Australian Research Council FX We thank the staff of Beatrice Hill Farm for access to their property, the Northern Territory Land Corporation for use of facilities, and the Australian Research Council for funding. We also thank two anonymous reviewers for their improving comments and suggestions. NR 76 TC 0 Z9 0 U1 5 U2 16 PU SPRINGER PI DORDRECHT PA VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS SN 1387-3547 EI 1573-1464 J9 BIOL INVASIONS JI Biol. Invasions PD JAN PY 2016 VL 18 IS 1 BP 103 EP 114 DI 10.1007/s10530-015-0993-1 PG 12 WC Biodiversity Conservation; Ecology SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DD6WT UT WOS:000370066000009 ER PT J AU Moser, CS Wier, TP Grant, JF First, MR Tamburri, MN Ruiz, GM Miller, AW Drake, LA AF Moser, Cameron S. Wier, Timothy P. Grant, Jonathan F. First, Matthew R. Tamburri, Mario N. Ruiz, Gregory M. Miller, A. Whitman Drake, Lisa A. TI Quantifying the total wetted surface area of the world fleet: a first step in determining the potential extent of ships' biofouling SO BIOLOGICAL INVASIONS LA English DT Article DE Aquatic nuisance species; Hull fouling; Invasive species; Wetted surface area; Global fleet; Non-indigenous species ID SEA; INVASIONS; BIOFILMS; GRAVITY; IMPACT AB Ships' hulls can transport aquatic nuisance species, but there is little quantitative information about the magnitude of vessel biofouling on a global or regional scale. There does not exist a robust method to estimate the wetted surface area (WSA) of a particular fleet of ships, especially across the diversity of possible vessel types. An estimate of the total WSA of ship arrivals into a port or region is essential to determine the potential scope of biofouling and to inform management strategies to reduce the future invasions. Multiple statistical models were developed so commonly available ships' parameters could be used to estimate the WSA for a given set of fleet data. Using individual ship characteristics and publicly available data from similar to 120,000 active commercial ships in the world fleet, the method results in a total global minimum WSA estimate of approximately 325 9 10(6) m(2). The size of the global fleet employed here is greater than the commonly cited vessel number of approximately 80,000-90,000, as we include ships <100 gross tons. Over 190,000 vessels were initially identified, representing a WSA of 571 9 10(6) m(2), but active status of only 120,000 vessels could be confirmed. Reliable data were unavailable on the operating status of many additional and especially smaller vessels. This approach, along with a contemporary and comprehensive estimate of global WSA, when combined with knowledge of the different operational profiles of ships that may reduce biofouling (port residence times, steaming speeds, extent of antifouling coatings, cleaning frequency, etc.), can inform current numerical models and risk assessments of bioinvasions. C1 [Moser, Cameron S.; Wier, Timothy P.] Excet Inc, Springfield, VA 22151 USA. [Grant, Jonathan F.] Battenkill Technol Inc, Manchester Ctr, VT 05255 USA. [First, Matthew R.] Naval Res Lab, Div Chem, Code 6136, Washington, DC 20375 USA. [Tamburri, Mario N.] Univ Maryland, Chesapeake Biol Lab, Ctr Environm Sci, Solomons, MD 20688 USA. [Ruiz, Gregory M.; Miller, A. Whitman] Smithsonian Environm Res Ctr, POB 28, Edgewater, MD 21037 USA. [Drake, Lisa A.] Naval Res Lab, Div Chem, Code 6136, Key West, FL 33041 USA. RP Moser, CS (reprint author), Excet Inc, Springfield, VA 22151 USA. EM cameron.moser.ctr@nrl.navy.mil OI First, Matthew/0000-0003-1330-3353; First, Matt/0000-0003-3465-2376; Ruiz, Gregory/0000-0003-2499-441X; Miller, Whitman/0000-0003-0484-182X FU University of Maryland Center for Environmental Science [2012-38]; U.S. Maritime Administration (MARAD) FX This work was supported by the University of Maryland Center for Environmental Science (funding agreement 2012-38) and the U.S. Maritime Administration (MARAD). We thank Carolyn Junemann (MARAD) for guidance and programmatic support and Mark Minton (Smithsonian Environmental Research Center) for his advice with shipping data. We appreciate advice from Rich Everett (U.S. Coast Guard) and the data provided from the National Ballast Information Clearinghouse. This work was supported by Diane Lysogorski, Section Head of NRL Code 6136 and Director of the Center for Corrosion Science and Engineering-Key West, Florida. Finally, the reviews of this manuscript by Stephanie Robbins-Wamsley, Diane Lysogorski, Edward Lemieux (Branch Head, Code 6130), Barry Spargo (Acting Superintendent, Chemistry Division, Naval Research Laboratory), Jim Carlton, and three anonymous reviewers improved it-thank you. NR 46 TC 2 Z9 2 U1 5 U2 13 PU SPRINGER PI DORDRECHT PA VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS SN 1387-3547 EI 1573-1464 J9 BIOL INVASIONS JI Biol. Invasions PD JAN PY 2016 VL 18 IS 1 BP 265 EP 277 DI 10.1007/s10530-015-1007-z PG 13 WC Biodiversity Conservation; Ecology SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DD6WT UT WOS:000370066000020 ER PT J AU Evans, N McKeon, CS AF Evans, Nathaniel McKeon, C. Seabird TI New records and field observations support a facultative commensal association of Thalamita longifrons and Thalamita murinae with soft coral SO BULLETIN OF MARINE SCIENCE LA English DT Editorial Material C1 [Evans, Nathaniel] Univ Florida, Florida Museum Nat Hist, Gainesville, FL 32611 USA. [Evans, Nathaniel; McKeon, C. Seabird] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20013 USA. [McKeon, C. Seabird] Smithsonian Marine Stn Ft Pierce, Ft Pierce, FL 34949 USA. RP Evans, N (reprint author), Univ Florida, Florida Museum Nat Hist, Gainesville, FL 32611 USA.; Evans, N (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20013 USA. EM evansnat@ufl.edu OI Evans, Nathaniel/0000-0003-4524-372X NR 5 TC 0 Z9 0 U1 0 U2 2 PU ROSENSTIEL SCH MAR ATMOS SCI PI MIAMI PA 4600 RICKENBACKER CAUSEWAY, MIAMI, FL 33149 USA SN 0007-4977 EI 1553-6955 J9 B MAR SCI JI Bull. Mar. Sci. PD JAN PY 2016 VL 92 IS 1 BP 105 EP 106 DI 10.5343/bms.2015.1063 PG 2 WC Marine & Freshwater Biology; Oceanography SC Marine & Freshwater Biology; Oceanography GA DD7OJ UT WOS:000370113700007 ER PT J AU Antonelli, TS Leischner, CL Ososky, JJ Hartstone-Rose, A AF Antonelli, T. S. Leischner, C. L. Ososky, J. J. Hartstone-Rose, A. TI The effect of captivity on the oral health of the critically endangered black-footed ferret (Mustela nigripes) SO CANADIAN JOURNAL OF ZOOLOGY LA English DT Article DE Mustela nigripes; black-footed ferret; calculus; periodontal disease; captivity ID PERIODONTAL-DISEASE; WEAR; CALCULUS; DIET AB Black-footed ferrets (Mustela nigripes (Audubon and Bachman, 1851)), a North American species of mustelid, faced near extinction after westward expansion during the 20th century destroyed a majority of the population of prairie dogs (genus Cynomys Rafinesque, 1817), their primary food source. Fearing extinction of the black-footed ferret, the U.S. Fish and Wildlife Service captured the entire population between 1985 and 1987 and began a captive breeding program. While in captivity, the fertility and genetic diversity of the species was closely monitored; however, there is little information about other health consequences of this breeding program. For instance, the black-footed ferrets have been fed a diet that is very different than what they consume in the wild. How did the composition of this diet affect the oral health of these animals? An analysis of dentition of wild and captive black-footed ferrets reveals that calculus accumulation and periodontal diseases occurred with greater severity in captive black-footed ferrets, suggesting that such oral pathologies arose from the unnaturally soft diet fed to them. These findings offer insight into how mechanical properties of diet can affect oral health and how these dietary properties should be considered, not only in regard to the health of black-footed ferrets but also to the health of all mammals including humans. C1 [Antonelli, T. S.; Leischner, C. L.; Hartstone-Rose, A.] Univ S Carolina, Sch Med, Dept Cell Biol & Anat, CBA Bldg 1,Room C-36,6439 Garners Ferry Rd, Columbia, SC 29209 USA. [Ososky, J. J.] Smithsonian Inst, Dept Vertebrate Zool, POB 37012,MRC 108, Washington, DC 20013 USA. RP Hartstone-Rose, A (reprint author), Univ S Carolina, Sch Med, Dept Cell Biol & Anat, CBA Bldg 1,Room C-36,6439 Garners Ferry Rd, Columbia, SC 29209 USA. EM AdamHR@sc.edu RI Hartstone-Rose, Adam/I-3503-2016 OI Hartstone-Rose, Adam/0000-0001-5307-5573 NR 31 TC 1 Z9 1 U1 12 U2 30 PU CANADIAN SCIENCE PUBLISHING, NRC RESEARCH PRESS PI OTTAWA PA 65 AURIGA DR, SUITE 203, OTTAWA, ON K2E 7W6, CANADA SN 0008-4301 EI 1480-3283 J9 CAN J ZOOL JI Can. J. Zool. PD JAN PY 2016 VL 94 IS 1 BP 15 EP 22 DI 10.1139/cjz-2015-0135 PG 8 WC Zoology SC Zoology GA DD6SE UT WOS:000370053700003 ER PT J AU Rota, CT Wikle, CK Kays, RW Forrester, TD McShea, WJ Parsons, AW Millspaugh, JJ AF Rota, Christopher T. Wikle, Christopher K. Kays, Roland W. Forrester, Tavis D. McShea, William J. Parsons, Arielle W. Millspaugh, Joshua J. TI A two-species occupancy model accommodating simultaneous spatial and interspecific dependence SO ECOLOGY LA English DT Article DE coyote (Canis latrans); data augmentation; detection probability; eMammal; geostatistical model; hierarchical models; interacting species; point-referenced model; red fox (Vulpes vulpes); spatial statistics ID RED FOXES; COOCCURRENCE; PARAMETERIZATION; SELECTION; PATTERNS AB Occupancy models are popular for estimating the probability a site is occupied by a species of interest when detection is imperfect. Occupancy models have been extended to account for interacting species and spatial dependence but cannot presently allow both factors to act simultaneously. We propose a two-species occupancy model that accommodates both interspecific and spatial dependence. We use a point-referenced multivariate hierarchical spatial model to account for both spatial and interspecific dependence. We model spatial random effects with predictive process models and use probit regression to improve efficiency of posterior sampling. We model occupancy probabilities of red fox (Vulpes vulpes) and coyote (Canis latrans) with camera trap data collected from six mid-Atlantic states in the eastern United States. We fit four models comprising a fully factorial combination of spatial and interspecific dependence to two-thirds of camera trapping sites and validated models with the remaining data. Red fox and coyotes each exhibited spatial dependence at distances >0.8 and 0.4km, respectively, and exhibited geographic variation in interspecific dependence. Consequently, predictions from the model assuming simultaneous spatial and interspecific dependence best matched test data observations. This application highlights the utility of simultaneously accounting for spatial and interspecific dependence. C1 [Rota, Christopher T.; Millspaugh, Joshua J.] Univ Missouri, Dept Fisheries & Wildlife Sci, Columbia, MO 65203 USA. [Rota, Christopher T.; Wikle, Christopher K.] Univ Missouri, Dept Stat, Columbia, MO 65203 USA. [Kays, Roland W.; Parsons, Arielle W.] North Carolina Museum Nat Sci, Raleigh, NC 27603 USA. [Forrester, Tavis D.; McShea, William J.] Smithsonian Conservat Biol Inst, Front Royal, VA 22630 USA. RP Rota, CT (reprint author), Univ Missouri, Dept Fisheries & Wildlife Sci, Columbia, MO 65203 USA. EM christopher.rota@gmail.com OI Rota, Christopher/0000-0001-9272-4687 FU National Science Foundation [1232442, 1319293]; VWR Foundation; U.S. Forest Service; North Carolina Museum of Natural Sciences; Smithsonian Institution; NSF [DMS-104903] FX We thank our 376 volunteers for their hard work collecting camera trap data for this study. For their field assistance and volunteer coordination we thank the staff of the National Park Service, U.S. Fish and Wildlife Service, U.S. Forest Service, The Nature Conservancy, North Carolina, South Carolina, Virginia, Maryland, and Tennessee State Parks, North Carolina Wildlife Resources Commission, Tennessee Division of Forestry, Virginia Department of Game and Inland Fisheries, West Virginia Water Authority, the Wintergreen Nature Foundation, and Raleigh, Parks, Recreation and Cultural Resources. We thank N. Fuentes, S. Higdon, T. Perkins, L. Gatens, R. Owens, R. Gayle, C. Backman, K. Clark, J. Grimes, and J. Simkins for their help reviewing photographs. This work was conducted with funding from the National Science Foundation grant #1232442 and #1319293, the VWR Foundation, the U.S. Forest Service, the North Carolina Museum of Natural Sciences and the Smithsonian Institution. C. K. Wikle was partially supported by NSF DMS-104903. We thank P. Conn, S. Holan, M. Hooten, and an anonymous reviewer for helpful comments on early versions of this manuscript. NR 32 TC 3 Z9 3 U1 28 U2 60 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0012-9658 EI 1939-9170 J9 ECOLOGY JI Ecology PD JAN PY 2016 VL 97 IS 1 BP 48 EP 53 DI 10.1890/15-1193.1 PG 6 WC Ecology SC Environmental Sciences & Ecology GA DD3VZ UT WOS:000369852600007 PM 27008774 ER PT J AU Chang, CH Szlavecz, K Filley, T Buyer, JS Bernard, MJ Pitz, SL AF Chang, Chih-Han Szlavecz, Katalin Filley, Timothy Buyer, Jeffrey S. Bernard, Michael J. Pitz, Scott L. TI Belowground competition among invading detritivores SO ECOLOGY LA English DT Article DE Amynthas hilgendorfi; C-13 and N-15 labeling; earthworm; Eisenoides lonnbergi; functional group; interspecific competition; invasive species; Lumbricus rubellus; Octolasion lacteum; stable isotope; temperate deciduous forest ID STABLE-ISOTOPE ANALYSIS; LUMBRICUS-RUBELLUS; EARTHWORM INVASIONS; FUNCTIONAL-GROUPS; TEMPERATE FOREST; SOIL BIOTA; DIVERSITY; FOOD; COMMUNITIES; NICHE AB The factors regulating soil animal communities are poorly understood. Current theory favors niche complementarity and facilitation over competition as the primary forms of non-trophic interspecific interaction in soil fauna; however, competition has frequently been suggested as an important community-structuring factor in earthworms, ecosystem engineers that influence belowground processes. To date, direct evidence of competition in earthworms is lacking due to the difficulty inherent in identifying a limiting resource for saprophagous animals. In the present study, we offer the first direct evidence of interspecific competition for food in this dominant soil detritivore group by combining field observations with laboratory mesocosm experiments using C-13 and N-15 double-enriched leaf litter to track consumption patterns. In our experiments, the Asian invasive species Amynthas hilgendorfi was a dominant competitor for leaf litter against two European species currently invading the temperate deciduous forests in North America. This competitive advantage may account for recent invasion success of A. hilgendorfi in forests with established populations of European species, and we hypothesize that specific phenological differences play an important role in determining the outcome of the belowground competition. In contrast, Eisenoides lonnbergi, a common native species in the Eastern United States, occupied a unique trophic position with limited interactions with other species, which may contribute to its persistence in habitats dominated by invasive species. Furthermore, our results supported neither the hypothesis that facilitation occurs between species of different functional groups nor the hypothesis that species in the same group exhibit functional equivalency in C and N translocation in the soil. We propose that species identity is a more powerful approach to understand earthworm invasion and its impacts on belowground processes. C1 [Chang, Chih-Han; Szlavecz, Katalin; Bernard, Michael J.; Pitz, Scott L.] Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21210 USA. [Filley, Timothy] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA. [Buyer, Jeffrey S.] USDA ARS, Sustainable Agr Syst Lab, Beltsville, MD 20705 USA. [Pitz, Scott L.] Smithsonian Environm Res Ctr, POB 28, Edgewater, MD 21037 USA. [Bernard, Michael J.] Marine Biol Lab, Ecosyst Ctr, Woods Hole, MA 02543 USA. RP Chang, CH (reprint author), Johns Hopkins Univ, Dept Earth & Planetary Sci, Baltimore, MD 21210 USA. EM yuanpau@gmail.com OI Buyer, Jeffrey/0000-0003-2098-0547 FU EPS Field Funds; National Science Foundation [EEC-0540832, ACI 1244820, EAR-0748574]; Microsoft Research FX We appreciate two anonymous reviewers for their insightful and constructive comments on an earlier version of this manuscript. We are also grateful to Jay O'Neill, Stanley Tesch, Mac A. Callaham Jr., Pavlo Bohutskyi, Alan Stone, and Chuan-Chin Huang for their suggestions or logistical help, and to the people who helped in the field and during the lab experiments, especially Ziwei He, Kelly Baker, Zachary Ferguson, Adam Dec, and Jia-Hsing Wu. Funding for this study was partially provided by the EPS Field Funds, the National Science Foundation (EEC-0540832, ACI 1244820, and EAR-0748574), and Microsoft Research. NR 63 TC 5 Z9 5 U1 9 U2 39 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0012-9658 EI 1939-9170 J9 ECOLOGY JI Ecology PD JAN PY 2016 VL 97 IS 1 BP 160 EP 170 DI 10.1890/15-0551.1 PG 11 WC Ecology SC Environmental Sciences & Ecology GA DD3VZ UT WOS:000369852600018 PM 27008785 ER PT J AU Martinez-Izquierdo, L Garcia, MM Powers, JS Schnitzer, SA AF Martinez-Izquierdo, Laura Garcia, Maria M. Powers, Jennifer S. Schnitzer, Stefan A. TI Lianas suppress seedling growth and survival of 14 tree species in a Panamanian tropical forest SO ECOLOGY LA English DT Article DE Barro Colorado Island; community ecology; Gigante Peninsula; liana cutting; Panama; tropical plant competition ID BELOW-GROUND COMPETITION; BARRO COLORADO ISLAND; RAIN-FOREST; UNCERTAINTY PRINCIPLE; MOIST-FOREST; COSTA-RICA; REGENERATION; GAPS; UNDERSTOREY; PATTERNS AB Lianas are a common plant growth form in tropical forests, where they compete intensely with trees, decreasing tree recruitment, growth, and survival. If the detrimental effects of lianas vary significantly with tree species identity, as is often assumed, then lianas may influence tree species diversity and community composition. Furthermore, recent studies have shown that liana abundance and biomass are increasing relative to trees in neotropical forests, which will likely magnify the detrimental effects of lianas and may ultimately alter tree species diversity, relative abundances, and community composition. Few studies, however, have tested the responses of multiple tree species to the presence of lianas in robust, well-replicated experiments. We tested the hypotheses that lianas reduce tree seedling growth and survival, and that the effect of lianas varies with tree species identity. We used a large-scale liana removal experiment in Central Panama in which we planted 14 replicate seedlings of 14 different tree species that varied in shade tolerance in each of 16 80x80m plots (eight liana-removal and eight unmanipulated controls; 3136 total seedlings). Over a nearly two-yr period, we found that tree seedlings survived 75% more, grew 300% taller, and had twice the aboveground biomass in liana-removal plots than seedlings in control plots, consistent with strong competition between lianas and tree seedlings. There were no significant differences in the response of tree species to liana competition (i.e., there was no species by treatment interaction), indicating that lianas had a similar negative effect on all 14 tree species. Furthermore, the effect of lianas did not vary with tree species shade tolerance classification, suggesting that the liana effect was not solely based on light. Based on these findings, recently observed increases in liana abundance in neotropical forests will substantially reduce tree regeneration, but will not significantly alter tropical tree species diversity, relative abundance, or community composition. C1 [Martinez-Izquierdo, Laura; Garcia, Maria M.; Schnitzer, Stefan A.] Marquette Univ, Dept Biol Sci, POB 1881, Milwaukee, WI 53201 USA. [Powers, Jennifer S.] Univ Minnesota, Dept Ecol Evolut & Behav, 1987 Upper Buford Circle, St Paul, MN 55108 USA. [Powers, Jennifer S.] Univ Minnesota, Dept Plant Biol, 1987 Upper Buford Circle, St Paul, MN 55108 USA. [Powers, Jennifer S.; Schnitzer, Stefan A.] Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Balboa, Panama. RP Schnitzer, SA (reprint author), Marquette Univ, Dept Biol Sci, POB 1881, Milwaukee, WI 53201 USA.; Schnitzer, SA (reprint author), Smithsonian Trop Res Inst, Apartado Postal 0843-03092, Balboa, Panama. EM S1@marquette.edu FU [NSF-DEB 0845071]; [NSF-DEB1019436]; [NSF DEB-1019441] FX We thank Guadalupe Alvarado, Evelyn Sanchez, Salome Perez, Oldemar Valdes, Abelino Valdes, Severino Valdes, and Boris Bernal for valuable assistance in the field. We are grateful to Nick Rowe, Deborah Clark, and especially Natalia Norden, who made substantive comments on several versions of the manuscript. Financial support was provided by NSF-DEB 0845071 and NSF-DEB 1019436 (to S. A. Schnitzer), and NSF DEB-1019441 (to J. S. Powers). NR 64 TC 4 Z9 5 U1 12 U2 27 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0012-9658 EI 1939-9170 J9 ECOLOGY JI Ecology PD JAN PY 2016 VL 97 IS 1 BP 215 EP 224 DI 10.1890/14-2261.1 PG 10 WC Ecology SC Environmental Sciences & Ecology GA DD3VZ UT WOS:000369852600023 PM 27008790 ER PT J AU DeVience, SJ Walsworth, RL Rosen, MS AF DeVience, Stephen J. Walsworth, Ronald L. Rosen, Matthew S. TI Probing scalar coupling differences via long-lived singlet states SO JOURNAL OF MAGNETIC RESONANCE LA English DT Article DE Nuclear singlet state; Spin-lock induced crossing; J coupling; Decoherence-free subspace ID NUCLEAR-MAGNETIC-RESONANCE; SPIN STATES; NMR-SPECTROSCOPY; SLOW DIFFUSION; HYPERPOLARIZATION; LIFETIMES; ORDER; FIELD; MRI; POLARIZATION AB We probe small scalar coupling differences via the coherent interactions between two nuclear spin singlet states in organic molecules. We show that the spin-lock induced crossing (SLIC) technique enables the coherent transfer of singlet order between one spin pair and another. The transfer is mediated by the difference in syn and anti vicinal or long-range J couplings among the spins. By measuring the transfer rate, we calculate a J coupling difference of 8 +/- 2 mHz in phenylalanine-glycine-glycine and 2.57 +/- 0.04 Hz in glutamate. We also characterize a coherence between two singlet states in glutamate, which may enable the creation of a long-lived quantum memory. Published by Elsevier Inc. C1 [DeVience, Stephen J.] Harvard Univ, Dept Chem & Chem Biol, 12 Oxford St, Cambridge, MA 02138 USA. [Walsworth, Ronald L.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Walsworth, Ronald L.; Rosen, Matthew S.] Harvard Univ, Dept Phys, 17 Oxford St, Cambridge, MA 02138 USA. [Walsworth, Ronald L.] Harvard Univ, Ctr Brain Sci, 52 Oxford St, Cambridge, MA 02138 USA. [Rosen, Matthew S.] Harvard Univ, Sch Med, 25 Shattuck St, Boston, MA 02115 USA. [Rosen, Matthew S.] AA Martinos Ctr Biomed Imaging, 149 Thirteenth St, Boston, MA 02129 USA. RP Walsworth, RL (reprint author), Harvard Smithsonian Ctr Astrophys, MS 59,60 Garden St, Cambridge, MA 02138 USA. EM rwalsworth@cfa.harvard.edu RI DeVience, Stephen/D-7274-2012 OI DeVience, Stephen/0000-0003-3142-7296 FU National Science Foundation; Smithsonian Astrophysical Observatory FX This work was supported by the National Science Foundation and the Smithsonian Astrophysical Observatory. NR 50 TC 2 Z9 2 U1 3 U2 6 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1090-7807 EI 1096-0856 J9 J MAGN RESON JI J. Magn. Reson. PD JAN PY 2016 VL 262 BP 42 EP 49 DI 10.1016/j.jmr.2015.12.003 PG 8 WC Biochemical Research Methods; Physics, Atomic, Molecular & Chemical; Spectroscopy SC Biochemistry & Molecular Biology; Physics; Spectroscopy GA DD4FK UT WOS:000369877700007 PM 26717036 ER PT J AU Cairns, SD AF Cairns, Stephen D. TI A key to the genera and species of the transversely-dividing Flabellidae (Anthozoa, Scleractinia, Flabellidae), with a guide to the literature, and the description of two new species SO ZOOKEYS LA English DT Article DE Flabellidae; Truncatoflabellum; Placotrochides; Blastotrochus; Placotrochus; Falcatoflabellum; transversely dividing; key; asexual reproduction ID AZOOXANTHELLATE SCLERACTINIA; CNIDARIA ANTHOZOA; CORALS; ISLANDS; VANUATU AB The transversely-dividing flabellids consist of five genera (Truncatoflabellum, Placotrochides, Blastotrochus, Placotrochus, and Falcatoflabellum) and 45 species. A dichotomous key is provided for these five genera as well as the species of the genus Truncatoflabellum and Placotrochides, the other three genera being monotypic. A tabular key is also provided for the 38 species of Truncatoflabellum. Two new combinations are suggested (T. gambierense and T. sphenodeum) and two new species are described (T. duncani and T. mozambiquensis). All but one species are illustrated and accompanied by their known distribution and a guide to the pertinent literature for the species. New records of 19 of the 45 species are listed. The transversely-dividing flabellids range from the Middle Eocene to the Recent at depths of 2-3010 m, and constitute 60% of the 65 known extant species of transversely-dividing Scleractinia. C1 [Cairns, Stephen D.] Natl Museum Nat Hist, Dept Invertebrate Zool, Smithsonian Inst, Washington, DC 20560 USA. RP Cairns, SD (reprint author), Natl Museum Nat Hist, Dept Invertebrate Zool, Smithsonian Inst, Washington, DC 20560 USA. EM cairnss@si.edu NR 70 TC 1 Z9 1 U1 1 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 562 BP 1 EP 48 DI 10.3897/zookeys.562.7310 PG 48 WC Zoology SC Zoology GA DD5LE UT WOS:000369964400001 PM 27006620 ER PT J AU Whelan, NV Strong, EE AF Whelan, Nathan V. Strong, Ellen E. TI Morphology, molecules and taxonomy: extreme incongruence in pleurocerids (Gastropoda, Cerithioidea, Pleuroceridae) SO ZOOLOGICA SCRIPTA LA English DT Article ID POTOMAC HORSE FEVER; FRESH-WATER SNAIL; MITOCHONDRIAL-DNA PHYLOGEOGRAPHY; EHRLICHIA-RISTICII; PHYLOGENETIC ANALYSIS; ECOPHENOTYPIC PLASTICITY; GENETIC DIFFERENTIATION; EVOLUTIONARY HISTORY; LITHASIA GASTROPODA; POPULATION-GROWTH AB Pronounced mitochondrial heterogeneity within putative species of Pleuroceridae has prevented meaningful systematic revisions of this critically imperilled freshwater family. Previous studies have demonstrated that this mitochondrial diversity often produces polyphyletic species on mitochondrial gene trees, but its significance is unclear. Hypotheses advanced to explain this pattern have included cryptic species, retained ancestral polymorphisms and introgression; other possible explanations such as doubly uniparental inheritance or the presence of pseudogenes have not been given due consideration. Previous analyses have not included adequate sampling, neither in terms of number of individuals nor in geographic coverage, to adequately test any of these hypotheses. To fully characterize mitochondrial heterogeneity in pleurocerids and robustly assess possible causal explanations, we collected 239 individuals representing four putative species from seven sites and sequenced the COI and 16S rRNA mitochondrial genes and the H3 nuclear gene for all individuals. We also used whole-genome shotgun sequencing to construct and annotate a mitochondrial genome for one individual. Characters with demonstrated utility in morphospecies delineation of gastropods (head-foot coloration, shell and radular morphology, pallial oviduct anatomy) were examined for a subset of individuals to determine whether morphology co-varied by haplotype clade. We found pronounced mitochondrial heterogeneity at both the population level and species level in three of the species examined, but our data reject paralogous nuclear copies of mitochondrial genes (NUMTs) and doubly uniparental inheritance as causal mechanisms, and there was no evidence of cryptic diversity. Mutation rates were found to differ significantly among mitochondrial lineages, and population genetic statistics revealed a signature of balancing selection that could be acting to maintain this diversity. The observed pattern is similar to that seen in lineages with inherited endosymbionts like Wolbachia infections, which merits further investigation. Although questions remain concerning the precise cause(s) of intraspecific mitochondrial diversity in pleurocerids, nuclear and/or genomic data, combined with anatomical and life history investigations in an integrative phylogenetic context, is the most promising avenue for resolving pleurocerid systematics. C1 [Whelan, Nathan V.] Univ Alabama, Dept Biol Sci, Box 870345, Tuscaloosa, AL 35487 USA. [Whelan, Nathan V.] Auburn Univ, Dept Biol Sci, 101 Life Sci Bldg, Auburn, AL 36849 USA. [Strong, Ellen E.] Natl Museum Nat Hist, Dept Invertebrate Zool, Smithsonian Inst, POB 37012,MRC 163, Washington, DC 20013 USA. RP Whelan, NV (reprint author), Univ Alabama, Dept Biol Sci, Box 870345, Tuscaloosa, AL 35487 USA. EM nwhelan@auburn.edu; StrongE@si.edu OI Whelan, Nathan/0000-0002-3542-2102 FU Birmingham Audubon Society; American Malacological Society; Conchologists of America; Smithsonian Institution predoctoral fellowship; National Science Foundation DDIG [DEB-1110638] FX P.D. Johnson, J.T. Garner (Alabama Department of Conservation and Natural Resources), E. Hartfield (Oregon State University) and E. Toso helped collect snails. P.M. Harris (University of Alabama), D.L. Graf (University of Wisconsin-Stevens Point) and B.L. Fluker (Arkansas State University) provided discussions that improved this manuscript. D. Schneider aided with GIS. We are grateful to R. Turner and A. Windsor (Laboratories of Analytical Biology, USNM) for generating the COI, 16S and H3 sequences, and to Vanessa Gonzalez (LAB, USNM) for producing the mitochondrial genome and preliminary annotations. Four anonymous reviewers provided helpful comments to improve this manuscript. This work was made possible in part by a grant of high-performance computing resources and technical support from the Alabama Supercomputer Authority. The Birmingham Audubon Society, American Malacological Society, Conchologists of America, a Smithsonian Institution predoctoral fellowship to NVW, and a National Science Foundation DDIG (award DEB-1110638 to NVW) provided funding for non-computing aspects of this study. Sampling was completed under respective state permits, federal permit TE130300 and a United States Fish and Wildlife Service Section 6 agreement with the Alabama Department of Conservation and Natural Resources. NR 105 TC 2 Z9 2 U1 3 U2 14 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0300-3256 EI 1463-6409 J9 ZOOL SCR JI Zool. Scr. PD JAN PY 2016 VL 45 IS 1 BP 62 EP 87 DI 10.1111/zsc.12139 PG 26 WC Evolutionary Biology; Zoology SC Evolutionary Biology; Zoology GA DD7AG UT WOS:000370075400006 ER PT J AU Somgird, C Homkong, P Sripiboon, S Brown, JL Stout, TAE Colenbrander, B Mahasawangkul, S Thitaram, C AF Somgird, Chaleamchat Homkong, Pongpon Sripiboon, Supaphen Brown, Janine L. Stout, Tom A. E. Colenbrander, Ben Mahasawangkul, Sittidet Thitaram, Chatchote TI Potential of a gonadotropin-releasing hormone vaccine to suppress musth in captive male Asian elephants (Elephas maximus) SO ANIMAL REPRODUCTION SCIENCE LA English DT Article DE Asian elephant (Elephas maximus); GnRH vaccine; GnRH antibody titer; Musth; Testosterone; LH ID FEMALE AFRICAN ELEPHANTS; LOXODONTA-AFRICANA; SERUM TESTOSTERONE; COMPARATIVE ENDOCRINOLOGY; NONINVASIVE ASSESSMENT; LUTEINIZING-HORMONE; OVARIAN CYCLICITY; BULL; GNRH; BEHAVIOR AB Musth in adult bull elephants is a period of increased androgen concentrations ranging from a few weeks to several months. For captive elephant bull management, musth presents a serious challenge because of the aggressive behavior of musth bulls toward people and other elephants. Commercially available GnRH vaccines have been shown to suppress testicular function by interrupting the hypothalamo-pituitary-gonadal (HPG) axis in many species. The aim of this study was to test the efficacy of a GnRH vaccine in elephant bulls for suppressing the HPG axis and mitigating musth-related aggressive behavior. Five adult Asian elephant bulls (22-55 years old) were immunized with a GnRH vaccine starting with an initial injection 2-4 months before the predicted musth period, and followed by three boosters at approximately 4-week intervals. Blood samples were collected twice weekly for hormone and antibody titer analysis. An increase in GnRH antibody titers was observed in all bulls after the second or third booster, and titers remained elevated for 2-3 months after the final booster. Musth was attenuated and shortened in three bulls and postponed completely in two. We conclude that GnRH vaccination is capable of suppressing symptoms of musth in adult bull elephants. With appropriate timing, GnRH vaccination could be used to control or manage musth and aggressive behavior in captive elephant bulls. However, more work is needed to identify an optimal dose, booster interval, and vaccination schedule for complete suppression of testicular steroidogenesis. (C) 2015 Elsevier B.V. All rights reserved. C1 [Somgird, Chaleamchat; Thitaram, Chatchote] Chiang Mai Univ, Fac Vet Med, Chiang Mai 50100, Thailand. [Somgird, Chaleamchat; Sripiboon, Supaphen; Thitaram, Chatchote] Chiang Mai Univ, Ctr Excellence Elephant Res & Educ, Chiang Mai 50200, Thailand. [Homkong, Pongpon; Mahasawangkul, Sittidet] Forest Ind Org, Natl Elephant Inst, Thai Elephant Conservat Ctr, Lampang 52190, Thailand. [Brown, Janine L.] Smithsonian Inst, Smithsonian Conservat Biol Inst, Front Royal, VA 22630 USA. [Stout, Tom A. E.; Colenbrander, Ben] Univ Utrecht, Fac Vet Med, Yalelaan 112, NL-3854 CM Utrecht, Netherlands. [Stout, Tom A. E.] Univ Pretoria, Fac Vet Sci, ZA-0002 Pretoria, South Africa. [Homkong, Pongpon] Chiang Mai Municipal, Dept Publ Hlth & Environm, Vet Sect, Muang Chiang Mai 50100, Thailand. [Sripiboon, Supaphen] Kasetsart Univ, Fac Vet Med, Kamphaeng Saen Campus, Nakhon Pathom 73140, Thailand. RP Somgird, C (reprint author), Chiang Mai Univ, Fac Vet Med, Chiang Mai 50100, Thailand. EM chaleamchat.s@cmu.ac.th; chatchote.thitaram@cmu.ac.th FU National Research Council of Thailand (NRCT); Royal Thai Government scholarship; Asia-Link Programme, Europe-aid Co-operation Office; Elephant Hill; Elephant Nature Park; National Elephant Institute FX We would like to thank the National Research Council of Thailand (NRCT), Royal Thai Government scholarship and the Asia-Link Programme, Europe-aid Co-operation Office for providing research funding. Elephant Hill, Elephant Nature Park, and the National Elephant Institute for co-operating in and supporting this study, Miss Chawewan Nhuthong, Dr. Prasit Moleechai, and the mahouts for taking care of the elephants and their kind help. NR 56 TC 0 Z9 0 U1 8 U2 18 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0378-4320 EI 1873-2232 J9 ANIM REPROD SCI JI Anim. Reprod. Sci. PD JAN PY 2016 VL 164 BP 111 EP 120 DI 10.1016/j.anireprosci.2015.11.019 PG 10 WC Agriculture, Dairy & Animal Science; Reproductive Biology SC Agriculture; Reproductive Biology GA DC9TC UT WOS:000369562900015 PM 26656504 ER PT J AU Imara, N Loeb, A AF Imara, N. Loeb, A. TI LIMITS ON INTERGALACTIC DUST DURING REIONIZATION SO ASTROPHYSICAL JOURNAL LETTERS LA English DT Article DE dark ages, reionization, first stars; dust, extinction; galaxies: high-redshift; intergalactic medium ID INTERSTELLAR DUST; METAL ENRICHMENT; COSMOLOGICAL SIMULATIONS; GALAXIES; METALLICITY; ABSORPTION; CONSTRAINTS; SUPERNOVA; EVOLUTION; CLUSTERS AB In this Letter, we constrain the dust-to-gas ratio in the intergalactic medium (IGM) at high redshifts. We employ models for dust in the local universe to constrain the dust-to-gas ratio during the epoch of reionization at redshifts z similar to 6-10. The observed level of reddening of high redshift galaxies implies that the IGM was enriched to an intergalactic dust-to-gas ratio of less than 3% of the Milky Way value by a redshift of z = 10. C1 [Imara, N.; Loeb, A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. RP Imara, N (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM nimara@cfa.harvard.edu FU NSF [AST-1312034]; Harvard-MIT FFL Postdoctoral Fellowship FX We thank Anastasia Fialkov, Pascal Oesch, and Steven Furlanetto for their helpful comments on the paper. We also thank an anonymous referee whose suggestions helped to improve this paper. This work was supported in part by NSF grant AST-1312034. N.I. acknowledges the support of the Harvard-MIT FFL Postdoctoral Fellowship. NR 34 TC 1 Z9 1 U1 0 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 2041-8205 EI 2041-8213 J9 ASTROPHYS J LETT JI Astrophys. J. Lett. PD JAN 1 PY 2016 VL 816 IS 1 AR L16 DI 10.3847/2041-8205/816/1/L16 PG 5 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC7AE UT WOS:000369369900016 ER PT J AU Simionescu, A Stawarz, L Ichinohe, Y Cheung, CC Jamrozy, M Siemiginowska, A Hagino, K Gandhi, P Werner, N AF Simionescu, A. Stawarz, L. Ichinohe, Y. Cheung, C. C. Jamrozy, M. Siemiginowska, A. Hagino, K. Gandhi, P. Werner, N. TI SERENDIPITOUS DISCOVERY OF AN EXTENDED X-RAY JET WITHOUT A RADIO COUNTERPART IN A HIGH-REDSHIFT QUASAR SO ASTROPHYSICAL JOURNAL LETTERS LA English DT Article DE galaxies: active; galaxies: jets; quasars: individual (B3 0727+409); radiation mechanisms: non-thermal; radio continuum: galaxies; X-rays: general ID ACTIVE GALACTIC NUCLEI; SCALE JETS; EMISSION; CHANDRA; Z=4.3; GB-1508+5714; EVOLUTION AB A recent Chandra observation of the nearby galaxy cluster Abell 585 has led to the discovery of an extended X-ray jet associated with the high-redshift background quasar B3 0727+ 409, a luminous radio source at redshift z = 2.5. This is one of only few examples of high-redshift X-ray jets known to date. It has a clear extension of about 12", corresponding to a projected length of similar to 100 kpc, with a possible hot spot located 35" from the quasar. The archival high resolution Very Large Array maps surprisingly reveal no extended jet emission, except for one knot about 1"4 from the quasar. The high X-ray to radio luminosity ratio for this source appears consistent with the alpha(1 + z)(4) amplification expected from the inverse Compton radiative model. This serendipitous discovery may signal the existence of an entire population of similar systems with bright X-ray and faint radio jets at high redshift, a selection bias that must be accounted for when drawing any conclusions about the redshift evolution of jet properties and indeed about the cosmological evolution of supermassive black holes and active galactic nuclei in general. C1 [Simionescu, A.; Ichinohe, Y.; Hagino, K.] JAXA, ISAS, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan. [Stawarz, L.; Jamrozy, M.] Jagiellonian Univ, Astron Observ, Ul Orla 171, PL-30244 Krakow, Poland. [Ichinohe, Y.] Univ Tokyo, Grad Sch Sci, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan. [Cheung, C. C.] Naval Res Lab, Div Space Sci, Washington, DC 20375 USA. [Siemiginowska, A.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Gandhi, P.] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England. [Werner, N.] Stanford Univ, KIPAC, 452 Lomita Mall, Stanford, CA 94305 USA. [Werner, N.] Stanford Univ, Dept Phys, 382 Via Pueblo Mall, Stanford, CA 94305 USA. RP Simionescu, A (reprint author), JAXA, ISAS, Chuo Ku, 3-1-1 Yoshinodai, Sagamihara, Kanagawa 2525210, Japan. OI , kouichi/0000-0003-4235-5304 FU Polish NSC [DEC-2012/04/A/ST9/00083, DEC-2013/09/B/ST9/00599]; NASA [DPR S-15633-Y, NAS8-03060, GO5-16127X] FX L.S. and M.J. were supported by Polish NSC grants DEC-2012/04/A/ST9/00083 and DEC-2013/09/B/ST9/00599, respectively. Y.I. acknowledges a Grant-in-Aid for Japan Society for the Promotion of Science (JSPS) Fellows. C.C.C. was supported at NRL by NASA DPR S-15633-Y. A. Siemiginowska was supported by NASA contract NAS8-03060 to the Chandra X-ray Center. N.W. acknowledges NASA grant GO5-16127X. NR 25 TC 2 Z9 2 U1 0 U2 2 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 2041-8205 EI 2041-8213 J9 ASTROPHYS J LETT JI Astrophys. J. Lett. PD JAN 1 PY 2016 VL 816 IS 1 AR L15 DI 10.3847/2041-8205/816/1/L15 PG 5 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC7AE UT WOS:000369369900015 ER PT J AU Toloba, E Sand, DJ Spekkens, K Crnojevic, D Simon, JD Guhathakurta, P Strader, J Caldwell, N McLeod, B Seth, AC AF Toloba, Elisa Sand, David J. Spekkens, Kristine Crnojevic, Denija Simon, Joshua D. Guhathakurta, Puragra Strader, Jay Caldwell, Nelson McLeod, Brian Seth, Anil C. TI A TIDALLY DISRUPTING DWARF GALAXY IN THE HALO OF NGC 253 SO ASTROPHYSICAL JOURNAL LETTERS LA English DT Article DE galaxies: dwarf; galaxies: halos; galaxies: individual (NGC 253); galaxies: photometry; galaxies: stellar content ID MILKY-WAY SATELLITE; DIGITAL SKY SURVEY; GIANT BRANCH STARS; SPHEROIDAL GALAXIES; DIFFUSE GALAXIES; LOCAL GROUP; 3-PI SURVEY; M81 GROUP; FAINT; DISCOVERY AB We report the discovery of Scl-MM-Dw2, a new dwarf galaxy at a projected separation of similar to 50 kpc from NGC 253, as part of the Panoramic Imaging Survey of Centaurus and Sculptor project (PISCeS). We measure a tip of the red giant branch (RGB) distance of 3.12. +/- 0.30 Mpc, suggesting that Scl-MM-Dw2 is likely a satellite of NGC 253. We qualitatively compare the distribution of RGB stars in the color-magnitude diagram with theoretical isochrones and find that it is consistent with an old, similar to 12 Gyr, and metal-poor, -2.3 < [Fe/H]. < -1.1, stellar population. We also detect a small number of asymptotic giant branch stars consistent with a metal-poor 2-3 Gyr population in the center of the dwarf. Our non-detection of HI in a deep Green Bank Telescope spectrum implies a gas fractionM(HI)/L-V < 0.02M(circle dot) L-circle dot. The stellar and gaseous properties of Scl-MM-Dw2 suggest that it is a dwarf spheroidal galaxy. Scl-MM-Dw2 has a luminosity of M-V = -12.1 +/- 0.5 mag and a half-light radius of r(h) = 2.94 +/- 0.46 kpc, which makes it moderately larger than dwarf galaxies in the Local Group of the same luminosity. However, Scl-MM-Dw2 is very elongated (epsilon= 0.66 +/- 0.06), and it has an extremely low surface brightness (mu(0,V) = 27.7 +/- 0.6 mag arcsec(-2)). Its elongation and diffuseness make it an outlier in the ellipticity-luminosity and surface brightness-luminosity scaling relations. These properties suggest that this dwarf is being tidally disrupted by NGC 253. C1 [Toloba, Elisa; Sand, David J.; Crnojevic, Denija] Texas Tech Univ, Dept Phys, Box 41051, Lubbock, TX 79409 USA. [Toloba, Elisa; Guhathakurta, Puragra] Univ Calif Santa Cruz, UCO Lick Observ, 1156 High St, Santa Cruz, CA 95064 USA. [Spekkens, Kristine] Royal Mil Coll Canada, Dept Phys, POB 17000, Kingston, ON K7L 7B4, Canada. [Simon, Joshua D.] Carnegie Observ, 813 Santa Barbara St, Pasadena, CA 91101 USA. [Strader, Jay] Michigan State Univ, Dept Phys & Astron, E Lansing, MI 48824 USA. [Caldwell, Nelson; McLeod, Brian] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Seth, Anil C.] Univ Utah, Dept Phys & Astron, Salt Lake City, UT 84112 USA. RP Toloba, E (reprint author), Texas Tech Univ, Dept Phys, Box 41051, Lubbock, TX 79409 USA.; Toloba, E (reprint author), Univ Calif Santa Cruz, UCO Lick Observ, 1156 High St, Santa Cruz, CA 95064 USA. EM toloba@ucolick.org OI Seth, Anil/0000-0003-0248-5470 FU NSF [AST-1412504, AST-1010039, AST-1517649]; Natural Sciences and Engineering Research Council of Canada (NSERC) FX E.T., D.J.S, J.D.S., and P.G. acknowledge the NSF grant AST-1412504. E.T. and P.G. are also supported by NSF grant AST-1010039 and D.J.S. by AST-1517649. K.S. acknowledges support from the Natural Sciences and Engineering Research Council of Canada (NSERC). NR 51 TC 7 Z9 7 U1 1 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 2041-8205 EI 2041-8213 J9 ASTROPHYS J LETT JI Astrophys. J. Lett. PD JAN 1 PY 2016 VL 816 IS 1 AR L5 DI 10.3847/2041-8205/816/1/L5 PG 6 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC7AE UT WOS:000369369900005 ER PT J AU Wiggins, NL Forrister, DL Endara, MJ Coley, PD Kursar, TA AF Wiggins, Natasha L. Forrister, Dale L. Endara, Maria-Jose Coley, Phyllis D. Kursar, Thomas A. TI Quantitative and qualitative shifts in defensive metabolites define chemical defense investment during leaf development in Inga, a genus of tropical trees SO ECOLOGY AND EVOLUTION LA English DT Article DE Foliar chemistry; Inga; leaf development; metabolomics; plant defense traits; secondary metabolites ID PLANT DEFENSE; YOUNG LEAVES; ANTIHERBIVORE DEFENSES; HERBIVORY; DIVERSITY; SECONDARY; EVOLUTION; AVAILABILITY; STRATEGIES; CHEMISTRY AB Selective pressures imposed by herbivores are often positively correlated with investments that plants make in defense. Research based on the framework of an evolutionary arms race has improved our understanding of why the amount and types of defenses differ between plant species. However, plant species are exposed to different selective pressures during the life of a leaf, such that expanding leaves suffer more damage from herbivores and pathogens than mature leaves. We hypothesize that this differential selective pressure may result in contrasting quantitative and qualitative defense investment in plants exposed to natural selective pressures in the field. To characterize shifts in chemical defenses, we chose six species of Inga, a speciose Neotropical tree genus. Focal species represent diverse chemical, morphological, and developmental defense traits and were collected from a single site in the Amazonian rainforest. Chemical defenses were measured gravimetrically and by characterizing the metabolome of expanding and mature leaves. Quantitative investment in phenolics plus saponins, the major classes of chemical defenses identified in Inga, was greater for expanding than mature leaves (46% and 24% of dry weight, respectively). This supports the theory that, because expanding leaves are under greater selective pressure from herbivores, they rely more upon chemical defense as an antiherbivore strategy than do mature leaves. Qualitatively, mature and expanding leaves were distinct and mature leaves contained more total and unique metabolites. Intraspecific variation was greater for mature leaves than expanding leaves, suggesting that leaf development is canalized. This study provides a snapshot of chemical defense investment in a speciose genus of tropical trees during the short, few-week period of leaf development. Exploring the metabolome through quantitative and qualitative profiling enables a more comprehensive examination of foliar chemical defense investment. C1 [Wiggins, Natasha L.; Forrister, Dale L.; Endara, Maria-Jose; Coley, Phyllis D.; Kursar, Thomas A.] Univ Utah, Dept Biol, Salt Lake City, UT 84112 USA. [Wiggins, Natasha L.] Univ Tasmania, Sch Biol Sci, Private Bag 5, Hobart, Tas 7001, Australia. [Coley, Phyllis D.; Kursar, Thomas A.] Smithsonian Trop Res Inst, Balboa, Panama. RP Wiggins, NL (reprint author), Univ Tasmania, Sch Biol Sci, Private Bag 5, Hobart, Tas 7001, Australia. EM wigginsn@utas.edu.au FU Directorate for Biological Sciences [DEB-1135733] FX Directorate for Biological Sciences, (Grant/Award Number: DEB-1135733). NR 73 TC 3 Z9 3 U1 10 U2 26 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 2045-7758 J9 ECOL EVOL JI Ecol. Evol. PD JAN PY 2016 VL 6 IS 2 BP 478 EP 492 DI 10.1002/ece3.1896 PG 15 WC Ecology; Evolutionary Biology SC Environmental Sciences & Ecology; Evolutionary Biology GA DC4BJ UT WOS:000369164400008 PM 26843932 ER PT J AU Zhang, KM Shen, Y Fang, YM Liu, Y AF Zhang, Kai-Mei Shen, Yu Fang, Yan-Ming Liu, Ying TI Changes in gametophyte physiology of Pteris multifida induced by the leaf leachate treatment of the invasive Bidens pilosa SO ENVIRONMENTAL SCIENCE AND POLLUTION RESEARCH LA English DT Article DE Pteris multifida; Gametophyte; Bidens pilosa; allelopathy ID INDUCED OXIDATIVE STRESS; AGERATINA-ADENOPHORA; SPORE GERMINATION; PLANT INVASION; VITTATA L; CYANOBACTERIA; INHIBITION; MECHANISM; IMPACTS; REVEALS AB In recent years, the response of fern gametophytes to environment has raised much attention. However, studies on the influence of plant invasion to fern gametophytes are scarce. Allelopathy plays an important role in biological invasion. Hence, it is necessary to study the allelopathic effects of invasive plants on fern gametophytes and elucidate the mechanisms by which invasive plants cause phytotoxicity. As one of the main invasive plants in China, Bidens pilosa exhibits allelopathic effects on spermatophyte growth. Field investigation shows that many ferns are threatened by the invasion of B. pilosa. The distribution of Pteris multifida overlaps with that of B. pilosa in China. To examine the potential involvement of allelopathic mechanisms of B. pilosa leaves, changes in the physiology in P. multifida gametophytes are analyzed. We found that cell membrane and antioxidant enzyme activities as well as photosynthesis pigment contents of the gametophytes were affected by B. pilosa leachates. Gametophytes of P. multifida exposed to B. pilosa had increased damages to cell membranes, expressed in thiobarbituric acid reacting substance (TBARS) concentrations, malondialdehyde (MDA), electrolyte leakage (membrane permeability), and degree of injury. Enzyme activities, assessed by superoxide dismutase (SOD) and catalase (CAT) as well as guaiacol peroxidase (GPX) enhanced with the increase in leachate concentration after 2-day exposure. Meanwhile, lower chlorophyll a (Chl a), chlorophyll b (Chl b), carotenoid (Car), and the total chlorophyll were measured as leachate concentrations increased. At day 10, leaf leachates of B. pilosa exhibited the greatest inhibition. These results suggest that the observed inhibitory or stimulatory effects on the physiology studied can have an adverse effect on P. multifida and that allelopathic interference seems to have involved in this process. C1 [Zhang, Kai-Mei; Shen, Yu; Fang, Yan-Ming; Liu, Ying] Nanjing Forestry Univ, Coinnovat Ctr Sustainable Forestry Southern China, Nanjing 210037, Jiangsu, Peoples R China. [Zhang, Kai-Mei; Shen, Yu; Fang, Yan-Ming; Liu, Ying] Nanjing Forestry Univ, Coll Biol & Environm, Nanjing 210037, Jiangsu, Peoples R China. [Zhang, Kai-Mei] Smithsonian Inst, Dept Bot, Washington, DC 20013 USA. [Shen, Yu] Nanjing Agr Univ, Coll Resources & Environm Sci, Nanjing 210095, Jiangsu, Peoples R China. RP Fang, YM (reprint author), Nanjing Forestry Univ, Coinnovat Ctr Sustainable Forestry Southern China, Nanjing 210037, Jiangsu, Peoples R China.; Fang, YM (reprint author), Nanjing Forestry Univ, Coll Biol & Environm, Nanjing 210037, Jiangsu, Peoples R China. EM jwu4@njfu.edu.cn FU National Natural Science Foundation of China [31200233]; Priority Academic Program Development of Jiangsu Higher Education Institutions (PAPD); Collaborative Innovation Plan of Jiangsu Higher Education; Jiangsu Government Scholarship for Overseas Studies; Laboratories of Analytical Biology of the National Museum of Natural History, the Smithsonian Institution FX This work was supported by the National Natural Science Foundation of China (31200233), the Priority Academic Program Development of Jiangsu Higher Education Institutions (PAPD), Collaborative Innovation Plan of Jiangsu Higher Education, the Jiangsu Government Scholarship for Overseas Studies, and the Laboratories of Analytical Biology of the National Museum of Natural History, the Smithsonian Institution. NR 30 TC 1 Z9 1 U1 5 U2 17 PU SPRINGER HEIDELBERG PI HEIDELBERG PA TIERGARTENSTRASSE 17, D-69121 HEIDELBERG, GERMANY SN 0944-1344 EI 1614-7499 J9 ENVIRON SCI POLLUT R JI Environ. Sci. Pollut. Res. PD JAN PY 2016 VL 23 IS 4 BP 3578 EP 3585 DI 10.1007/s11356-015-5589-x PG 8 WC Environmental Sciences SC Environmental Sciences & Ecology GA DC6PP UT WOS:000369342400059 PM 26490937 ER PT J AU Tichenor, HR Culver, SJ Corbett, DR Walsh, JP Buzas, MA AF Tichenor, Hal R. Culver, Stephen J. Corbett, D. Reide Walsh, John P. Buzas, Martin A. TI DOES THE PEB INDEX RESPOND ONLY TO HYPOXIA IN THE MISSISSIPPI DELTA, GULF OF MEXICO? SO JOURNAL OF FORAMINIFERAL RESEARCH LA English DT Article ID LOUISIANA CONTINENTAL-SHELF; NORTHERN ADRIATIC SEA; BENTHIC FORAMINIFERA; OXYGEN DEPLETION; RIVER DELTA; COASTAL EUTROPHICATION; HISTORICAL TRENDS; SEASONAL HYPOXIA; DEEP-SEA; BAY AB The frequency of anthropogenic seasonal hypoxia on the continental shelf west of the Mississippi Delta (the Louisiana Bight) has increased since the middle of the 20th century. This study applies the PEB index, a proxy for hypoxia, to four similar to 2 m kasten cores taken southwest of Southwest Pass of the Mississippi Delta. The PEB index is defined as the cumulative percent of Protononion atlanticum ( = Nonionella atlantica of this study), Nonionella opima, Epistominella vitrea and Buliminella morgani. The PEB index varies little in the shallowest core, KC4 (59 m water depth). Assemblages were strongly dominated by PEB taxa (average 95%), due mainly to the dominance of E. vitrea (average 76%). In core KC3 (75 m), an average PEB value of 84% is also due mainly to E. vitrea (61%). The PEB index of KC3 was consistently higher above 90 cm, a level dated at 1955-1960 (Pb-210 age estimate), and could reflect an increased influence of hypoxia or an increased rate of sediment accumulation associated with delta progradation. A similar trend characterizes core KC2 (87 m). The PEB index is 18% from 240 cm to 140 cm, increasing up core as the abundance of E. vitrea increases, likely due to delta progradation. Other PEB taxa, B. morgani and N. opima, increase in the top 30 cm of the core, probably due to increased hypoxia between 1952 and 1968 (Pb-210 age estimate). Core KC1 (473 m) differed from shallower cores in its higher species diversity. Bolivina lowmani, Cassidulina neocarinata, and Bolivina ordinaria each comprise similar to 15% of assemblages and PEB taxa are rare (average 5%) but increase to 19% in a 30 cm interval attributed to off-shelf transport. We conclude that the PEB index is a useful indicator of anthropogenic hypoxia but dominance of E. vitrea may also be attributable to sedimentological factors related to delta progradation. C1 [Tichenor, Hal R.; Culver, Stephen J.; Corbett, D. Reide; Walsh, John P.] E Carolina Univ, Dept Geol Sci, Greenville, NC 27858 USA. [Buzas, Martin A.] Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol, Washington, DC 20560 USA. RP Culver, SJ (reprint author), E Carolina Univ, Dept Geol Sci, Greenville, NC 27858 USA. EM culvers@ecu.edu FU American Chemical Society (Petroleum Research Found) [49560-ND8]; National Science Foundation [OCE-0841092, OCE-0452166] FX Acknowledgment is made to the donors of the American Chemical Society (Petroleum Research Found award 49560-ND8) for support of this research. Cores were collected under National Science Foundation awards OCE-0841092 and OCE-0452166. Katrina Rabien, Sarah Hardison, Anna Lee Woodson and Caitlin Lauback provided support in the laboratory. Reviews by C. Wylie Poag and Lisa Osterman were very useful. NR 102 TC 0 Z9 0 U1 1 U2 3 PU CUSHMAN FOUNDATION FORAMINIFERAL RES PI CAMBRIDGE PA MUSEUM COMPARATIVE ZOOLOGY, DEPT INVERTEBRATE PALEONTOLOGY 26 OXFORD ST, HARVARD UNIV, CAMBRIDGE, MA 02138 USA SN 0096-1191 J9 J FORAMIN RES JI J. Foraminifer. Res. PD JAN PY 2016 VL 46 IS 1 BP 48 EP 60 PG 13 WC Paleontology SC Paleontology GA DC8KK UT WOS:000369468200007 ER PT J AU Robinson, H Yankowski, S AF Robinson, Harold Yankowski, Stanley TI The Taxonomic Significance of ducts in the corolla lobes of Vernonia (Vernonieae: Asteraceae) SO PHYTOKEYS LA English DT Article DE Ducts; corolla lobes; Vernonia; Vernonanthura; Trepadonia ID PLANT MATERIAL AB The multiple longitudinal ducts in the corolla lobes found in the closely related genera Vernonia, Vernonanthura and Trepadonia are microscopically studied and illustrated. The lack of such ducts in the two South American species that have until now been retained in Vernonia indicates that they should probably be excluded from the genus. C1 [Robinson, Harold; Yankowski, Stanley] Smithsonian Inst, Dept Bot, NMNH, MRC 166,POB 37012, Washington, DC 20013 USA. RP Robinson, H (reprint author), Smithsonian Inst, Dept Bot, NMNH, MRC 166,POB 37012, Washington, DC 20013 USA. EM robinsoh@si.edu NR 12 TC 0 Z9 0 U1 0 U2 0 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 58 BP 1 EP 7 DI 10.3897/phytokeys.58.7009 PG 7 WC Plant Sciences SC Plant Sciences GA DC6WQ UT WOS:000369360700001 ER PT J AU Costion, CM Plunkett, GM AF Costion, Craig M. Plunkett, Gregory M. TI A revision of the genus Osmoxylon (Araliaceae) in Palau, including two new species SO PHYTOKEYS LA English DT Article DE Pacific Islands; taxonomy; Asteriids; Apiales AB Osmoxylon Miq. (Araliaceae) is revised for Palau, Micronesia including descriptions of two new taxa Osmoxylon leidichii Costion, sp. nov. and Osmoxylon ngardokense Costion, sp. nov. Full descriptions are provided for all four Palau species, along with diagnostic field keys. C1 [Costion, Craig M.] Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, POB 37012, Washington, DC 20013 USA. [Plunkett, Gregory M.] New York Bot Garden, Cullman Program Mol Systemat, 2900 Southern Blvd, Bronx, NY 10458 USA. RP Costion, CM (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Bot, POB 37012, Washington, DC 20013 USA. EM costionc@si.edu FU Institute of Pacific Islands Forestry, US Forest Service FX This work was made possible through the funding of the Institute of Pacific Islands Forestry, US Forest Service. We would like to especially also thank Susan Cordell, Christian Giardina, Julian Dendy, Kevin Mesebeluu, Lori Colin, Misako Mishima at the Kyushu University Museum herbarium, Ron Leidich, Palau Forestry, the Ngardok Nature Reserve, Melekeok State, Ann Kitalong, the Belau National Museum, the Coral Reef Research Foundation of Palau, Michael Balick, and the National Geographic Society. NR 12 TC 0 Z9 0 U1 0 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 58 BP 49 EP 64 DI 10.3897/phytokeys.58.5292 PG 16 WC Plant Sciences SC Plant Sciences GA DC6WQ UT WOS:000369360700004 ER PT J AU Appelhans, MS Wen, J AF Appelhans, Marc S. Wen, Jun TI On the identity of Blanco's Cissus frutescens and its correct name in Melicope (Rutaceae) with neotypification of Cissus arborea Blanco SO PHYTOKEYS LA English DT Article DE Blanco; Cissus; Melicope confusa; Melicope frutescens; Nomenclature; Philippines; Rutaceae; Vitaceae ID COMBINATIONS AB The names Cissus frutescens and C. arborea have a long history of confusion. Cissus frutescens Blanco belongs to the genus Melicope (Rutaceae) and we herein correct a nomenclatural mistake made by T.G. Hartley in the revision of Melicope. The name Melicope confusa (Merr.) P.S. Liu was accepted for this taxon by Hartley. However, Cissus frutescens Blanco represents the earliest name for this entity and a new combination, Melicope frutescens (Blanco) Appelhans & J.Wen is herein proposed. Neotypification of Cissus arborea Blanco is also provided. C1 [Appelhans, Marc S.] Univ Gottingen, Albrecht von Haller Inst Plant Sci, Dept Systemat Bot, Untere Karspule 2, D-37073 Gottingen, Germany. [Appelhans, Marc S.; Wen, Jun] Smithsonian Inst, Dept Bot, POB 37012, Washington, DC 20013 USA. RP Appelhans, MS (reprint author), Univ Gottingen, Albrecht von Haller Inst Plant Sci, Dept Systemat Bot, Untere Karspule 2, D-37073 Gottingen, Germany.; Appelhans, MS (reprint author), Smithsonian Inst, Dept Bot, POB 37012, Washington, DC 20013 USA. EM Marc.Appelhans@biologie.uni-goettingen.de FU Open Access Publication Funds of Gottingen University FX We thank Sue Lutz for her assistance with obtaining relevant publications, the curators of A for providing a high-resolution image of the specimen Merrill 904, Warren Wagner, Larry Dorr and John Boggan for their suggestions, and Pedro Acevedo for his detailed edits of the manuscript. We acknowledge support by the Open Access Publication Funds of Gottingen University. NR 15 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 58 BP 81 EP 85 DI 10.3897/phytokeys.58.5847 PG 5 WC Plant Sciences SC Plant Sciences GA DC6WQ UT WOS:000369360700006 ER PT J AU Brilhaus, D Brautigam, A Mettler-Altmann, T Winter, K Weber, APM AF Brilhaus, Dominik Braeutigam, Andrea Mettler-Altmann, Tabea Winter, Klaus Weber, Andreas P. M. TI Reversible Burst of Transcriptional Changes during Induction of Crassulacean Acid Metabolism in Talinum triangulare SO PLANT PHYSIOLOGY LA English DT Article ID PHOSPHOENOLPYRUVATE CARBOXYLASE KINASE; COMMON ICE PLANT; 2C PROTEIN PHOSPHATASES; ZINC-FINGER PROTEIN; MESEMBRYANTHEMUM-CRYSTALLINUM; ABSCISIC-ACID; ARABIDOPSIS-THALIANA; C-4 PHOTOSYNTHESIS; MESSENGER-RNA; ENZYMATIC CHARACTERISTICS AB Drought tolerance is a key factor for agriculture in the 21st century as it is a major determinant of plant survival in natural ecosystems as well as crop productivity. Plants have evolved a range of mechanisms to cope with drought, including a specialized type of photosynthesis termed Crassulacean acid metabolism(CAM). CAM is associated with stomatal closure during the day as atmospheric CO2 is assimilated primarily during the night, thus reducing transpirational water loss. The tropical herbaceous perennial species Talinum triangulare is capable of transitioning, in a facultative, reversible manner, from C-3 photosynthesis to weakly expressed CAM in response to drought stress. The transcriptional regulation of this transition has been studied. Combining mRNA-Seq with targeted metabolite measurements, we found highly elevated levels of CAM-cycle enzyme transcripts and their metabolic products in T. triangulare leaves upon water deprivation. The carbohydrate metabolism is rewired to reduce the use of reserves for growth to support the CAM-cycle and the synthesis of compatible solutes. This large-scale expression dataset of drought-induced CAM demonstrates transcriptional regulation of the C-3-CAM transition. We identified candidate transcription factors to mediate this photosynthetic plasticity, which may contribute in the future to the design of more drought-tolerant crops via engineered CAM. C1 [Brilhaus, Dominik; Braeutigam, Andrea; Mettler-Altmann, Tabea; Weber, Andreas P. M.] Univ Dusseldorf, Inst Plant Biochem, Cluster Excellence Plant Sci CEPLAS, D-40225 Dusseldorf, Germany. [Winter, Klaus] Smithsonian Trop Res Inst, Balboa, Ancon, Panama. RP Weber, APM (reprint author), Univ Dusseldorf, Inst Plant Biochem, Cluster Excellence Plant Sci CEPLAS, D-40225 Dusseldorf, Germany. EM andreas.weber@hhu.de RI Weber, Andreas/A-6250-2011; OI Weber, Andreas/0000-0003-0970-4672; Brilhaus, Dominik/0000-0001-9021-3197 FU International Graduate Program for Plant Science (iGRAD-Plant); Deutsche Forschungsgemeinschaft [EXC 1028, IRTG 1525]; Smithsonian Tropical Research Institute FX This work was supported by the International Graduate Program for Plant Science (iGRAD-Plant; to D.B.) and grants from Deutsche Forschungsgemeinschaft (EXC 1028; IRTG 1525 to A.P.M.W.). K.W. was supported by the Smithsonian Tropical Research Institute. NR 110 TC 3 Z9 3 U1 4 U2 23 PU AMER SOC PLANT BIOLOGISTS PI ROCKVILLE PA 15501 MONONA DRIVE, ROCKVILLE, MD 20855 USA SN 0032-0889 EI 1532-2548 J9 PLANT PHYSIOL JI Plant Physiol. PD JAN PY 2016 VL 170 IS 1 BP 102 EP 122 DI 10.1104/pp.15.01076 PG 21 WC Plant Sciences SC Plant Sciences GA DC6OB UT WOS:000369338300009 PM 26530316 ER PT J AU Ackermann, M Ajello, M Atwood, WB Baldini, L Ballet, J Barbiellini, G Bastieri, D Gonzalez, JB Bellazzini, R Bissaldi, E Blandford, RD Bloom, ED Bonino, R Bottacini, E Brandt, TJ Bregeon, J Bruel, P Buehler, R Buson, S Caliandro, GA Cameron, RA Caputo, R Caragiulo, M Caraveo, PA Cavazzuti, E Cecchi, C Charles, E Chekhtman, A Cheung, CC Chiang, J Chiaro, G Ciprini, S Cohen, JM Cohen-Tanugi, J Cominsky, LR Conrad, J Cuoco, A Cutini, S D'Ammando, F de Angelis, A de Palma, F Desiante, R Di Mauro, M Di Venere, L Dominguez, A Drell, PS Favuzzi, C Fegan, SJ Ferrara, EC Focke, WB Fortin, P Franckowiak, A Fukazawa, Y Funk, S Furniss, AK Fusco, P Gargano, F Gasparrini, D Giglietto, N Giommi, P Giordano, F Giroletti, M Glanzman, T Godfrey, G Grenier, IA Grondin, MH Guillemot, L Guiriec, S Harding, AK Hays, E Hewitt, JW Hill, AB Horan, D Iafrate, G Hartmann, D Jogler, T Johannesson, G Johnson, AS Kamae, T Kataoka, J Knodlseder, J Kuss, M La Mura, G Larsson, S Latronico, L Lemoine-Goumard, M Li, J Li, L Longo, F Loparco, F Lott, B Lovellette, MN Lubrano, P Madejski, GM Maldera, S Manfreda, A Mayer, M Mazziotta, MN Michelson, PF Mirabal, N Mitthumsiri, W Mizuno, T Moiseev, AA Monzani, ME Morselli, A Moskalenko, IV Murgia, S Nuss, E Ohsugi, T Omodei, N Orienti, M Orlando, E Ormes, JF Paneque, D Perkins, JS Pesce-Rollins, M Petrosian, V Piron, F Pivato, G Porter, TA Raino, S Rando, R Razzano, M Razzaque, S Reimer, A Reimer, O Reposeur, T Romani, RW Sanchez-Conde, M Parkinson, PMS Schmid, J Schulz, A Sgro, C Siskind, EJ Spada, F Spandre, G Spinelli, P Suson, DJ Tajima, H Takahashi, H Takahashi, M Takahashi, T Thayer, JB Thompson, DJ Tibaldo, L Torres, DF Tosti, G Troja, E Vianello, G Wood, KS Wood, M Yassine, M Zaharijas, G Zimmer, S AF Ackermann, M. Ajello, M. Atwood, W. B. Baldini, L. Ballet, J. Barbiellini, G. Bastieri, D. Gonzalez, J. Becerra Bellazzini, R. Bissaldi, E. Blandford, R. D. Bloom, E. D. Bonino, R. Bottacini, E. Brandt, T. J. Bregeon, J. Bruel, P. Buehler, R. Buson, S. Caliandro, G. A. Cameron, R. A. Caputo, R. Caragiulo, M. Caraveo, P. A. Cavazzuti, E. Cecchi, C. Charles, E. Chekhtman, A. Cheung, C. C. Chiang, J. Chiaro, G. Ciprini, S. Cohen, J. M. Cohen-Tanugi, J. Cominsky, L. R. Conrad, J. Cuoco, A. Cutini, S. D'Ammando, F. de Angelis, A. de Palma, F. Desiante, R. Di Mauro, M. Di Venere, L. Dominguez, A. Drell, P. S. Favuzzi, C. Fegan, S. J. Ferrara, E. C. Focke, W. B. Fortin, P. Franckowiak, A. Fukazawa, Y. Funk, S. Furniss, A. K. Fusco, P. Gargano, F. Gasparrini, D. Giglietto, N. Giommi, P. Giordano, F. Giroletti, M. Glanzman, T. Godfrey, G. Grenier, I. A. Grondin, M. -H. Guillemot, L. Guiriec, S. Harding, A. K. Hays, E. Hewitt, J. W. Hill, A. B. Horan, D. Iafrate, G. Hartmann, Dieter Jogler, T. Johannesson, G. Johnson, A. S. Kamae, T. Kataoka, J. Knoedlseder, J. Kuss, M. La Mura, G. Larsson, S. Latronico, L. Lemoine-Goumard, M. Li, J. Li, L. Longo, F. Loparco, F. Lott, B. Lovellette, M. N. Lubrano, P. Madejski, G. M. Maldera, S. Manfreda, A. Mayer, M. Mazziotta, M. N. Michelson, P. F. Mirabal, N. Mitthumsiri, W. Mizuno, T. Moiseev, A. A. Monzani, M. E. Morselli, A. Moskalenko, I. V. Murgia, S. Nuss, E. Ohsugi, T. Omodei, N. Orienti, M. Orlando, E. Ormes, J. F. Paneque, D. Perkins, J. S. Pesce-Rollins, M. Petrosian, V. Piron, F. Pivato, G. Porter, T. A. Raino, S. Rando, R. Razzano, M. Razzaque, S. Reimer, A. Reimer, O. Reposeur, T. Romani, R. W. Sanchez-Conde, M. Parkinson, P. M. Saz Schmid, J. Schulz, A. Sgro, C. Siskind, E. J. Spada, F. Spandre, G. Spinelli, P. Suson, D. J. Tajima, H. Takahashi, H. Takahashi, M. Takahashi, T. Thayer, J. B. Thompson, D. J. Tibaldo, L. Torres, D. F. Tosti, G. Troja, E. Vianello, G. Wood, K. S. Wood, M. Yassine, M. Zaharijas, G. Zimmer, S. TI 2FHL: THE SECOND CATALOG OF HARD FERMI-LAT SOURCES SO ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES LA English DT Article DE catalogs; gamma-rays: general ID LARGE-AREA TELESCOPE; EXTRAGALACTIC BACKGROUND LIGHT; GAMMA-RAY EMISSION; GALAXY SURVEY DATA; ENERGETIC PSR J1357-6429; REMNANT RCW 86; MULTIWAVELENGTH OBSERVATIONS; SUPERNOVA-REMNANTS; SKY SURVEY; HESS AB We present a catalog of sources detected above 50 GeV by the Fermi-Large Area Telescope (LAT) in 80 months of data. The newly delivered Pass. 8 event-level analysis allows the detection and characterization of sources in the 50 GeV-2 TeV energy range. In this energy band, Fermi-LAT. has detected 360 sources, which constitute the second catalog of hard Fermi-LAT. sources (2FHL). The improved angular resolution enables the precise localization of point sources (similar to 1.' 7 radius at 68% C.L.) and the detection and characterization of spatially extended sources. We find that 86% of the sources can be associated with counterparts at other wavelengths, of which the majority (75%) are active galactic nuclei and the rest (11%) are Galactic sources. Only 25% of the 2FHL sources have been previously detected by Cherenkov telescopes, implying that the 2FHL provides a reservoir of candidates to be followed up at very high energies. This work closes the energy gap between the observations performed at GeV energies by Fermi-LAT. on orbit and the observations performed at higher energies by Cherenkov telescopes from the ground. C1 [Ackermann, M.; Buehler, R.; Mayer, M.; Schulz, A.] Deutsch Elektronen Synchrotron DESY, D-15738 Zeuthen, Germany. [Ajello, M.; Dominguez, A.; Hartmann, Dieter] Clemson Univ, Dept Phys & Astron, Kinard Lab Phys, Clemson, SC 29634 USA. [Atwood, W. B.; Caputo, R.; Parkinson, P. M. Saz] Univ Calif Santa Cruz, Dept Phys, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA. [Atwood, W. B.; Caputo, R.; Parkinson, P. M. Saz] Univ Calif Santa Cruz, Dept Astron & Astrophys, Santa Cruz, CA 95064 USA. [Baldini, L.] Univ Pisa, I-56127 Pisa, Italy. [Baldini, L.] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy. [Baldini, L.; Blandford, R. D.; Bloom, E. D.; Bottacini, E.; Caliandro, G. A.; Cameron, R. A.; Charles, E.; Chiang, J.; Di Mauro, M.; Drell, P. S.; Focke, W. B.; Franckowiak, A.; Furniss, A. K.; Glanzman, T.; Godfrey, G.; Hill, A. B.; Jogler, T.; Johnson, A. S.; Madejski, G. M.; Michelson, P. F.; Monzani, M. E.; Moskalenko, I. V.; Omodei, N.; Orlando, E.; Paneque, D.; Pesce-Rollins, M.; Petrosian, V.; Porter, T. A.; Reimer, A.; Reimer, O.; Romani, R. W.; Tajima, H.; Thayer, J. B.; Vianello, G.; Wood, M.] Stanford Univ, Dept Phys, Kavli Inst Particle Astrophys & Cosmol, WW Hansen Expt Phys Lab, Stanford, CA 94305 USA. [Baldini, L.; Blandford, R. D.; Bloom, E. D.; Bottacini, E.; Caliandro, G. A.; Cameron, R. A.; Charles, E.; Chiang, J.; Di Mauro, M.; Drell, P. S.; Focke, W. B.; Franckowiak, A.; Furniss, A. K.; Glanzman, T.; Godfrey, G.; Hill, A. B.; Jogler, T.; Johnson, A. S.; Madejski, G. M.; Michelson, P. F.; Monzani, M. E.; Moskalenko, I. V.; Omodei, N.; Orlando, E.; Paneque, D.; Pesce-Rollins, M.; Petrosian, V.; Porter, T. A.; Reimer, A.; Reimer, O.; Romani, R. W.; Tajima, H.; Thayer, J. B.; Vianello, G.; Wood, M.] Stanford Univ, SLAC Natl Accelerator Lab, Stanford, CA 94305 USA. [Ballet, J.; Grenier, I. A.; Schmid, J.] Univ Paris Diderot, CEA Saclay, CNRS, Lab AIM,CEA,IRFU,Serv Astrophys, F-91191 Gif Sur Yvette, France. [Barbiellini, G.; Iafrate, G.; Longo, F.] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy. [Barbiellini, G.; Longo, F.] Univ Trieste, Dipartimento Fis, I-34127 Trieste, Italy. [Bastieri, D.; Rando, R.] Ist Nazl Fis Nucl, Sez Padova, I-35131 Padua, Italy. [Bastieri, D.; Chiaro, G.; La Mura, G.; Rando, R.] Univ Padua, Dipartimento Fis & Astron G Galilei, I-35131 Padua, Italy. [Gonzalez, J. Becerra; Brandt, T. J.; Buson, S.; Cohen, J. M.; Ferrara, E. C.; Guiriec, S.; Harding, A. K.; Hays, E.; Mirabal, N.; Perkins, J. S.; Thompson, D. J.; Troja, E.] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. [Gonzalez, J. Becerra; Cohen, J. M.; Moiseev, A. A.; Troja, E.] Univ Maryland, Dept Phys, College Pk, MD 20742 USA. [Gonzalez, J. Becerra; Cohen, J. M.; Moiseev, A. A.; Troja, E.] Univ Maryland, Dept Astron, College Pk, MD 20742 USA. [Bellazzini, R.; Kuss, M.; Manfreda, A.; Pesce-Rollins, M.; Pivato, G.; Razzano, M.; Sgro, C.; Spada, F.; Spandre, G.] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy. [Bissaldi, E.; Caragiulo, M.; de Palma, F.; Di Venere, L.; Favuzzi, C.; Fusco, P.; Gargano, F.; Giglietto, N.; Giordano, F.; Loparco, F.; Mazziotta, M. N.; Raino, S.; Spinelli, P.] Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy. [Bonino, R.; Cuoco, A.; Desiante, R.; Latronico, L.; Maldera, S.] Ist Nazl Fis Nucl, Sez Torino, I-10125 Turin, Italy. [Bonino, R.; Cuoco, A.] Univ Turin, Dipartimento Fis Gen Amadeo Avogadro, I-10125 Turin, Italy. [Bregeon, J.; Cohen-Tanugi, J.; Nuss, E.; Piron, F.; Yassine, M.] Univ Montpellier, CNRS, IN2P3, Lab Univ & Particules Montpellier, F-34059 Montpellier, France. [Bruel, P.; Fegan, S. J.; Horan, D.] Ecole Polytech, CNRS, IN2P3, Lab Leprince Ringuet, F-91128 Palaiseau, France. [Buson, S.] Univ Maryland Baltimore Cty, Dept Phys, Baltimore, MD 21250 USA. [Buson, S.] Univ Maryland Baltimore Cty, Ctr Space Sci & Technol, Baltimore, MD 21250 USA. [Buson, S.; Moiseev, A. A.] Ctr Res & Explorat Space Sci & Technol CRESST, Greenbelt, MD 20771 USA. [Buson, S.; Moiseev, A. A.] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA. [Caliandro, G. A.] Consorzio Interuniv Fis Spaziale CIFS, I-10133 Turin, Italy. [Caragiulo, M.; Di Venere, L.; Favuzzi, C.; Fusco, P.; Giglietto, N.; Giordano, F.; Loparco, F.; Raino, S.; Spinelli, P.] Univ Politecn Bari, Dipartimento Fis M Merlin, I-70126 Bari, Italy. [Caraveo, P. A.] INAF Ist Astrofis Spaziale & Fis Cosm, I-20133 Milan, Italy. [Cavazzuti, E.; Ciprini, S.; Cutini, S.; Gasparrini, D.; Giommi, P.] Agenzia Spaziale Italiana ASI, Sci Data Ctr, I-00133 Rome, Italy. [Cecchi, C.; Ciprini, S.; Cutini, S.; Gasparrini, D.; Lubrano, P.; Tosti, G.] Ist Nazl Fis Nucl, Sez Perugia, I-06123 Perugia, Italy. [Cecchi, C.; Tosti, G.] Univ Perugia, Dipartimento Fis, I-06123 Perugia, Italy. [Chekhtman, A.] George Mason Univ, Coll Sci, Fairfax, VA 22030 USA. [Cheung, C. C.; Lovellette, M. N.; Wood, K. S.] Naval Res Lab, Div Space Sci, Washington, DC 20375 USA. [Cominsky, L. R.] Sonoma State Univ, Dept Phys & Astron, Rohnert Pk, CA 94928 USA. [Conrad, J.; Sanchez-Conde, M.; Zimmer, S.] Stockholm Univ, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden. [Conrad, J.; Larsson, S.; Li, L.; Sanchez-Conde, M.; Zimmer, S.] AlbaNova, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden. [Cutini, S.] INAF, Osservatorio Astron Roma, I-00040 Rome, Italy. [D'Ammando, F.; Giroletti, M.; Orienti, M.] INAF, Ist Radioastron, I-40129 Bologna, Italy. [D'Ammando, F.] Univ Bologna, Dipartimento Astron, I-40127 Bologna, Italy. [de Angelis, A.] Univ Udine, Dipartimento Fis, I-33100 Udine, Italy. [de Angelis, A.] Ist Nazl Fis Nucl, Sez Trieste, Grp Collegato Udine, I-33100 Udine, Italy. [de Palma, F.] Univ Telemat Pegaso, Piazza Trieste & Trento, I-80132 Naples, Italy. [Desiante, R.] Univ Udine, I-33100 Udine, Italy. [Fortin, P.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Fukazawa, Y.; Takahashi, H.] Hiroshima Univ, Dept Phys Sci, Higashihiroshima, Hiroshima 7398526, Japan. [Funk, S.] Erlangen Ctr Astroparticle Phys, D-91058 Erlangen, Germany. [Grondin, M. -H.; Lemoine-Goumard, M.; Lott, B.; Reposeur, T.] Univ Bordeaux 1, Ctr Etud Nucl Bordeaux Gradignan, CNRS, IN2P3, F-33175 Gradignan, France. [Guillemot, L.] Univ Orleans, Lab Phys & Chim Environm & Espace, CNRS, F-45071 Orleans 02, France. [Guillemot, L.] CNRS, INSU, Stn Radioastron Nancay Observ Paris, F-18330 Nancay, France. [Hewitt, J. W.] Univ N Florida, Dept Phys, Jacksonville, FL 32224 USA. [Hill, A. B.] Univ Southampton, Sch Phys & Astron, Southampton SO17 1BJ, Hants, England. [Iafrate, G.] Ist Nazl Astrofis, Osservatorio Astron Trieste, I-34143 Trieste, Italy. [Johannesson, G.] Univ Iceland, Inst Sci, IS-107 Reykjavik, Iceland. [Kamae, T.] Univ Tokyo, Grad Sch Sci, Dept Phys, Bunkyo Ku, Tokyo 1130033, Japan. [Kataoka, J.] Waseda Univ, Res Inst Sci & Engn, Shinjuku Ku, Tokyo 1698555, Japan. [Knoedlseder, J.] CNRS, IRAP, F-31028 Toulouse 4, France. [Knoedlseder, J.] Univ Toulouse, UPS OMP, IRAP, GAHEC, Toulouse, France. [La Mura, G.; Reimer, A.; Reimer, O.] Univ Innsbruck, Inst Astro & Teilchenphys, A-6020 Innsbruck, Austria. [La Mura, G.; Reimer, A.; Reimer, O.] Univ Innsbruck, Inst Theoret Phys, A-6020 Innsbruck, Austria. [Larsson, S.; Li, L.] KTH Royal Inst Technol, Dept Phys, AlbaNova, SE-10691 Stockholm, Sweden. [Li, J.; Torres, D. F.] Inst Space Sci IEEC CSIC, E-08193 Barcelona, Spain. [Mitthumsiri, W.] Mahidol Univ, Dept Phys, Fac Sci, Bangkok 10400, Thailand. [Mizuno, T.; Ohsugi, T.] Hiroshima Univ, Hiroshima Astrophys Sci Ctr, Higashihiroshima, Hiroshima 7398526, Japan. [Morselli, A.] Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy. [Murgia, S.] Univ Calif Irvine, Ctr Cosmol, Dept Phys & Astron, Irvine, CA 92697 USA. [Ormes, J. F.] Univ Denver, Dept Phys & Astron, Denver, CO 80208 USA. [Paneque, D.; Takahashi, M.] Max Planck Inst Phys & Astrophys, D-80805 Munich, Germany. [Razzaque, S.] Univ Johannesburg, Dept Phys, ZA-2006 Auckland Pk, South Africa. [Parkinson, P. M. Saz] Univ Hong Kong, Dept Phys, Hong Kong, Hong Kong, Peoples R China. [Siskind, E. J.] NYCB Real Time Comp Inc, Lattingtown, NY 11560 USA. [Suson, D. J.] Purdue Univ Calumet, Dept Chem & Phys, Hammond, IN 46323 USA. [Tajima, H.] Nagoya Univ, Solar Terr Environm Lab, Nagoya, Aichi 4648601, Japan. [Takahashi, T.] Japan Aerosp Explorat Agcy, Inst Space & Astronaut Sci, Chuo Ku, Sagamihara, Kanagawa 2525210, Japan. [Tibaldo, L.] Max Planck Inst Kernphys, D-69029 Heidelberg, Germany. [Torres, D. F.] Inst Catalana Recerca & Estudis Avancats ICREA, Barcelona, Spain. [Zaharijas, G.] Ist Nazl Fis Nucl, Sez Trieste, I-34127 Trieste, Italy. [Zaharijas, G.] Univ Trieste, I-34127 Trieste, Italy. [Zaharijas, G.] Univ Nova Gorica, Lab Astroparticle Phys, SI-5000 Nova Gorica, Slovenia. RP Gasparrini, D (reprint author), Clemson Univ, Dept Phys & Astron, Kinard Lab Phys, Clemson, SC 29634 USA. EM jcohen@astro.umd.edu; gasparrini@asdc.asi.it RI Morselli, Aldo/G-6769-2011; Reimer, Olaf/A-3117-2013; giglietto, nicola/I-8951-2012; Moskalenko, Igor/A-1301-2007; Bissaldi, Elisabetta/K-7911-2016; Orlando, E/R-5594-2016; Funk, Stefan/B-7629-2015; Bonino, Raffaella/S-2367-2016; Torres, Diego/O-9422-2016; Di Venere, Leonardo/C-7619-2017; OI Morselli, Aldo/0000-0002-7704-9553; Reimer, Olaf/0000-0001-6953-1385; giglietto, nicola/0000-0002-9021-2888; Moskalenko, Igor/0000-0001-6141-458X; Bissaldi, Elisabetta/0000-0001-9935-8106; Funk, Stefan/0000-0002-2012-0080; Torres, Diego/0000-0002-1522-9065; Di Venere, Leonardo/0000-0003-0703-824X; Sgro', Carmelo/0000-0001-5676-6214; Zaharijas, Gabrijela/0000-0001-8484-7791; Gargano, Fabio/0000-0002-5055-6395; Pesce-Rollins, Melissa/0000-0003-1790-8018; Hill, Adam/0000-0003-3470-4834; Dominguez, Alberto/0000-0002-3433-4610; orienti, monica/0000-0003-4470-7094; DI MAURO, MATTIA/0000-0003-2759-5625; Cutini, Sara/0000-0002-1271-2924; Becerra Gonzalez, Josefa/0000-0002-6729-9022 FU National Aeronautics and Space Administration; Department of Energy in the United States; Commissariat a l'Energie Atomique; Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France; Agenzia Spaziale Italiana; Istituto Nazionale di Fisica Nucleare in Italy; Ministry of Education, Culture, Sports, Science and Technology (MEXT); High Energy Accelerator Research Organization; Japan Aerospace Exploration Agency (JAXA) in Japan; K. A. Wallenberg Foundation; Swedish Research Council; Swedish National Space Board in Sweden; Istituto Nazionale di Astrofisica in Italy; Centre National d' Etudes Spatiales in France FX The Fermi LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States, the Commissariat a l'Energie Atomique and the Centre National de la Recherche Scientifique/Institut National de Physique Nucleaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy, the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK) and Japan Aerospace Exploration Agency (JAXA) in Japan, and the K. A. Wallenberg Foundation, the Swedish Research Council and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d' Etudes Spatiales in France. This research has made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. NR 87 TC 32 Z9 32 U1 3 U2 7 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0067-0049 EI 1538-4365 J9 ASTROPHYS J SUPPL S JI Astrophys. J. Suppl. Ser. PD JAN PY 2016 VL 222 IS 1 AR 5 DI 10.3847/0067-0049/222/1/5 PG 19 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC1NF UT WOS:000368982300005 ER PT J AU Liu, T Zhang, QZ Kim, KT Wu, YF Lee, CW Lee, JE Tatematsu, K Choi, M Juvela, M Thompson, M Goldsmith, PF Liu, SY Naomi, H Koch, P Henkel, C Sanhueza, P He, JH Rivera-Ingraham, A Wang, K Cunningham, MR Tang, YW Lai, SP Yuan, JH Li, D Fuller, G Kang, MJ Luong, QN Liu, HB Ristorcelli, I Yang, J Xu, Y Hirota, T Mardones, D Qin, SL Chen, HR Kwon, W Meng, FY Zhang, HW Kim, MR Yi, HW AF Liu, Tie Zhang, Qizhou Kim, Kee-Tae Wu, Yuefang Lee, Chang Won Lee, Jeong-Eun Tatematsu, Ken'ichi Choi, Minho Juvela, Mika Thompson, Mark Goldsmith, Paul F. Liu, Sheng-yuan Naomi, Hirano Koch, Patrick Henkel, Christian Sanhueza, Patricio He, JinHua Rivera-Ingraham, Alana Wang, Ke Cunningham, Maria R. Tang, Ya-Wen Lai, Shih-Ping Yuan, Jinghua Li, Di Fuller, Gary Kang, Miju Luong, Quang Nguyen Liu, Hauyu Baobab Ristorcelli, Isabelle Yang, Ji Xu, Ye Hirota, Tomoya Mardones, Diego Qin, Sheng-Li Chen, Huei-Ru Kwon, Woojin Meng, Fanyi Zhang, Huawei Kim, Mi-Ryang Yi, Hee-Weon TI PLANCK COLD CLUMPS IN THE lambda ORIONIS COMPLEX. I. DISCOVERY OF AN EXTREMELY YOUNG CLASS 0 PROTOSTELLAR OBJECT AND A PROTO-BROWN DWARF CANDIDATE IN THE BRIGHT-RIMMED CLUMP PGCC G192.32-11.88 SO ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES LA English DT Article DE ISM: jets and outflows; ISM: kinematics and dynamics; stars: formation ID MASSIVE-STAR-FORMATION; SPECTRAL ENERGY-DISTRIBUTIONS; RADIATION-DRIVEN IMPLOSION; IRAS POINT SOURCES; H-II REGIONS; STELLAR OBJECTS; MOLECULAR CLOUDS; SUBMILLIMETER ARRAY; FORMING REGION; CORES AB We are performing a series of observations with ground-based telescopes toward Planck Galactic cold clumps (PGCCs) in the lambda Orionis complex in order to systematically investigate the effects of stellar feedback. In the particular case of PGCC G192.32-11.88, we discovered an extremely young Class 0 protostellar object (G192N) and a proto-brown dwarf candidate (G192S). G192N and G192S are located in a gravitationally bound brightrimmed clump. The velocity and temperature gradients seen in line emission of CO isotopologues indicate that PGCC G192.32-11.88 is externally heated and compressed. G192N probably has the lowest bolometric luminosity (similar to 0.8 L-circle dot) and accretion rate (6.3 x 10(-7) M-circle dot yr(-1)) when compared with other young Class 0 sources (e.g., PACS Bright Red Sources) in the Orion complex. It has slightly larger internal luminosity (0.21 +/- 0.01 L-circle dot) and outflow velocity (similar to 14 km s(-1)) than the predictions of first hydrostatic cores (FHSCs). G192N might be among the youngest Class 0 sources, which are slightly more evolved than an FHSC. Considering its low internal luminosity (0.08 +/- 0.01 L-circle dot) and accretion rate (2.8 x 10(-8) M-circle dot yr(-1)), G192S is an ideal proto-brown dwarf candidate. The star formation efficiency (similar to 0.3%-0.4%) and core formation efficiency (similar to 1%) in PGCC G192.32-11.88 are significantly smaller than in other giant molecular clouds or filaments, indicating that the star formation therein is greatly suppressed owing to stellar feedback. C1 [Liu, Tie; Kim, Kee-Tae; Lee, Chang Won; Choi, Minho; Kang, Miju; Kwon, Woojin; Kim, Mi-Ryang] Korea Astron & Space Sci Inst, Daejeon 34055, South Korea. [Zhang, Qizhou] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Wu, Yuefang; Zhang, Huawei] Peking Univ, Dept Astron, Beijing 100871, Peoples R China. [Lee, Chang Won] Univ Sci & Technol, Daejeon 305333, South Korea. [Lee, Jeong-Eun; Yi, Hee-Weon] Kyung Hee Univ, Sch Space Res, Yongin 446701, Gyeonggi Do, South Korea. [Tatematsu, Ken'ichi; Sanhueza, Patricio; Luong, Quang Nguyen; Hirota, Tomoya] Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan. [Juvela, Mika] Univ Helsinki, Dept Phys, FI-00014 Helsinki, Finland. [Thompson, Mark] Univ Hertfordshire, Ctr Astrophys Res, Hatfield AL10 9AB, Herts, England. [Goldsmith, Paul F.] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA. [Liu, Sheng-yuan; Naomi, Hirano; Koch, Patrick; Tang, Ya-Wen; Liu, Hauyu Baobab; Chen, Huei-Ru] Acad Sinica, Inst Astron & Astrophys, Taipei 106, Taiwan. [Henkel, Christian] Max Planck Inst Radioastron, D-53121 Bonn, Germany. [Henkel, Christian] Abdulaziz Univ, Dept Astron, Jeddah 21589, Saudi Arabia. [He, JinHua] Chinese Acad Sci, Key Lab Struct & Evolut Celestial Objects, Yunnan Observ, Kunming 650011, Yunnan Province, Peoples R China. [Rivera-Ingraham, Alana] ESA ESAC, E-28691 Madrid, Spain. [Wang, Ke] European So Observ, D-85748 Garching, Germany. [Cunningham, Maria R.] Univ New S Wales, Sch Phys, Sydney, NSW 2052, Australia. [Lai, Shih-Ping] Natl Tsing Hua Univ, Inst Astron, Hsinchu, Taiwan. [Lai, Shih-Ping] Natl Tsing Hua Univ, Dept Phys, Hsinchu, Taiwan. [Yuan, Jinghua; Li, Di] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China. [Li, Di] Chinese Acad Sci, Key Lab Radio Astron, Beijing 100864, Peoples R China. [Fuller, Gary] Univ Manchester, Sch Phys & Astron, Jodrell Bank Ctr Astrophys, Manchester M13 9PL, Lancs, England. [Ristorcelli, Isabelle] Univ Toulouse 3, CNRS, IRAP, UMR5277, F-31028 Toulouse 4, France. [Yang, Ji; Xu, Ye] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China. [Mardones, Diego] Univ Chile, Dept Astron, Santiago, Chile. [Qin, Sheng-Li] Yunnan Univ, Dept Astron, Kunming 650091, Peoples R China. [Qin, Sheng-Li] Yunnan Univ, Key Lab Astroparticle Phys Yunnan Prov, Kunming 650091, Peoples R China. [Meng, Fanyi] Univ Cologne, Inst Phys, D-50937 Cologne, Germany. RP Liu, T (reprint author), Korea Astron & Space Sci Inst, 776 Daedeokdae Ro, Daejeon 34055, South Korea. EM liutiepku@gmail.com RI Goldsmith, Paul/H-3159-2016; Mardones, Diego/I-5719-2016 FU KASI fellowship; China Ministry of Science and Technology under State Key Development Program for Basic Research [2012CB821800]; NSFC [11373009, 11433008]; ESO fellowship; DFG Priority Program ("Physics of the Interstellar Medium") [1573, WA3628-1/1]; National Research Foundation of Korea (NRF) - Ministry of Education, Science, and Technology [NRF-2013R1A1A2A10005125]; global research collaboration of the Korea Research Council of Fundamental Science & Technology (KRCF); National Research Foundation of Korea (NRF) [NRF-2015R1A2A2A01004769]; Korea Astronomy and Space Science Institute under the RD program [2015-1-320-18]; Ministry of Science and Technology of Taiwan [MoST 102-2119-M-007-004-MY3] FX We are grateful to the SMA, PMO, CSO, JCMT, and the KVN staff. T.L. is supported by KASI fellowship. Y.W. is partly supported by the China Ministry of Science and Technology under State Key Development Program for Basic Research (No. 2012CB821800), the grants of NSFC No. 11373009 and No. 11433008. K. W. acknowledges the support from the ESO fellowship and DFG Priority Program 1573 ("Physics of the Interstellar Medium") grant WA3628-1/1. C.W.L. was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education, Science, and Technology (NRF-2013R1A1A2A10005125) and also by the global research collaboration of the Korea Research Council of Fundamental Science & Technology (KRCF). This work was carried out in part at the Jet Propulsion Laboratory, operated for NASA by the California Institute of Technology. J.-E.L. was supported by the Basic Science Research Program through the National Research Foundation of Korea (NRF) (grant No. NRF-2015R1A2A2A01004769) and the Korea Astronomy and Space Science Institute under the R&D program (Project No. 2015-1-320-18) supervised by the Ministry of Science, ICT, and Future Planning. The KVN is a facility operated by the Korea Astronomy and Space Science Institute. S.P.L. thanks the support of the Ministry of Science and Technology of Taiwan with grant MoST 102-2119-M-007-004-MY3. Figures 24 and 25 are used with permission from Dr. A. Stutz. NR 104 TC 3 Z9 3 U1 1 U2 2 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0067-0049 EI 1538-4365 J9 ASTROPHYS J SUPPL S JI Astrophys. J. Suppl. Ser. PD JAN PY 2016 VL 222 IS 1 AR 7 PG 28 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC1NF UT WOS:000368982300007 ER PT J AU Vanderburg, A Latham, DW Buchhave, LA Bieryla, A Berlind, P Calkins, ML Esquerdo, GA Welsh, S Johnson, JA AF Vanderburg, Andrew Latham, David W. Buchhave, Lars A. Bieryla, Allyson Berlind, Perry Calkins, Michael L. Esquerdo, Gilbert A. Welsh, Sophie Johnson, John Asher TI PLANETARY CANDIDATES FROM THE FIRST YEAR OF THE K2 MISSION SO ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES LA English DT Article DE methods: data analysis; planets and satellites: detection; techniques: photometric ID TRANSIT SIGNAL RECOVERY; LIGHT CURVES; COLOR TRANSFORMATIONS; ECLIPSING BINARIES; INTRINSIC COLORS; BLEND SCENARIOS; KEPLER MISSION; MAIN-SEQUENCE; HOT JUPITERS; DATA RELEASE AB The Kepler Space Telescope is currently searching for planets transiting stars along the ecliptic plane as part of its extended K2 mission. We processed the publicly released data from the first year of K2 observations (Campaigns 0, 1, 2, and 3) and searched for periodic eclipse signals consistent with planetary transits. Out of the 59,174 targets that we searched, we detect 234 planetary candidates around 208 stars. These candidates range in size from gas giants to smaller than the Earth, and range in orbital periods from hours to over a month. We conducted initial reconnaissance spectroscopy of 68 of the brighter candidate host stars, and present high-resolution optical spectra for these stars. We make all of our data products, including light curves, spectra, and vetting diagnostics available to users online. C1 [Vanderburg, Andrew; Latham, David W.; Bieryla, Allyson; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Welsh, Sophie; Johnson, John Asher] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Buchhave, Lars A.] Univ Copenhagen, Nat Hist Museum Denmark, Ctr Star & Planet Format, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark. [Buchhave, Lars A.] Univ Copenhagen, Niels Bohr Inst, Oster Voldgade 5-7, DK-1350 Copenhagen K, Denmark. RP Vanderburg, A (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM avanderburg@cfa.harvard.edu FU NSF Graduate Research Fellowship [DGE 1144152]; Kepler mission under NASA cooperative agreement [NNX13AB58A]; John Templeton Foundation; NASA [NAS5-26555]; NASA Office of Space Science [NNX13AC07G]; NASA Science Mission directorate FX We thank Dave Charbonneau, Courtney Dressing, Xavier Dumusque, Dan Foreman-Mackey, Mercedes Lopez-Morales, Ben Montet, Elisabeth Newton, and Roberto Sanchis-Ojeda for helpful discussions. We thank the referee, Drake Deming, for a thoughtful report with suggestions that improved the manuscript. We gratefully acknowledge the efforts of the entire Kepler/K2 team who made this work possible. A.V. is supported by the NSF Graduate Research Fellowship, grant No. DGE 1144152. D.W.L. gratefully acknowledges support from the Kepler mission under NASA cooperative agreement NNX13AB58A to the Smithsonian Astrophysical Observatory. We additionally acknowledge support from the John Templeton Foundation. The opinions expressed in this publication are those of the authors and do not necessarily reflect the views of the John Templeton Foundation. This research has made use of NASA's Astrophysics Data System, the VizieR catalogue access tool, CDS, Strasbourg, France, and the NASA Exoplanet Archive (particularly ExoFOP-K2), operated by the California Institute of Technology, under contract with NASA under the Exoplanet Exploration Program. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts. This paper includes data collected by the Kepler/K2 mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. NR 67 TC 29 Z9 29 U1 1 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0067-0049 EI 1538-4365 J9 ASTROPHYS J SUPPL S JI Astrophys. J. Suppl. Ser. PD JAN PY 2016 VL 222 IS 1 AR 14 DI 10.3847/0067-0049/222/1/14 PG 15 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DC1NF UT WOS:000368982300014 ER PT J AU Fowler, AE Blakeslee, AMH Canning-Clode, J Repetto, MF Phillip, AM Carlton, JT Moser, FC Ruiz, GM Miller, AW AF Fowler, Amy E. Blakeslee, April M. H. Canning-Clode, Joao Repetto, Michele F. Phillip, Anne M. Carlton, James T. Moser, Fredrika C. Ruiz, Gregory M. Miller, A. Whitman TI Opening Pandora's bait box: a potent vector for biological invasions of live marine species SO DIVERSITY AND DISTRIBUTIONS LA English DT Article DE biological invasions; bloodworm; introduced; marine; Mid-Atlantic (USA); packing algae; wormweed ID CRABS CARCINUS-MAENAS; SAN-FRANCISCO BAY; PROPAGULE PRESSURE; CANCER-IRRORATUS; NORTH-AMERICA; RICHNESS; CALIFORNIA; DIVERSITY; ATLANTIC; COMMUNITIES AB AimFor over 80years, the Maine baitworm trade has shipped live polychaete worms and packing algae wormweed' to distributors world-wide, while also consistently transferring a wide diversity and abundance of hitchhiking organisms of all life stages to numerous recipient communities. Here, we investigate this potent, yet underestimated, invasion vector using an important recipient region (the Mid-Atlantic) to examine the stepwise species transfer and survival along four stages of the vector. LocationMaine and Mid-Atlantic region (New Jersey, Delaware, Maryland, Virginia and North Carolina), USA. MethodsWe quantified taxonomic identities and abundances of organisms associated with packing algae at four stages along the vector pathway during summer 2011: (1) Maine source habitats; (2) bait boxes from Maine distributors; (3) bait boxes from distributors in five Mid-Atlantic States; and (4) bait bags from retailers in five Mid-Atlantic States. We also examined functional diversity based on significant physical and life history characteristics and assessed genetic diversity for two common hitchhiking snail species. ResultsWe identified 17,798 live macro-organisms across 58 taxa, including marine macro-invertebrates, macroalgae, vascular plants and semi-terrestrial or aquatic invertebrates, present in bait boxes and bags. In all measures of diversity and abundance, we observed decreases of live marine macro-invertebrates across sequential stages of the vector from source to recipient regions. Significant differences in community composition were also observed between stages and were driven by isopods (taxonomic diversity) and isopods, amphipods and some gastropods (functional diversity). Main conclusionsThe lack of management in the face of the sheer magnitude and diversity of organisms that are transported via the live marine bait trade underscores how this is an underappreciated vector that could be a considerable source of successful invasions globally. C1 [Fowler, Amy E.; Blakeslee, April M. H.; Canning-Clode, Joao; Repetto, Michele F.; Phillip, Anne M.; Ruiz, Gregory M.; Miller, A. Whitman] Smithsonian Environm Res Ctr, Marine Invas Lab, Edgewater, MD 21037 USA. [Fowler, Amy E.] South Carolina Dept Nat Resources, Marine Resources Res Inst, 217 Ft Johnson Rd, Charleston, SC 29422 USA. [Blakeslee, April M. H.] E Carolina Univ, Dept Biol, 1001 East 5th St, Greenville, NC 27858 USA. [Canning-Clode, Joao] Marine & Environm Sci Ctr, Estacao Biol Marinha Funchal, P-9000107 Cais Do Carvao, Funchal, Portugal. [Canning-Clode, Joao] Univ Azores, Ctr IMAR, Dept Oceanog & Fisheries UAz, Rua Prof Dr Frederico Machado 4, P-9901862 Horta, Azores, Portugal. [Carlton, James T.] Williams Coll, Mystic Seaport Maritime Studies Program, Mystic, CT 06355 USA. [Moser, Fredrika C.] Univ Syst Maryland, Maryland Sea Grant, College Pk, MD 20740 USA. RP Fowler, AE (reprint author), Smithsonian Environm Res Ctr, Marine Invas Lab, Edgewater, MD 21037 USA.; Fowler, AE (reprint author), South Carolina Dept Nat Resources, Marine Resources Res Inst, 217 Ft Johnson Rd, Charleston, SC 29422 USA. EM fowlera@dnr.sc.gov OI Canning Clode, Joao/0000-0003-2143-6535; Ruiz, Gregory/0000-0003-2499-441X; Miller, Whitman/0000-0003-0484-182X FU Darling Marine Center; Maryland Sea Grant [NA10OAR4170072, SA7528120] FX We thank the SERC Marine Invasions Laboratory, numerous interns and other personnel. We also thank Pete Thayer for field expertise and industry knowledge and Norm Woodley for identifying insect larvae, pupae and adults. We appreciate laboratory space, accommodations and support provided by the Darling Marine Center. We also thank three anonymous referees for comments that significantly improved the manuscript. This research was supported by Maryland Sea Grant awards NA10OAR4170072 and SA7528120. Algae and associated organisms were collected under ME DMR Special License Numbers ME 2011-77-00 and ME 2012-14-01. NR 68 TC 1 Z9 1 U1 6 U2 16 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1366-9516 EI 1472-4642 J9 DIVERS DISTRIB JI Divers. Distrib. PD JAN PY 2016 VL 22 IS 1 BP 30 EP 42 DI 10.1111/ddi.12376 PG 13 WC Biodiversity Conservation; Ecology SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DC2SI UT WOS:000369066200004 ER PT J AU Thorwirth, S Martin-Drumel, MA Endres, CP Salomon, T Zingsheim, O van Wijngaarden, J Pirali, O Gruet, S Lewen, F Schlemmer, S McCarthy, MC AF Thorwirth, S. Martin-Drumel, M. A. Endres, C. P. Salomon, T. Zingsheim, O. van Wijngaarden, J. Pirali, O. Gruet, S. Lewen, F. Schlemmer, S. McCarthy, M. C. TI An ASAP treatment of vibrationally excited S2O: The v(3) mode and the v(3) + v(2) - v(2) hot band SO JOURNAL OF MOLECULAR SPECTROSCOPY LA English DT Article DE Fourier-transform spectroscopy; Far-infrared; Synchrotron radiation; Millimeter-wave spectroscopy; Disulfur monoxide; S2O; Radio-frequency discharge ID DISULFUR MONOXIDE; SPECTROSCOPY; SPECTRUM AB The fundamental S-S stretching mode v(3) of disulfur monoxide, S2O, located at 679 cm(-1), has been investigated using Fourier-transform far-infrared spectroscopy at the SOLEIL synchrotron facility. A spectroscopic analysis has been performed using an Automated Spectral Assignment Procedure (ASAP) which permits accurate determination of more than 2000 energy levels from v3. In addition, the v(3) + v(2)-v(2) hot band was observed for the first time and some 500 corresponding energy levels were assigned. The high-resolution synchrotron study was complemented with pure rotational spectra of S2O in the (v(1), v(2), v(3)) = (0, 0,1) vibrational state observed in the frequency range from 250 to 280 GHz using a long-path absorption cell. From these combined measurements, extensive molecular parameter sets have been determined and precise band centers have been derived for both vibrational bands. (C) 2015 Elsevier Inc. All rights reserved. C1 [Thorwirth, S.; Endres, C. P.; Salomon, T.; Zingsheim, O.; Lewen, F.; Schlemmer, S.] Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany. [Martin-Drumel, M. A.; McCarthy, M. C.] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. [Endres, C. P.] Max Planck Inst Extraterr Phys, Giessenbachstr 1, D-85748 Garching, Germany. [van Wijngaarden, J.] Univ Manitoba, Dept Chem, Winnipeg, MB R3T 2N2, Canada. [Pirali, O.; Gruet, S.] SOLEIL Synchrotron, F-91192 Gif Sur Yvette, France. [Pirali, O.; Gruet, S.] Univ Paris Saclay, Univ Paris 11, ISMO, CNRS, F-91405 Orsay, France. [Gruet, S.] Max Planck Inst Struktur & Dynam Materie, Luruper Chaussee 149, D-22761 Hamburg, Germany. RP Thorwirth, S (reprint author), Univ Cologne, Inst Phys 1, Zulpicher Str 77, D-50937 Cologne, Germany. EM sthorwirth@ph1.uni-koeln.de RI Schlemmer, Stephan/E-2903-2015; Thorwirth, Sven/C-6217-2011 OI Schlemmer, Stephan/0000-0002-1421-7281; Thorwirth, Sven/0000-0001-8200-6710 FU Deutsche Forschungsgemeinschaft (DFG) [SFB 956]; DFG [TH 1301/3-2]; NASA [NNX13AE59G]; Natural Sciences and Engineering Research Council of Canada (NSERC) [RGPIN/326993-2010] FX The authors are grateful to SOLEIL for providing beamtime on the AILES beamline under the proposal 20140364. The present work was supported by the Deutsche Forschungsgemeinschaft (DFG) through Grant SFB 956. S. T. gratefully acknowledges funding from the DFG through Grant TH 1301/3-2. M. C. M. and M. A. M.-D. thank the Smithsonian Astrophysical Observatory and NASA Grant NNX13AE59G for travel support. Travel support for J. v. W. was provided by the Natural Sciences and Engineering Research Council of Canada (NSERC) through the Discovery Grant (JvW: RGPIN/326993-2010) program. NR 10 TC 0 Z9 0 U1 3 U2 7 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0022-2852 EI 1096-083X J9 J MOL SPECTROSC JI J. Mol. Spectrosc. PD JAN PY 2016 VL 319 BP 47 EP 49 DI 10.1016/j.jms.2015.12.009 PG 3 WC Physics, Atomic, Molecular & Chemical; Spectroscopy SC Physics; Spectroscopy GA DC1IN UT WOS:000368970100007 ER PT J AU Caterino, MS Tishechkin, AK AF Caterino, Michael S. Tishechkin, Alexey K. TI A revision of Megalocraerus Lewis, 1902 (Coleoptera, Histeridae: Exosternini) SO ZOOKEYS LA English DT Article DE Histeridae; Histerinae; Exosternini; subcortical predator; Neotropical region ID PHYLOGENY AB The formely monotypic Neotropical genus Megalocraerus Lewis is revised to include five species, known from southeastern Brazil to Costa Rica: M. rubricatus Lewis, M. mandibularis sp. n., M. chico sp. n., M. madrededios sp. n., and M. tiputini sp. n. We describe the species, map their distributions, and provide a key for their identification. Their subcylindrical body form and emarginate mesosternum have previously hindered placement to tribe, although their curent assignment to Exosternini now appears well supported by morphological evidence. Nothing is known of the natural history of the species. C1 [Caterino, Michael S.] Clemson Univ, Dept Agr & Environm Sci, Clemson, SC 29634 USA. [Tishechkin, Alexey K.] Smithsonian Inst, USDA, Systemat Entomol Lab, Natl Museum Nat Hist, Washington, DC 20013 USA. RP Caterino, MS (reprint author), Clemson Univ, Dept Agr & Environm Sci, Clemson, SC 29634 USA. EM mcateri@clemson.edu FU National Science Foundation [DEB-0949790] FX For providing specimen material, assistance in the field, and assistance with permitting, we would like to thank Luciana Masutti de Almeida, Daniel Moura, Fernando Leivas, and Kleber Mise (UFPR), Max Barclay and Roger Booth (BMNH), Angel Solis (INBIO), Paul Skelley (Florida State Collection of Arthropods), Tiputini Biodiversity Station, Zack Falin (Snow Entomological Collection, University of Kansas), Nicolas Degallier, and Al Allen. We also thank the National Science Foundation for financial support (DEB-0949790). NR 12 TC 0 Z9 0 U1 1 U2 3 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 557 BP 59 EP 78 DI 10.3897/zookeys.557.7087 PG 20 WC Zoology SC Zoology GA DC0OE UT WOS:000368916400003 PM 26877699 ER PT J AU McKamey, SH AF McKamey, Stuart H. TI A new species of Eutettix (Hemiptera, Cicadellidae, Deltocephalinae) from Wisconsin SO ZOOKEYS LA English DT Article DE Leafhopper; new species; Athysanini; Nearctic; Wisconsin; Quercus AB Eutettix latoides sp. n., is described from central Wisconsin. It most closely resembles the Californian species E. latus Hepner, and was collected from Quercus ellipsoidalis. C1 [McKamey, Stuart H.] Smithsonian Inst, USDA ARS, Systemat Entomol Lab, NMNH, MRC 168,POB 37012, Washington, DC 20013 USA. RP McKamey, SH (reprint author), Smithsonian Inst, USDA ARS, Systemat Entomol Lab, NMNH, MRC 168,POB 37012, Washington, DC 20013 USA. EM stuart.mckamey@ars.usda.gov NR 4 TC 0 Z9 0 U1 1 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 557 BP 79 EP 83 DI 10.3897/zookeys.557.5939 PG 5 WC Zoology SC Zoology GA DC0OE UT WOS:000368916400004 PM 26877700 ER PT J AU McKamey, SH Porter, MJ AF McKamey, Stuart H. Porter, Mitchell J. TI First Immature of the New World Treehopper tribe Thuridini (Hemiptera, Membracidae, Smiliinae) with a new synonym, a new combination, and a new country record SO ZOOKEYS LA English DT Article DE Thuris; Parantonae; nymph; syn. n.; comb. n.; Ecuador; Venezuela AB The species Thuris depressus Sakakibara (1975) is proposed as a syn. n. of Thuris binodosus (Goding 1926), comb. n. The distribution of the genus is expanded from Brazil and Peru to include Ecuador and Venezuela, and the immature is described based on 75 characters. C1 [McKamey, Stuart H.] Smithsonian Inst, USDA ARS, Systemat Entomol Lab, NMNH MRC 168, Washington, DC 20560 USA. [Porter, Mitchell J.] Univ Maryland, Dept Biol, College Pk, MD 20742 USA. RP McKamey, SH (reprint author), Smithsonian Inst, USDA ARS, Systemat Entomol Lab, NMNH MRC 168, Washington, DC 20560 USA. EM stuart.mckamey@ars.usda.gov NR 9 TC 0 Z9 0 U1 2 U2 4 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 557 BP 85 EP 91 DI 10.3897/zookeys.557.6602 PG 7 WC Zoology SC Zoology GA DC0OE UT WOS:000368916400005 PM 26877701 ER PT S AU Lessios, HA AF Lessios, H. A. BE Carlson, CA Giovannoni, SJ TI The Great Diadema antillarum Die-Off: 30 Years Later SO ANNUAL REVIEW OF MARINE SCIENCE, VOL 8 SE Annual Review of Marine Science LA English DT Review; Book Chapter DE coral reef; algae; recruitment; mortality; population recovery ID SEA-URCHIN-DIADEMA; CARIBBEAN CORAL-REEFS; DEPENDENT SIZE REGULATION; REGION-WIDE DECLINES; MASS MORTALITY EVENT; EL-NINO EVENT; PUERTO-RICO; POPULATION-DENSITY; COMMUNITY STRUCTURE; CLIMATE-CHANGE AB In 1983-1984, the sea urchin Diadema antillarum suffered mass mortality throughout the Caribbean, Florida, and Bermuda. The demise of this herbivore contributed to a phase shift of Caribbean reefs from coral-dominated to alga-dominated communities. A compilation of published data of D. antillarum population densities shows that there has been moderate recovery since 1983, with the highest rates on islands of the eastern Caribbean. On the average the current population densities are approximately 12% of those before the die-off, apparently because of recruitment limitation, but the exact factors that are constraining the recovery are unclear. Scattered D. antillarum cohorts in some localities and aggregation of settled individuals in shallow water have created zones of higher herbivory in which juvenile coral recruitment, survivorship, and growth are higher than they are in alga-dominated areas. Unlike other stressors on Caribbean coral reefs, recent changes in D. antillarum populations progress toward aiding the recovery of coral cover. C1 [Lessios, H. A.] Smithsonian Trop Res Inst, Balboa, Panama. RP Lessios, HA (reprint author), Smithsonian Trop Res Inst, Balboa, Panama. EM lessiosh@post.harvard.edu NR 128 TC 6 Z9 6 U1 18 U2 50 PU ANNUAL REVIEWS PI PALO ALTO PA 4139 EL CAMINO WAY, PO BOX 10139, PALO ALTO, CA 94303-0897 USA SN 1941-1405 BN 978-0-8243-4508-2 J9 ANNU REV MAR SCI JI Annu. Rev. Mar. Sci. PY 2016 VL 8 BP 267 EP 283 DI 10.1146/annurev-marine-122414-033857 PG 17 WC Geochemistry & Geophysics; Marine & Freshwater Biology; Oceanography SC Geochemistry & Geophysics; Marine & Freshwater Biology; Oceanography GA BE1QC UT WOS:000368369200012 PM 26048480 ER PT J AU Ranjan, S Sasselov, DD AF Ranjan, Sukrit Sasselov, Dimitar D. TI Influence of the UV Environment on the Synthesis of Prebiotic Molecules SO ASTROBIOLOGY LA English DT Article ID ABSOLUTE OSCILLATOR-STRENGTHS; ABSORPTION CROSS-SECTIONS; EARTHS EARLY ATMOSPHERE; LATE HEAVY BOMBARDMENT; TERRESTRIAL PLANETS; LIQUID WATER; RNA WORLD; CHEMICAL EVOLUTION; ORGANIC-MOLECULES; WESTERN-AUSTRALIA AB Ultraviolet radiation is common to most planetary environments and could play a key role in the chemistry of molecules relevant to abiogenesis (prebiotic chemistry). In this work, we explore the impact of UV light on prebiotic chemistry that might occur in liquid water on the surface of a planet with an atmosphere. We consider effects including atmospheric absorption, attenuation by water, and stellar variability to constrain the UV input as a function of wavelength. We conclude that the UV environment would be characterized by broadband input, and wavelengths below 204nm and 168nm would be shielded out by atmospheric CO2 and water, respectively. We compare this broadband prebiotic UV input to the narrowband UV sources (e.g., mercury lamps) often used in laboratory studies of prebiotic chemistry and explore the implications for the conclusions drawn from these experiments. We consider as case studies the ribonucleotide synthesis pathway of Powner et al. (2009) and the sugar synthesis pathway of Ritson and Sutherland (2012). Irradiation by narrowband UV light from a mercury lamp formed an integral component of these studies; we quantitatively explore the impact of more realistic UV input on the conclusions that can be drawn from these experiments. Finally, we explore the constraints solar UV input places on the buildup of prebiotically important feedstock gasses like CH4 and HCN. Our results demonstrate the importance of characterizing the wavelength dependence (action spectra) of prebiotic synthesis pathways to determine how pathways derived under laboratory irradiation conditions will function under planetary prebiotic conditions. Key Words: Laboratory investigationsOrigin of lifePlanetary environmentsUV radiationRNA world. Astrobiology 16, 68-88. C1 [Ranjan, Sukrit; Sasselov, Dimitar D.] Harvard Smithsonian Ctr Astrophys, 60 Garden St,Mail Stop 10, Cambridge, MA 02138 USA. RP Ranjan, S (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St,Mail Stop 10, Cambridge, MA 02138 USA. EM sranjan@cfa.harvard.edu OI Ranjan, Sukrit/0000-0002-5147-9053 FU Simons Foundation [290360] FX S.R. and D.D.S. gratefully acknowledge support from the Simons Foundation, grant no. 290360. NR 104 TC 3 Z9 3 U1 10 U2 30 PU MARY ANN LIEBERT, INC PI NEW ROCHELLE PA 140 HUGUENOT STREET, 3RD FL, NEW ROCHELLE, NY 10801 USA SN 1531-1074 EI 1557-8070 J9 ASTROBIOLOGY JI Astrobiology PD JAN 1 PY 2016 VL 16 IS 1 BP 68 EP 88 DI 10.1089/ast.2015.1359 PG 21 WC Astronomy & Astrophysics; Biology; Geosciences, Multidisciplinary SC Astronomy & Astrophysics; Life Sciences & Biomedicine - Other Topics; Geology GA DB7QB UT WOS:000368709500005 PM 26789356 ER PT J AU Pistone, M Blundy, JD Brooker, RA AF Pistone, Mattia Blundy, Jonathan D. Brooker, Richard A. CA EIMF TI Textural and chemical consequences of interaction between hydrous mafic and felsic magmas: an experimental study SO CONTRIBUTIONS TO MINERALOGY AND PETROLOGY LA English DT Article DE Magma; Mixing; Water; Diffusion; Comb layering; Undercooling ID UNIDIRECTIONAL SOLIDIFICATION TEXTURES; SIERRA-NEVADA BATHOLITH; PEGMATITE-APLITE DIKES; CRYSTAL MUSHES; 200 MPA; MULTIELEMENT GLASSES; GRANITIC LIQUIDS; ADAMELLO MASSIF; SILICATE MELTS; HIGH-PRESSURE AB Mantle-derived, hydrous mafic magmas are often invoked as a mechanism to transfer heat, mass and volatiles to felsic plutons in the Earth's crust. Field observations suggest that mafic, water-rich magmas often intrude viscous felsic crystal-rich mushes. This scenario can advect water from the crystallising mafic magma to the felsic magma, leading to an increase in melt fraction in the felsic mush and subsequent mobilisation, at the same time as the mafic magma becomes quenched through a combination of cooling and water loss. To investigate such a scenario, we conducted experiments on a water-undersaturated (4 wt% H2O in the interstitial melt) dacitic crystal mush (50-80 vol% quartz crystals) subject to volatile supply from a water-saturated (>= 6 wt% H2O) andesite magma at 950 degrees C and 4 kbar. Our experimental run products show unidirectional solidification textures (i.e. comb layering) as crystals nucleate at the mafic-felsic interface and grow into the mafic end-member. This process is driven by isothermal and isobaric undercooling resulting from a change in liquidus temperature as water migrates from the mafic to the felsic magma. We refer to this process as "chemical quenching" and suggest that some textures associated with natural mafic-felsic interactions are not simply cooling-driven in origin, but can be caused by exsolution of volatiles adjacent to an interface, whether a water-undersaturated felsic magma (as in our experiments) or a fracture. C1 [Pistone, Mattia; Blundy, Jonathan D.; Brooker, Richard A.] Univ Bristol, Sch Earth Sci, Wills Mem Bldg,Queens Rd, Bristol BS8 1RJ, Avon, England. [Pistone, Mattia] Smithsonian Inst, Natl Museum Nat Hist, Dept Mineral Sci, Washington, DC 20560 USA. [EIMF] Univ Edinburgh, Sch Geosci, Grant Inst, Edinburgh Ion Microprobe Facil, Edinburgh EH9 3JW, Midlothian, Scotland. RP Pistone, M (reprint author), Univ Bristol, Sch Earth Sci, Wills Mem Bldg,Queens Rd, Bristol BS8 1RJ, Avon, England. EM PistoneM@si.edu OI Pistone, Mattia/0000-0001-7560-3146 FU SNSF [EPM-PBEZP2_14922]; ERC Advanced Grant CRITMAG FX SNSF Grant EPM-PBEZP2_14922 and ERC Advanced Grant CRITMAG supported this research. We acknowledge: K. Stuart and B. Buse for supporting during the EPMA, FEG-EPMA, and SEM analyses (University of Bristol); R. Hinton for assisting during the SIMS analyses (EIMF, University of Edinburgh); C. Clapham and D. Hawley for technical support (University of Bristol); J. Riker for providing high-H2O-content silicate glasses as standards for SIMS analysis; Alberto Luisoni AG (Switzerland), Nabaltec AG (Germany), and B. Tripoli (ETH-Zurich) for supplying quartz crystals, APYRAL 60CD, and wollastonite used in the starting materials; O. Muntener, A. Acosta-Vigil, and an anonymous reviewer for their helpful comments on an earlier version of the manuscript. NR 114 TC 4 Z9 4 U1 8 U2 20 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 0010-7999 EI 1432-0967 J9 CONTRIB MINERAL PETR JI Contrib. Mineral. Petrol. PD JAN PY 2016 VL 171 IS 1 AR 8 DI 10.1007/s00410-015-1218-4 PG 21 WC Geochemistry & Geophysics; Mineralogy SC Geochemistry & Geophysics; Mineralogy GA DB7NO UT WOS:000368702600008 ER PT J AU Baker, JL Wood, B Karpinski, BA LaMantia, AS Maynard, TM AF Baker, Jennifer L. Wood, Bernard Karpinski, Beverly A. LaMantia, Anthony-S. Maynard, Thomas M. TI Testicular receptor 2, Nr2c1, is associated with stem cells in the developing olfactory epithelium and other cranial sensory and skeletal structures SO GENE EXPRESSION PATTERNS LA English DT Article DE Nr2c1; TR2; Olfactory epithelium; Pax7; Ncam; Ascl1 ID ORPHAN NUCLEAR RECEPTORS; ESTROGEN-RECEPTOR; SUPERFAMILY; NEURONS; DIVERSIFICATION; DIFFERENTIATION; PROGENITORS; EVOLUTION; PATHWAY; TR2 AB Comparative genomic analysis of the nuclear receptor family suggests that the testicular receptor 2, Nr2c1, undergoes positive selection in the human-chimpanzee clade based upon a significant increase in nonsynonymous compared to synonymous substitutions. Previous in situ analyses of Nr2c1 lacked the temporal range and spatial resolution necessary to characterize cellular expression of this gene from early to mid gestation, when many nuclear receptors are key regulators of tissue specific stem or progenitor cells. Thus, we asked whether Nr2c1 protein is associated with stem cell populations in the midgestation mouse embryo. Nr2c1 is robustly expressed in the developing olfactory epithelium. Its expression in the olfactory epithelium shifts from multiple progenitor classes at early stages to primarily transit amplifying cells later in olfactory epithelium development. In the early developing central nervous system, Nr2c1 is limited to the anterior telencephalon/olfactory bulb anlagen, coincident with Nestin-positive neuroepithelial stem cells. Nr2c1 is also seen in additional cranial sensory specializations including cells surrounding the mystacial vibrissae, the retinal pigment epithelium and Scarpa's ganglion. Nr2c1 was also detected in a subset of mesenchymal cells in developing teeth and cranial bones. The timing and distribution of embryonic expression suggests that Nr2c1 is primarily associated with the early genesis of mammalian cranial sensory neurons and craniofacial skeletal structures. Thus, Nr2c1 may be a candidate for mediating parallel adaptive changes in cranial neural sensory specializations such as the olfactory epithelium, retina and mystacial vibrissae and in non-neural craniofacial features including teeth. (C) 2015 Elsevier B.V. All rights reserved. C1 [Baker, Jennifer L.; Wood, Bernard] George Washington Univ, Ctr Adv Study Human Paleobiol, Washington, DC 20052 USA. [Wood, Bernard] Smithsonian Inst, Human Origins Program, Natl Museum Nat Hist, Washington, DC 20560 USA. [Karpinski, Beverly A.] George Washington Univ, Dept Anat & Regenerat Biol, Washington, DC 20052 USA. [Baker, Jennifer L.; LaMantia, Anthony-S.; Maynard, Thomas M.] George Washington Univ, GW Inst Neurosci, Washington, DC 20052 USA. [LaMantia, Anthony-S.; Maynard, Thomas M.] George Washington Univ, Dept Physiol & Pharmacol, Washington, DC 20052 USA. RP Baker, JL (reprint author), George Washington Univ, Ctr Adv Study Human Paleobiol, Washington, DC 20052 USA. EM jenniferlbaker7@gmail.com RI Maynard, Thomas/I-9039-2012; OI Maynard, Thomas/0000-0001-6976-3936; Baker, Jennifer/0000-0002-5192-2377 FU National Science Foundation Doctoral Dissertation Research Improvement Grant [BSC-1455625]; Wenner-Gren Foundation Dissertation Fieldwork Grant [8735]; NSF IGERT grant [DGE-0801634]; GWOVPR; GW School of Medicine for the GW Institute of Neuroscience Biomarker Core Facility; NIH [DC011534] FX This work was funded by a National Science Foundation Doctoral Dissertation Research Improvement Grant (BSC-1455625), a Wenner-Gren Foundation Dissertation Fieldwork Grant (#8735), a NSF IGERT grant (DGE-0801634), support from GWOVPR and The GW School of Medicine for the GW Institute of Neuroscience Biomarker Core Facility, and NIH DC011534 (ASL). NR 26 TC 1 Z9 1 U1 0 U2 1 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 1567-133X EI 1872-7298 J9 GENE EXPR PATTERNS JI Gene Expr. Patterns PD JAN PY 2016 VL 20 IS 1 BP 71 EP 79 DI 10.1016/j.gep.2015.12.002 PG 9 WC Developmental Biology; Genetics & Heredity SC Developmental Biology; Genetics & Heredity GA DB6FR UT WOS:000368610000008 PM 26712358 ER PT J AU Tymen, B Rejou-Mechain, M Dalling, JW Fauset, S Feldpausch, TR Norden, N Phillips, OL Turner, BL Viers, J Chave, J AF Tymen, Blaise Rejou-Mechain, Maxime Dalling, James W. Fauset, Sophie Feldpausch, Ted R. Norden, Natalia Phillips, Oliver L. Turner, Benjamin L. Viers, Jerome Chave, Jerome TI Evidence for arrested succession in a liana-infested Amazonian forest SO JOURNAL OF ECOLOGY LA English DT Article DE above-ground productivity; biomass; carbon turnover; determinants of plant community diversity and structure; forest dynamics; forest structure; French Guiana; remote sensing ID TROPICAL SECONDARY FORESTS; BARRO-COLORADO ISLAND; NEOTROPICAL FOREST; ABOVEGROUND BIOMASS; TREE REGENERATION; RAIN-FOREST; SEEDLING RESPONSES; SOUTH-AMERICA; FRENCH-GUIANA; TERM CHANGES AB 1. Empirical evidence and modelling both suggest that global changes may lead to an increased dominance of lianas and thus to an increased prevalence of liana-infested forest formations in tropical forests. The implications for tropical forest structure and the carbon cycle remain poorly understood. 2. We studied the ecological processes underpinning the structure and dynamics of a liana-infested forest in French Guiana, using a combination of long-term surveys (tree, liana, seedling and litter-fall), soil chemical analyses and remote-sensing approaches (LiDAR and Landsat). 3. At stand scale and for adult trees, the liana-infested forest had higher growth, recruitment and mortality rates than the neighbouring high-canopy forest. Both total seedling density and tree seedling recruitment were lower in the liana-infested forest. Stand scale above-ground biomass of the liana-infested forest was 58% lower than in the high-canopy forest. 4. Above-ground net primary productivity (ANPP) was comparable in the liana-infested and high-canopy forests. However, due to more abundant leaf production, the relative contribution of fast turnover carbon pools to ANPP was larger in the liana-infested forest and the carbon residence time was half that of the high-canopy forest. 5. Although soils of the liana-infested forest were richer in nutrients, soil elemental ratios suggest that liana-infested forest and high-canopy forest soils both derive from the same geological substrate. The higher nutrient concentration in the liana-infested forest may therefore be the result of a release of nutrients from vegetation after a forest blowdown. 6. Using small-footprint LiDAR campaigns, we show that the overall extent of the liana-infested forest has remained stable from 2007 to 2012 but about 10% of the forest area changed in forest cover type. Landsat optical imagery confirms the liana-infested forest presence in the landscape for at least 25 years. 7. Synthesis. Because persistently high rates of liana infestation are maintained by the fast dynamics of the liana-infested forest, liana-infested forests here appear to be the result of an arrested tropical forest succession. If the prevalence of such arrested succession forests were to increase in the future, this would have important implications for the carbon sink potential of Amazonian forests. C1 [Tymen, Blaise; Rejou-Mechain, Maxime; Chave, Jerome] Univ Toulouse 3, Lab Evolut & Diversite Biol, CNRS, UMR 5174, F-31062 Toulouse, France. [Rejou-Mechain, Maxime] French Inst Pondicherry, UMIFRE 21, USR CNRS MAEE 3330, Pondicherry, India. [Dalling, James W.] Univ Illinois, Dept Plant Biol, Urbana, IL 61801 USA. [Dalling, James W.; Turner, Benjamin L.] Smithsonian Trop Res Inst, Balboa, Ancon, Panama. [Fauset, Sophie; Feldpausch, Ted R.; Phillips, Oliver L.] Univ Leeds, Sch Geog, Leeds LS2 9JT, W Yorkshire, England. [Feldpausch, Ted R.] Univ Exeter, Coll Life & Environm Sci, Exeter EX4 4RJ, Devon, England. [Norden, Natalia] Fdn Cedrela, Bogota, Colombia. [Norden, Natalia] Univ Nacl Colombia, Ctr Int Fis, Bogota, Colombia. [Norden, Natalia] Univ Rosario, Programa Biol, Fac Ciencias Nat & Matemat, Bogota, Colombia. [Viers, Jerome] Univ Toulouse 3, Gosci Environm Toulouse, UMR 5563, CNRS,IRD, F-31400 Toulouse, France. RP Tymen, B (reprint author), Univ Toulouse 3, Lab Evolut & Diversite Biol, CNRS, UMR 5174, 118 Route Narbonne, F-31062 Toulouse, France. EM blaise.tymen@gmail.com RI Turner, Benjamin/E-5940-2011; Phillips, Oliver/A-1523-2011; Feldpausch, Ted/D-3436-2009 OI Turner, Benjamin/0000-0002-6585-0722; Phillips, Oliver/0000-0002-8993-6168; Feldpausch, Ted/0000-0002-6631-7962 FU CNES; Agence Nationale de la Recherche (CEBA) [ANR-10-LABX-25-01]; Agence Nationale de la Recherche (TULIP) [ANR-10-LABX-0041]; Agence Nationale de la Recherche (ANAEE-France) [ANR-11-INBS-0001]; Gordon and Betty Moore Foundation; NERC Consortium [NE/F005806/1]; ERC Advanced Grant; Royal Society Wolfson Research Merit Award FX We thank V. Alt, C. Baghooa, C. Baldeck, C. Baraloto, W. Betian, V. Bezard, L. Blanc, V. Chama Moscoso, P. Chatelet, M. Delaval, J. Engel, P. Gaucher, T. Gaui, S. Icho, G. Lopez-Gonzalez, A. Monteagudo, P. Petronelli, G. Pickavance and J. Ricardo for field data collection and curation. We gratefully acknowledge financial support from CNES (postdoctoral grant to MRM and TOSCA programme), and from 'Investissement d'Avenir' grants managed by Agence Nationale de la Recherche (CEBA, ref. ANR-10-LABX-25-01; TULIP: ANR-10-LABX-0041; ANAEE-France: ANR-11-INBS-0001) and the Gordon and Betty Moore Foundation and NERC Consortium Grants 'AMAZONICA' (NE/F005806/1) who supported the RAINFOR project. O.L.P. is supported by an ERC Advanced Grant and a Royal Society Wolfson Research Merit Award. Finally, we thank the US Geological Survey for providing access to the Landsat data. NR 70 TC 5 Z9 5 U1 14 U2 48 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0022-0477 EI 1365-2745 J9 J ECOL JI J. Ecol. PD JAN PY 2016 VL 104 IS 1 BP 149 EP 159 DI 10.1111/1365-2745.12504 PG 11 WC Plant Sciences; Ecology SC Plant Sciences; Environmental Sciences & Ecology GA DB1WC UT WOS:000368298700015 ER PT J AU Pillar, AG Marra, PP Flood, NJ Reudink, MW AF Pillar, Andrew G. Marra, Peter P. Flood, Nancy J. Reudink, Matthew W. TI Moult migration in Bullock's orioles (Icterus bullockii) confirmed by geolocators and stable isotope analysis SO JOURNAL OF ORNITHOLOGY LA English DT Article DE Bullock's oriole; Icterus bullockii; Stable isotope; Geolocator; Moult migration ID LIGHT-LEVEL GEOLOCATORS; ANIMAL MOVEMENT; STOPOVER SITES; HYDROGEN ISOTOPES; MONSOON REGION; MIGRANT BIRDS; PATTERNS; PRECIPITATION; CONNECTIVITY; FEATHERS AB In contrast to the majority of migratory songbirds in North America, which moult on or near their breeding grounds, the Bullock's oriole (Icterus bullockii) is reported to stop during fall migration to moult en route to the wintering grounds. These birds seem to take advantage of food resources during the Mexican monsoon season in the Southwestern USA and Northwestern Mexico. We studied a population of Bullock's orioles at the northern limit of their breeding range in Kamloops, British Columbia, Canada, using a combination of light-level geolocators and stable hydrogen isotope analysis. We found evidence that supports the existence of moult migration in this species, with geolocators indicating that all birds appeared to stay in the Mexican monsoon region for moult in an extended stopover period during fall migration. Feathers were isotopically enriched with deuterium compared to predicted breeding isotope values and were significantly more negative than winter-grown claws, confirming that moult occurred somewhere between the breeding and wintering grounds. Stable isotope data were consistent with complete prebasic stopover moult in adults and complete contour feather and variable tail feather moult in first-year orioles. Our results confirm that this northern population of Bullock's orioles employs a moult migration strategy and highlight the usefulness of combining geolocator and stable isotope studies. C1 [Pillar, Andrew G.; Flood, Nancy J.; Reudink, Matthew W.] Thompson Rivers Univ, Dept Biol Sci, Kamloops, BC, Canada. [Marra, Peter P.] Natl Zool Pk, Migratory Bird Ctr, Smithsonian Conservat Biol Inst, Washington, DC USA. RP Reudink, MW (reprint author), Thompson Rivers Univ, Dept Biol Sci, Kamloops, BC, Canada. EM mreudink@tru.ca OI Reudink, Matthew/0000-0001-8956-5849 FU Natural Sciences and Engineering Research Council Discovery Grant; Natural Sciences and Engineering Research Council Canada Graduate Scholarship FX We would like to thank D. Carlyle-Moses, and D. Green for insightful comments and suggestions on this manuscript. We would also like to thank S. Joly, O. Greaves, and J. Crawford for field assistance on this project and C. France for assistance with stable isotope analysis. Thank you also to the Dreger family, the owners of the Knutsford Campground and T. McLeod at Tranquille on the Lake for access to study sites and the Kamloops Naturalists Club for information on oriole locations. Funding was provided by a Natural Sciences and Engineering Research Council Discovery Grant to M. W. R. and a Natural Sciences and Engineering Research Council Canada Graduate Scholarship to A. G. P. NR 47 TC 1 Z9 1 U1 7 U2 25 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 0021-8375 EI 1439-0361 J9 J ORNITHOL JI J. Ornithol. PD JAN PY 2016 VL 157 IS 1 BP 265 EP 275 DI 10.1007/s10336-015-1275-5 PG 11 WC Ornithology SC Zoology GA DB6FY UT WOS:000368610900027 ER PT J AU Breedy, O Guzman, HM AF Breedy, Odalisca Guzman, Hector M. TI A revision of the genus Muricea Lamouroux, 1821 (Anthozoa, Octocorallia) in the eastern Pacific. Part I: Eumuricea Verrill, 1869 revisited (vol 537, pg 1, 2015) SO ZOOKEYS LA English DT Correction C1 [Breedy, Odalisca] Univ Costa Rica, Ctr Invest Estruct Microscop, Ctr Invest Ciencias Mar & Limnol, San Jose, Costa Rica. [Breedy, Odalisca; Guzman, Hector M.] Smithsonian Trop Res Inst, Panama City, Panama. RP Breedy, O (reprint author), Univ Costa Rica, Ctr Invest Estruct Microscop, Ctr Invest Ciencias Mar & Limnol, POB 11501-2060, San Jose, Costa Rica. EM odaliscab@gmail.com NR 1 TC 0 Z9 0 U1 2 U2 2 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 553 BP 149 EP 153 DI 10.3897/zookeys.553.7471 PG 5 WC Zoology SC Zoology GA DB3GN UT WOS:000368398400008 PM 26877676 ER PT J AU Megeath, ST Gutermuth, R Muzerolle, J Kryukova, E Hora, JL Allen, LE Flaherty, K Hartmann, L Myers, PC Pipher, JL Stauffer, J Young, ET Fazio, GG AF Megeath, S. T. Gutermuth, R. Muzerolle, J. Kryukova, E. Hora, J. L. Allen, L. E. Flaherty, K. Hartmann, L. Myers, P. C. Pipher, J. L. Stauffer, J. Young, E. T. Fazio, G. G. TI THE SPITZER SPACE TELESCOPE SURVEY OF THE ORION A AND B MOLECULAR CLOUDS. II. THE SPATIAL DISTRIBUTION AND DEMOGRAPHICS OF DUSTY YOUNG STELLAR OBJECTS SO ASTRONOMICAL JOURNAL LA English DT Article DE infrared: stars; ISM: individual objects (Orion A, Orion B); stars: formation; stars: protostars; stars: variables: T Tauri, Herbig Ae/Be ID INITIAL MASS FUNCTION; FIELD EXTINCTION MAPS; STAR CLUSTER FORMATION; X-RAY-EMISSION; NEBULA-CLUSTER; PROTOPLANETARY DISKS; CIRCUMSTELLAR DISKS; TRAPEZIUM CLUSTER; SOLAR NEIGHBORHOOD; ULTRADEEP PROJECT AB We analyze the spatial distribution of dusty young stellar objects (YSOs) identified in the Spitzer Survey of the Orion Molecular clouds, augmenting these data with Chandra X-ray observations to correct for incompleteness in dense clustered regions. We also devise a scheme to correct for spatially varying incompleteness when X-ray data are not available. The local surface densities of the YSOs range from 1 pc(-2) to over 10,000 pc(-2), with protostars tending to be in higher density regions. This range of densities is similar to other surveyed molecular clouds with clusters, but broader than clouds without clusters. By identifying clusters and groups as continuous regions with surface densities >= 10 pc(-2), we find that 59% of the YSOs are in the largest cluster, the Orion Nebula Cluster (ONC), while 13% of the YSOs are found in a distributed population. A lower fraction of protostars in the distributed population is evidence that it is somewhat older than the groups and clusters. An examination of the structural properties of the clusters and groups shows that the peak surface densities of the clusters increase approximately linearly with the number of members. Furthermore, all clusters with more than 70 members exhibit asymmetric and/or highly elongated structures. The ONC becomes azimuthally symmetric in the inner 0.1 pc, suggesting that the cluster is only similar to 2 Myr in age. We find that the star formation efficiency (SFE) of the Orion B cloud is unusually low, and that the SFEs of individual groups and clusters are an order of magnitude higher than those of the clouds. Finally, we discuss the relationship between the young low mass stars in the Orion clouds and the Orion OB 1 association, and we determine upper limits to the fraction of disks that may be affected by UV radiation from OB stars or dynamical interactions in dense, clustered regions. C1 [Megeath, S. T.; Kryukova, E.] Univ Toledo, Dept Phys & Astron, Ritter Astrophs Res Ctr, Toledo, OH 43606 USA. [Megeath, S. T.] Max Planck Inst Radioastron, Completed Sabbat, D-53121 Bonn, Germany. [Gutermuth, R.] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA. [Muzerolle, J.] Space Telescope Sci Inst, Baltimore, MD 21218 USA. [Hora, J. L.; Myers, P. C.; Fazio, G. G.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Allen, L. E.] Natl Opt Astron Observ, Tucson, AZ 85719 USA. [Flaherty, K.] Univ Arizona, Steward Observ, Tucson, AZ 85721 USA. [Hartmann, L.] Univ Michigan, Dept Astron, Ann Arbor, MI 48109 USA. [Pipher, J. L.] Univ Rochester, Dept Phys & Astron, Rochester, NY 14627 USA. [Stauffer, J.] CALTECH, Spitzer Sci Ctr, Pasadena, CA 91125 USA. [Young, E. T.] SOFIA Univ Space Res Assoc, NASA Ames Res Ctr, Moffett Field, CA 94035 USA. RP Megeath, ST (reprint author), Univ Toledo, Dept Phys & Astron, Ritter Astrophs Res Ctr, Toledo, OH 43606 USA. EM megeath@physics.utoledo.edu FU National Aeronautics and Space Administration; National Science Foundation; NASA [960541, 960785]; NASA; JPL/Caltech FX This work benefited immeasurably from discussions with Fred Adams, John Bally, Cesar Briceno, Neal Evans, Gabor Furesz, Charlie Lada, Pavel Kroupa, Thomas Henning, Amy Stutz and Scott Wolk. The analysis of the data would not be possible without the superb support we received from the staff of the Spitzer Science Center. This publication makes use of data products from the 2MASS, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis. Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This work is based in part on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. It received support through that provided to the IRAC and MIPS instruments by NASA through contracts 960541 and 960785, respectively, issued by JPL. Support for this work was also provided by NASA through awards issued to S. T. M. and JLP by JPL/Caltech. This paper was mostly completed while S. T. M. was on sabbatical at the Max-Planck-Institut fur Radioastronomie and further revised while continuing his sabbatical at the Max-Planck-Institut fur Astronomine. S. T. M. thanks those institutes for their support. NR 149 TC 12 Z9 12 U1 0 U2 2 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-6256 EI 1538-3881 J9 ASTRON J JI Astron. J. PD JAN PY 2016 VL 151 IS 1 AR 5 DI 10.3847/0004-6256/151/1/5 PG 39 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB1EN UT WOS:000368250900005 ER PT J AU Balser, DS Roshi, DA Jeyakumar, S Bania, TM Montet, BT Shitanishi, JA AF Balser, Dana S. Roshi, D. Anish Jeyakumar, S. Bania, T. M. Montet, Benjamin T. Shitanishi, J. A. TI MAGNETIC FIELD STRENGTHS IN PHOTODISSOCIATION REGIONS SO ASTROPHYSICAL JOURNAL LA English DT Article DE H II regions; ISM: general; ISM: magnetic fields; photon-dominatedregion (PDR); radio lines: ISM ID H-II REGIONS; CARBON RECOMBINATION LINES; ULTRACOMPACT HII-REGIONS; WAY INTERSTELLAR-MEDIUM; MOLECULAR CLOUDS; STAR-FORMATION; ZEEMAN OBSERVATIONS; SUPERSONIC TURBULENCE; PHYSICAL-PROPERTIES; NGC 6334 AB We measure carbon radio recombination line (RRL) emission at 5.3 GHz toward four H II regions with the Green Bank Telescope to determine the magnetic field strength in the photodissociation region (PDR) that surrounds the ionized gas. Roshi suggests that the non-thermal line widths of carbon RRLs from PDRs are predominantly due to magneto-hydrodynamic waves, thus allowing the magnetic field strength to be derived. We model the PDR with a simple geometry and perform the non-LTE radiative transfer of the carbon RRL emission to solve for the PDR physical properties. Using the PDR mass density from these models and the carbon RRL non-thermal line width we estimate total magnetic field strengths of B similar to 100-300 mu G in W3 and NGC. 6334A. Our results for W49 and NGC. 6334D are less well constrained with total magnetic field strengths between B similar to 200-1000 mG. H I and OH Zeeman measurements of the line of sight magnetic field strength (B-los), taken from the literature, are between a factor of similar to 0.5-1 of the lower bound of our carbon RRL magnetic field strength estimates. Since vertical bar B-los vertical bar <= B, our results are consistent with the magnetic origin of the non-thermal component of carbon RRL widths. C1 [Balser, Dana S.; Roshi, D. Anish] Natl Radio Astron Observ, Charlottesville, VA 22903 USA. [Jeyakumar, S.] Univ Guanajuato, Dept Astron, Guanajuato 36000, Mexico. [Bania, T. M.] Boston Univ, Inst Astrophys Res, Dept Astron, Boston, MA 02215 USA. [Montet, Benjamin T.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Montet, Benjamin T.] Cahill Ctr Astron & Astrophys, Pasadena, CA 91125 USA. [Shitanishi, J. A.] Univ So Calif, Dept Phys & Astron, Los Angeles, CA 90089 USA. RP Balser, DS (reprint author), Natl Radio Astron Observ, 520 Edgemont Rd, Charlottesville, VA 22903 USA. OI Montet, Benjamin/0000-0001-7516-8308 NR 43 TC 0 Z9 0 U1 0 U2 0 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-637X EI 1538-4357 J9 ASTROPHYS J JI Astrophys. J. PD JAN 1 PY 2016 VL 816 IS 1 AR 22 DI 10.3847/0004-637X/816/1/22 PG 11 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB0VH UT WOS:000368225100022 ER PT J AU Saral, G Hora, JL Willis, SE Koenig, XP Gutermuth, RA Saygac, AT AF Saral, G. Hora, J. L. Willis, S. E. Koenig, X. P. Gutermuth, R. A. Saygac, A. T. TI YOUNG STELLAR OBJECTS IN THE MASSIVE STAR FORMING REGION W49 (vol 813, 25, 2015) SO ASTROPHYSICAL JOURNAL LA English DT Correction C1 [Saral, G.; Hora, J. L.; Willis, S. E.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Saral, G.] Istanbul Univ, Grad Sch Sci & Engn, Istanbul, Turkey. [Koenig, X. P.] Yale Univ, Dept Astron, New Haven, CT 06520 USA. [Gutermuth, R. A.] Univ Massachusetts, Dept Astron, Amherst, MA 01003 USA. [Saygac, A. T.] Istanbul Univ, Fac Sci, Astron & Space Sci Dept, Istanbul, Turkey. RP Saral, G (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM gsaral@cfa.harvard.edu NR 2 TC 1 Z9 1 U1 0 U2 0 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-637X EI 1538-4357 J9 ASTROPHYS J JI Astrophys. J. PD JAN 1 PY 2016 VL 816 IS 1 AR 47 DI 10.3847/0004-637X/816/1/47 PG 3 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB0VH UT WOS:000368225100047 ER PT J AU Steele, A Hughes, AM Carpenter, J Ricarte, A Andrews, SM Wilner, DJ Chiang, E AF Steele, Amy Hughes, A. Meredith Carpenter, John Ricarte, Angelo Andrews, Sean M. Wilner, David J. Chiang, Eugene TI RESOLVED MILLIMETER-WAVELENGTH OBSERVATIONS OF DEBRIS DISKS AROUND SOLAR-TYPE STARS SO ASTROPHYSICAL JOURNAL LA English DT Article DE circumstellar matter; planetary systems; submillimeter: planetary systems ID ANALOG HD 107146; BETA-PICTORIS B; SUN-LIKE STARS; PLANETARY SYSTEMS; KUIPER-BELT; HR 8799; ALMA OBSERVATIONS; AU-MICROSCOPII; FOMALHAUT B; SUBMILLIMETER OBSERVATIONS AB The presence of debris disks around young main-sequence stars hints at the existence and structure of planetary systems. Millimeter-wavelength observations probe large grains that trace the location of planetesimal belts. The Formation and Evolution of Planetary Systems Spitzer Legacy survey of nearby young solar analogues yielded a sample of five debris disk-hosting stars with millimeter flux suitable for interferometric follow-up. We present observations with the Submillimeter Array (SMA) and the Combined Array for Research in Millimeter-wave Astronomy at similar to 2 '' resolution that spatially resolve the debris disks around these nearby (d similar to 50 pc) stars. Two of the five disks (HD 377, HD 8907) are spatially resolved for the first time and one (HD 104860) is resolved at millimeter wavelengths for the first time. We combine our new observations with archival SMA and Atacama Large Millimeter/Submillimeter Array data to enable a uniform analysis of the full five-object sample. We simultaneously model the broadband photometric data and resolved millimeter visibilities to constrain the dust temperatures and disk morphologies, and perform a Markov Chain Monte Carlo analysis to fit for basic structural parameters. We find that the radii and widths of the cold outer belts exhibit properties consistent with scaled-up versions of the Solar System' s Kuiper Belt. All the disks exhibit characteristic grain sizes comparable to the blowout size, and all the resolved observations of emission from large dust grains are consistent with an axisymmetric dust distribution to within the uncertainties. These results are consistent with comparable studies carried out at infrared wavelengths. C1 [Steele, Amy; Hughes, A. Meredith] Wesleyan Univ, Dept Astron, Van Vleck Observ, Middletown, CT 06459 USA. [Steele, Amy] Univ Maryland, Dept Astron, College Pk, MD 20742 USA. [Carpenter, John] CALTECH, Div Phys Math & Astron, Pasadena, CA 91125 USA. [Ricarte, Angelo] Yale Univ, Dept Astron, JW Gibbs Lab, New Haven, CT 06511 USA. [Andrews, Sean M.; Wilner, David J.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Chiang, Eugene] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA. RP Steele, A (reprint author), Wesleyan Univ, Dept Astron, Van Vleck Observ, 96 Foss Hill Dr, Middletown, CT 06459 USA. EM asteele@wesleyan.edu FU National Radio Astronomy Observatory; NASA Origins of Solar Systems [NNX13AI32G]; NSF [AST-1412647]; Gordon and Betty Moore Foundation; Associates of the California Institute of Technology; University of Chicago; state of California; state of Illinois; state of Maryland; National Science Foundation; CARMA; Kenneth T. and Eileen L. Norris Foundation; James S. McDonnell Foundation FX The work of A. S. was supported by a Student Observing Support grant from the National Radio Astronomy Observatory. A.M.H. gratefully acknowledges support from NASA Origins of Solar Systems grant NNX13AI32G and NSF grant AST-1412647. Support for CARMA construction was derived from the Gordon and Betty Moore Foundation, the Kenneth T. and Eileen L. Norris Foundation, the James S. McDonnell Foundation, the Associates of the California Institute of Technology, the University of Chicago, the states of California, Illinois, and Maryland, and the National Science Foundation. CARMA development and operations were supported by the National Science Foundation under a cooperative agreement, and by the CARMA partner universities. This paper makes use of the following ALMA data: ADS/JAO. ALMA#2011.0.00470. S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013). NR 88 TC 3 Z9 3 U1 0 U2 0 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-637X EI 1538-4357 J9 ASTROPHYS J JI Astrophys. J. PD JAN 1 PY 2016 VL 816 IS 1 AR 27 DI 10.3847/0004-637X/816/1/27 PG 14 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB0VH UT WOS:000368225100027 ER PT J AU Tajfirouze, E Reale, F Petralia, A Testa, P AF Tajfirouze, E. Reale, F. Petralia, A. Testa, P. TI TIME-RESOLVED EMISSION FROM BRIGHT HOT PIXELS OF AN ACTIVE REGION OBSERVED IN THE EUV BAND WITH SDO/AIA AND MULTI-STRANDED LOOP MODELING SO ASTROPHYSICAL JOURNAL LA English DT Article DE Sun: activity; Sun: corona; Sun: UV radiation ID HINODE/X-RAY TELESCOPE; SOLAR CORONAL LOOPS; NANOFLARE MODEL; DYNAMICS; PLASMA AB Evidence of small amounts of very hot plasma has been found in active regions and might be an indication of impulsive heating released at spatial scales smaller than the cross-section of a single loop. We investigate the heating and substructure of coronal loops in the core of one such active region by analyzing the light curves in the smallest resolution elements of solar observations in two EUV channels (94 and 335 A) from the Atmospheric Imaging Assembly on board the Solar Dynamics Observatory. We model the evolution of a bundle of strands heated by a storm of nanoflares by means of a hydrodynamic 0D loop model (EBTEL). The light curves obtained from a random combination of those of single strands are compared to the observed light curves either in a single pixel or in a row of pixels, simultaneously in the two channels, and using two independent methods: an artificial intelligent system (Probabilistic Neural Network) and a simple cross-correlation technique. We explore the space of the parameters to constrain the distribution of the heat pulses, their duration, their spatial size, and, as a feedback on the data, their signatures on the light curves. From both methods the best agreement is obtained for a relatively large population of events (1000) with a short duration (less than 1 minute) and a relatively shallow distribution (power law with index 1.5) in a limited energy range (1.5 decades). The feedback on the data indicates that bumps in the light curves, especially in the 94 A, are signatures of a heating excess that occurred a few minutes before. C1 [Tajfirouze, E.; Reale, F.; Petralia, A.] Univ Palermo, Dipartimento Fis & Chim, Piazza Parlamento 1, I-90134 Palermo, Italy. [Reale, F.] INAF Osservatorio Astron Palermo, I-90134 Palermo, Italy. [Testa, P.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. RP Tajfirouze, E (reprint author), Univ Palermo, Dipartimento Fis & Chim, Piazza Parlamento 1, I-90134 Palermo, Italy. EM aastex-help@aas.org OI Petralia, Antonino/0000-0002-9882-1020; Reale, Fabio/0000-0002-1820-4824 FU Italian Ministero dell'Universita e Ricerca; Lockheed-Martin [SP02H1701R]; NASA [NNX15AF50G] FX We thank the referee for very constructive comments, and Dr. T. Di Salvo for suggestions. E.T., F.R., and A.P. acknowledge support from Italian Ministero dell'Universita e Ricerca. P.T. was supported by contract SP02H1701R from Lockheed-Martin to the Smithsonian Astrophysical Observatory, and by NASA grant NNX15AF50G. SDO data was supplied courtesy of the SDO/AIA consortia. SDO is the first mission to be launched for NASA's Living With a Star (LWS) Program. NR 39 TC 4 Z9 4 U1 1 U2 1 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-637X EI 1538-4357 J9 ASTROPHYS J JI Astrophys. J. PD JAN 1 PY 2016 VL 816 IS 1 AR 12 DI 10.3847/0004-637X/816/1/12 PG 12 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB0VH UT WOS:000368225100012 ER PT J AU Ting, YS Conroy, C Rix, HW AF Ting, Yuan-Sen Conroy, Charlie Rix, Hans-Walter TI APOGEE CHEMICAL TAGGING CONSTRAINT ON THE MAXIMUM STAR CLUSTER MASS IN THE alpha-ENHANCED GALACTIC DISK SO ASTROPHYSICAL JOURNAL LA English DT Article DE Galaxy: abundances; Galaxy: disk; Galaxy: evolution; Galaxy: formation; ISM: abundances; stars: abundances ID MILKY-WAY DISK; FORMING GALAXIES; RADIAL MIGRATION; ELEMENTAL ABUNDANCE; SOLAR NEIGHBORHOOD; HIGH-REDSHIFT; STELLAR POPULATIONS; SCALE LENGTH; MOVING GROUP; THICK DISK AB Stars born from the same molecular cloud should be nearly homogeneous in their element abundances. The concept of chemical tagging is to identify members of disrupted clusters by their clustering in element abundance space. Chemical tagging requires large samples of stars with precise abundances for many individual elements. With uncertainties of sigma([X/Fe]) and sigma([Fe/H]) similar or equal to 0.05 for 10 elements measured for >10(4) stars, the APOGEE DR12 spectra may be the first well-suited data set to put this idea into practice. We find that even APOGEE data offer only similar to 500 independent volume elements in the 10-dimensional abundance space, when we focus on the a-enhanced Galactic disk. We develop and apply a new algorithm to search for chemically homogeneous sets of stars against a dominant background. By injecting star clusters into the APOGEE data set, we show that chemically homogeneous clusters with masses. 3 x 10(7) M-circle dot would be easily detectable and yet no such signal is seen in the data. By generalizing this approach, we put a first abundance-based constraint on the cluster mass function for the old disk stars in the Milky Way. C1 [Ting, Yuan-Sen; Conroy, Charlie] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Rix, Hans-Walter] Max Planck Inst Astron, D-69117 Heidelberg, Germany. RP Ting, YS (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. OI Ting, Yuan-Sen/0000-0001-5082-9536 FU National Science Foundation [NSF PHY11-25915]; Max-Planck-Institut fur Astronomie; DFG [SFB 881 (A3)]; European Research Council under the European Union's Seventh Framework Programme (FP 7) ERC [321035] FX We thank the referees for the careful and insightful comments. This research was inspired at the KITP Galatic Archaeology and Precision Stellar Astrophysics workshop in year 2015 and was supported in part by the National Science Foundation under Grant No. NSF PHY11-25915. Y.S.T. is grateful to the Max-Planck-Institut fur Astronomie and the DFG through the SFB 881 (A3) for their hospitality and financial support during the period in which part of this research was performed. H.W.R.'s research contribution is supported by the European Research Council under the European Union's Seventh Framework Programme (FP 7) ERC grant agreement No. [321035]. NR 94 TC 6 Z9 6 U1 2 U2 2 PU IOP PUBLISHING LTD PI BRISTOL PA TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND SN 0004-637X EI 1538-4357 J9 ASTROPHYS J JI Astrophys. J. PD JAN 1 PY 2016 VL 816 IS 1 AR 10 DI 10.3847/0004-637X/816/1/10 PG 12 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DB0VH UT WOS:000368225100010 ER PT J AU Pereyra, MO Baldo, D Blotto, BL Iglesias, PP Thome, MTC Haddad, CFB Barrio-Amoros, C Ibanez, R Faivovich, J AF Pereyra, Martin O. Baldo, Diego Blotto, Boris L. Iglesias, Patricia P. Thome, Maria T. C. Haddad, Celio F. B. Barrio-Amoros, Cesar Ibanez, Roberto Faivovich, Julian TI Phylogenetic relationships of toads of the Rhinella granulosa group (Anura: Bufonidae): a molecular perspective with comments on hybridization and introgression SO CLADISTICS LA English DT Article ID SOUTH-AMERICAN TOADS; NATURAL HYBRIDIZATION; BUFO ANURA; MELANOPHRYNISCUS-GALLARDO; NEOTROPICAL TOADS; SPECIES COMPLEX; LIFE-HISTORY; HYBRID ZONE; GENE FLOW; BIOGEOGRAPHY AB The Rhinella granulosa group consists of 13 species of toads distributed throughout open areas of South America and Panama. In this paper we perform a phylogenetic analysis considering all but one species of the group, employing five nuclear and four mitochondrial genes, for up to 7910 bp per specimen. Separate phylogenetic analyses under direct optimization (DO) of nuclear and mitochondrial sequences recovered the R. granulosa group as monophyletic and revealed topological incongruence that can be explained mainly by multiple events of hybridization and introgression, both mitochondrial and nuclear. The DO combined analysis, after the exclusion of putatively introgressed or heterozygous genomes, resulted in a phylogenetic hypothesis for the R. granulosa group in which most of the species are recovered as monophyletic, but with interspecific relationships poorly supported. The optimization of morphological (adult and larval), chromosomal, and behavioural characters resulted in 12 putative phenotypic synapomorphies for this species group and some other synapomorphies for internal clades. Our results indicate the need for additional population genetic studies on R. dorbignyi and R. fernandezae to corroborate the taxonomic status of both taxa. Finally, we discuss biological and genetic characteristics of Bufonidae, as possible explanations for the common occurrence of hybridization and introgression observed in some lineages of this family. (C) The Willi Hennig Society 2015. C1 [Pereyra, Martin O.; Blotto, Boris L.; Faivovich, Julian] Consejo Nacl Invest Cient & Tecn, Museo Argentino Ciencias Nat Bernardino Rivadavia, Div Herpetol, Buenos Aires, DF, Argentina. [Baldo, Diego] Univ Nacl Misiones, Lab Genet Evolut, Inst Biol Subtrop CONICET UNaM, Fac Ciencias Exactas Quim & Nat, Posadas, Misiones, Argentina. [Blotto, Boris L.] Univ Sao Paulo, Inst Biociencias, Dept Zool, BR-05508090 Sao Paulo, SP, Brazil. [Iglesias, Patricia P.] Univ Buenos Aires, Inst Ecol Genet & Evoluc Buenos Aires, Fac Ciencias Exactas & Nat, IEGEBA CONICET,Inst Ecol Genet & Evoluc, Buenos Aires, DF, Argentina. [Thome, Maria T. C.; Haddad, Celio F. B.] Univ Estadual Paulista, UNESP, Dept Zool, Inst Biociencias, BR-13506900 Rio Claro, SP, Brazil. [Barrio-Amoros, Cesar] Inst Biodiversidad Trop, Perez Zeledon 11901, San Isidro Del, Costa Rica. [Ibanez, Roberto] Smithsonian Trop Res Inst, Balboa, Panama. [Ibanez, Roberto] Univ Panama, Dept Zool, Panama City, Panama. [Ibanez, Roberto] Estafeta Univ, Circulo Herpetol Panama, Panama City, Panama. [Faivovich, Julian] Univ Buenos Aires, Fac Ciencias Exactas & Nat, Dept Biodiversidad & Biol Expt, Buenos Aires, DF, Argentina. RP Faivovich, J (reprint author), Consejo Nacl Invest Cient & Tecn, Museo Argentino Ciencias Nat Bernardino Rivadavia, Div Herpetol, Angel Gallardo 470,C1405DJR, Buenos Aires, DF, Argentina. EM julian@macn.gov.ar RI Haddad, Celio/C-4267-2012; OI Baldo, Diego/0000-0003-2382-0872 FU Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET); ANPCyT; Universidad de Buenos Aires; Sistema Nacional de Investigacion de Panama; Fundacao de Amparo a Pesquisa do Estado de Sao Paulo [PIP 1112008010-2422, 11220110100875, PIP 112201101-00889, PICT 2007-2202, 20111524, 2011-1895, 2012-2687, 404-2013, UBACyT 20020090200727, 20020110200213, 2013/50741-7]; Sao Paulo Research Foundation (FAPESP) FX We thank J. M. Padial, S. Castroviejo, M. T. Rodrigues, F. Kolenc, C. Borteiro, S. Sucre, E. A. Sanabria, L. B. Quiroga, S. J. Nenda, D. A. Barrasso, V. G. D. Orrico, F. Brusquetti, and F. Netto for sharing with us specimens, tissue samples and/or DNA sequences. T. Grant, A. Kwet, R. Montesinos, M. Rivera-Correa, A. Fouquet, and C. Marty sent us photographs of some specimens. T. Grant helped with the analyses done in the Museu de Zoologia da Universidade de Sao Paulo (MZUSP) cluster. F. Vargas-Salinas, Z. Tarano, A. Garda, T. R. de Carvalho, and A. R. de Morais kindly shared with us information about advertisement calls of some species. For comments on the manuscript and discussions we thank C. Borteiro and F. Kolenc. We thank E. O. Lavilla, S. Kretzschmar, M. Canepa (Fundacion Miguel Lillo, Tucuman, Argentina), H. Zaher and T. Grant (MZUSP), and M. T. Rodrigues (Universidade de Sao Paulo) for allowing us to study vouchers under their care. We thank Consejo Nacional de Investigaciones Cientificas y Tecnicas (CONICET), ANPCyT, Universidad de Buenos Aires, Sistema Nacional de Investigacion de Panama, and Fundacao de Amparo a Pesquisa do Estado de Sao Paulo for financial support: PIP 1112008010-2422, 11220110100875, PIP 112201101-00889; PICT 2007-2202, 20111524, 2011-1895, 2012-2687, and 404-2013; UBACyT 20020090200727 and 20020110200213; and Grants 2013/50741-7 and 2013/50741-7, Sao Paulo Research Foundation (FAPESP). The Centro de Estudos de Insetos Sociais, I. B., UNESP, Rio Claro allowed access to its molecular laboratory facilities for the production of some sequences used in this study. Specimens from Venezuela were collected under permit issued by the Ministerio del Ambiente de Venezuela number 2231, and permit to access to Genetic resources to Fundacion AndigenA. Specimens from Panama were collected under permit No. SE/A-130-10 granted by the Autoridad Nacional del Ambiente. NR 121 TC 4 Z9 4 U1 1 U2 4 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0748-3007 EI 1096-0031 J9 CLADISTICS JI Cladistics PD JAN PY 2016 VL 32 IS 1 BP 36 EP 53 DI 10.1111/cla.12110 PG 18 WC Evolutionary Biology SC Evolutionary Biology GA DA6OD UT WOS:000367923600003 ER PT J AU Miller, AD Dietze, MC DeLucia, EH Anderson-Teixeira, KJ AF Miller, Adam D. Dietze, Michael C. DeLucia, Evan H. Anderson-Teixeira, Kristina J. TI Alteration of forest succession and carbon cycling under elevated CO2 SO GLOBAL CHANGE BIOLOGY LA English DT Article DE climate change; duke FACE; ecosystem demography model; forest regeneration; succession; simulation ID NET ECOSYSTEM EXCHANGE; PINUS-TAEDA L.; TERRESTRIAL BIOSPHERE; ATMOSPHERIC CO2; NITROGEN AVAILABILITY; SPECIES-RICHNESS; CLIMATE-CHANGE; UNITED-STATES; MODEL; ENRICHMENT AB Regenerating forests influence the global carbon (C) cycle, and understanding how climate change will affect patterns of regeneration and C storage is necessary to predict the rate of atmospheric carbon dioxide (CO2) increase in future decades. While experimental elevation of CO2 has revealed that young forests respond with increased productivity, there remains considerable uncertainty as to how the long-term dynamics of forest regrowth are shaped by elevated CO2 (eCO(2)). Here, we use the mechanistic size- and age- structured Ecosystem Demography model to investigate the effects of CO2 enrichment on forest regeneration, using data from the Duke Forest Free-Air Carbon dioxide Enrichment (FACE) experiment, a forest chronosequence, and an eddy-covariance tower for model parameterization and evaluation. We find that the dynamics of forest regeneration are accelerated, and stands consistently hit a variety of developmental benchmarks earlier under eCO(2). Because responses to eCO(2) varied by plant functional type, successional pathways, and mature forest composition differed under eCO(2), with mid- and late-successional hardwood functional types experiencing greater increases in biomass compared to early-successional functional types and the pine canopy. Over the simulation period, eCO(2) led to an increase in total ecosystem C storage of 9.7 Mg C ha(-1). Model predictions of mature forest biomass and ecosystem-atmosphere exchange of CO2 and H2O were sensitive to assumptions about nitrogen limitation; both the magnitude and persistence of the ecosystem response to eCO(2) were reduced under N limitation. In summary, our simulations demonstrate that eCO(2) can result in a general acceleration of forest regeneration while altering the course of successional change and having a lasting impact on forest ecosystems. C1 [Miller, Adam D.; Anderson-Teixeira, Kristina J.] Natl Zool Pk, Conservat Ecol Ctr, Smithsonian Conservat Biol Inst, Front Royal, VA 22630 USA. [Miller, Adam D.; DeLucia, Evan H.] Univ Illinois, Inst Sustainabil Energy & Environm, Urbana, IL 61801 USA. [Dietze, Michael C.] Boston Univ, Dept Earth & Environm, Boston, MA 02215 USA. [DeLucia, Evan H.] Univ Illinois, Dept Plant Biol, Urbana, IL 61801 USA. [Anderson-Teixeira, Kristina J.] Smithsonian Trop Res Inst, Forest Global Earth Observ, Ctr Trop Forest Sci, Panama City, Panama. RP Anderson-Teixeira, KJ (reprint author), Natl Zool Pk, Conservat Ecol Ctr, Smithsonian Conservat Biol Inst, 1500 Remount Rd, Front Royal, VA 22630 USA. EM TeixeiraK@si.edu FU DOE [DE-SC0010039, DE-SC0008085]; NSF ABI [1062547] FX The authors thank Jackie Mohan, John Drake, David LeBauer, Jenny McGarvey, Sara Childs, and Maria Wang for helpful discussion. This research was funded by DOE award #DE-SC0010039 / #DE-SC0008085 to KAT and EHD, with support to MCD from NSF ABI #1062547. The authors have no conflict of interests. NR 65 TC 1 Z9 1 U1 11 U2 47 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1354-1013 EI 1365-2486 J9 GLOBAL CHANGE BIOL JI Glob. Change Biol. PD JAN PY 2016 VL 22 IS 1 BP 351 EP 363 DI 10.1111/gcb.13077 PG 13 WC Biodiversity Conservation; Ecology; Environmental Sciences SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DA7KL UT WOS:000367982900028 PM 26316364 ER PT J AU Pastore, MA Megonigal, JP Langley, JA AF Pastore, Melissa A. Megonigal, J. Patrick Langley, J. Adam TI Elevated CO2 promotes long-term nitrogen accumulation only in combination with nitrogen addition SO GLOBAL CHANGE BIOLOGY LA English DT Article DE brackish marsh; CO2 enrichment; denitrification; isotopic biogeochemistry; nitrogen pollution; nitrogen retention and loss ID SALT-MARSH SEDIMENTS; COASTAL MARINE ECOSYSTEMS; SUBTROPICAL OAK WOODLAND; CHESAPEAKE BAY WETLAND; SOIL ORGANIC-MATTER; SEA-LEVEL RISE; CARBON-DIOXIDE; TERRESTRIAL ECOSYSTEMS; FRESH-WATER; RESPONSES AB Biogeochemical models that incorporate nitrogen (N) limitation indicate that N availability will control the magnitude of ecosystem carbon uptake in response to rising CO2. Some models, however, suggest that elevated CO2 may promote ecosystem N accumulation, a feedback that in the long term could circumvent N limitation of the CO2 response while mitigating N pollution. We tested this prediction using a nine-year CO(2)xN experiment in a tidal marsh. Although the effects of CO2 are similar between uplands and wetlands in many respects, this experiment offers a greater likelihood of detecting CO2 effects on N retention on a decadal timescale because tidal marshes have a relatively open N cycle and can accrue soil organic matter rapidly. To determine how elevated CO2 affects N dynamics, we assessed the three primary fates of N in a tidal marsh: (1) retention in plants and soil, (2) denitrification to the atmosphere, and (3) tidal export. We assessed changes in N pools and tracked the fate of a N-15 tracer added to each plot in 2006 to quantify the fraction of added N retained in vegetation and soil, and to estimate lateral N movement. Elevated CO2 alone did not increase plant N mass, soil N mass, or N-15 label retention. Unexpectedly, CO2 and N interacted such that the combined N+CO2 treatment increased ecosystem N accumulation despite the stimulation in N losses indicated by reduced N-15 label retention. These findings suggest that in N-limited ecosystems, elevated CO2 is unlikely to increase long-term N accumulation and circumvent progressive N limitation without additional N inputs, which may relieve plant-microbe competition and allow for increased plant N uptake. C1 [Pastore, Melissa A.; Langley, J. Adam] Villanova Univ, Dept Biol, Villanova, PA 19085 USA. [Megonigal, J. Patrick; Langley, J. Adam] Smithsonian Environm Res Ctr, Edgewater, MD 21037 USA. RP Pastore, MA (reprint author), Villanova Univ, Dept Biol, 800 Lancaster Ave, Villanova, PA 19085 USA. EM lispastore@gmail.com FU NSF-LTREB Program [DEB-0950080, DEB-1457100]; Smithsonian Institution; Villanova University FX The authors thank J. Duls, G. Peresta, and A. Peresta for assistance with data collection and maintenance of the experiment and treatments at the Smithsonian Global Change Research Wetland. We also thank Melanie Vile for her insight and expertise in measuring gas fluxes, as well as three anonymous reviewers for their helpful comments. This work was supported by NSF-LTREB Program Grants DEB-0950080 and DEB-1457100, the Smithsonian Institution, and Villanova University. NR 65 TC 2 Z9 2 U1 17 U2 47 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1354-1013 EI 1365-2486 J9 GLOBAL CHANGE BIOL JI Glob. Change Biol. PD JAN PY 2016 VL 22 IS 1 BP 391 EP 403 DI 10.1111/gcb.13112 PG 13 WC Biodiversity Conservation; Ecology; Environmental Sciences SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DA7KL UT WOS:000367982900031 PM 26577708 ER PT J AU Mueller, P Jensen, K Megonigal, JP AF Mueller, Peter Jensen, Kai Megonigal, James Patrick TI Plants mediate soil organic matter decomposition in response to sea level rise SO GLOBAL CHANGE BIOLOGY LA English DT Article DE blue carbon; carbon sequestration; marsh organ; priming; Schoenoplectus; soil elevation; tidal wetland stability ID RADIAL OXYGEN LOSS; TIDAL MARSHES; ELEVATED CO2; SALT-MARSH; PHOTOSYNTHESIS CONTROLS; METHANE EMISSIONS; ABIOTIC FACTORS; CLIMATE-CHANGE; CARBON; RHIZOSPHERE AB Tidal marshes have a large capacity for producing and storing organic matter, making their role in the global carbon budget disproportionate to land area. Most of the organic matter stored in these systems is in soils where it contributes 2-5 times more to surface accretion than an equal mass of minerals. Soil organic matter (SOM) sequestration is the primary process by which tidal marshes become perched high in the tidal frame, decreasing their vulnerability to accelerated relative sea level rise (RSLR). Plant growth responses to RSLR are well understood and represented in century-scale forecast models of soil surface elevation change. We understand far less about the response of SOM decomposition to accelerated RSLR. Here we quantified the effects of flooding depth and duration on SOM decomposition by exposing planted and unplanted field-based mesocosms to experimentally manipulated relative sea level over two consecutive growing seasons. SOM decomposition was quantified as CO2 efflux, with plant- and SOM-derived CO2 separated via (CO2)-C-13. Despite the dominant paradigm that decomposition rates are inversely related to flooding, SOM decomposition in the absence of plants was not sensitive to flooding depth and duration. The presence of plants had a dramatic effect on SOM decomposition, increasing SOM-derived CO2 flux by up to 267% and 125% (in 2012 and 2013, respectively) compared to unplanted controls in the two growing seasons. Furthermore, plant stimulation of SOM decomposition was strongly and positively related to plant biomass and in particular aboveground biomass. We conclude that SOM decomposition rates are not directly driven by relative sea level and its effect on oxygen diffusion through soil, but indirectly by plant responses to relative sea level. If this result applies more generally to tidal wetlands, it has important implications for models of SOM accumulation and surface elevation change in response to accelerated RSLR. C1 [Mueller, Peter; Jensen, Kai] Univ Hamburg, Appl Plant Ecol, Bioctr Klein Flottbek, D-22609 Hamburg, Germany. [Megonigal, James Patrick] Smithsonian Environm Res Ctr, Edgewater, MD 21037 USA. RP Mueller, P (reprint author), Univ Hamburg, Appl Plant Ecol, Bioctr Klein Flottbek, Ohnhorststr 18, D-22609 Hamburg, Germany. EM peter.mueller@uni-hamburg.de; megonigalp@si.edu RI Jensen, Kai/L-6657-2015 FU Smithsonian Institution's Graduate Student Fellowship Program; University of Hamburg; Student Research Grant Program of the Society of Wetland Scientists; Smithsonian Institution; NSF-LTREB Program [DEB-0950080]; Maryland Sea Grant [SA7528114-WW]; US Department of Energy [DE-FG02-97ER62458] FX We thank J. Duls, A. Peresta, J. Meschter, G. Peresta, and K. Pannier for their help with field and laboratory work. Financial support was provided to P. Mueller through the Smithsonian Institution's Graduate Student Fellowship Program, the University of Hamburg, and the Student Research Grant Program of the Society of Wetland Scientists. The field study was supported by the Smithsonian Institution, the NSF-LTREB Program (DEB-0950080), Maryland Sea Grant (SA7528114-WW), and the US Department of Energy (DE-FG02-97ER62458). Use of trade, product, or firm names does not imply endorsement by the US government. NR 65 TC 5 Z9 5 U1 21 U2 73 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1354-1013 EI 1365-2486 J9 GLOBAL CHANGE BIOL JI Glob. Change Biol. PD JAN PY 2016 VL 22 IS 1 BP 404 EP 414 DI 10.1111/gcb.13082 PG 11 WC Biodiversity Conservation; Ecology; Environmental Sciences SC Biodiversity & Conservation; Environmental Sciences & Ecology GA DA7KL UT WOS:000367982900032 PM 26342160 ER PT J AU Jung, JH Choi, JM Coats, DW Kim, YO AF Jung, Jae-Ho Choi, Jung Min Coats, D. Wayne Kim, Young-Ok TI Euduboscquella costata n. sp (Dinoflagellata, Syndinea), an Intracellular Parasite of the Ciliate Schmidingerella arcuata: Morphology, Molecular Phylogeny, Life Cycle, Prevalence, and Infection Intensity SO JOURNAL OF EUKARYOTIC MICROBIOLOGY LA English DT Article DE 18S ribosomal RNA; marine intracellular parasite; plankton; Syndinean dinoflagellate; tintinnid ID HOST EUTINTINNUS-PECTINIS; DUBOSCQUELLA-CACHONI; MAXIMUM-LIKELIHOOD; FAVELLA-PANAMENSIS; COASTAL WATERS; DIVERSITY; MODELS AB The syndinean dinoflagellate Euduboscquella costata n. sp., an intracellular parasite of the tintinnid ciliate Schmidingerella arcuata, was discovered from Korean coastal water in November of 2013. Euduboscquella costata parasitized in about 62% of the host population, with infection intensity (- number of trophonts in a single host cell) ranging from 1 to 8. Based on morphology and nuclear 18S ribosomal RNA gene sequences, the parasite is new to science. Euduboscquella costata n. sp. had an infection cycle typical of the genus, but had morphological and developmental features that distinguished it from congeneric species. These features include: (1) episome of the trophont with 2540 grooves converging toward the center of the shield; (2) a narrow, funnel-shaped lamina pharyngea extending from the margin of the episomal shield to the nucleus; (3) persistence of grooves during extracellular development (sporogenesis); (4) a single food vacuole during sporogenesis; (5) separation of sporocytes early in sporogenesis, regardless of type of spore formed; and (6) dinospore size (ca. 14 mu m in length) and shape (bulbous episome with narrower, tapering hyposome). After sporogenesis, E. costata produced four different types of spore that showed completely identical 18S rRNA gene sequences. The gene sequence was completely identical with a previously reported population, Euduboscquella sp. ex S. arcuata, from Assawoman Bay, USA, indicating that the two populations are likely conspecific. Favella ehrenbergii, a widely recorded tintinnid known to host Euduboscquella spp., co-occurred with S. arcuata, but was not infected by E. costata in field samples or during short-term, cross-infection experiments. C1 [Jung, Jae-Ho; Choi, Jung Min; Kim, Young-Ok] Korea Inst Ocean Sci & Technol, Jangmok Myon 656834, Geoje, South Korea. [Coats, D. Wayne] Smithsonian Environm Res Ctr, Edgewater, MD 21037 USA. RP Kim, YO (reprint author), Korea Inst Ocean Sci & Technol, 41 Jangmok 1, Jangmok Myon 656834, Geoje, South Korea. EM yokim@kiost.ac FU KIOST project [PE99193] FX This research was supported by KIOST projects (PE99193). NR 26 TC 0 Z9 0 U1 2 U2 7 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1066-5234 EI 1550-7408 J9 J EUKARYOT MICROBIOL JI J. Eukaryot. Microbiol. PD JAN-FEB PY 2016 VL 63 IS 1 BP 3 EP 15 DI 10.1111/jeu.12231 PG 13 WC Microbiology SC Microbiology GA DA9LZ UT WOS:000368131600001 PM 25963420 ER PT J AU Bentlage, B Rogers, TS Bachvaroff, TR Delwiche, CF AF Bentlage, Bastian Rogers, Travis S. Bachvaroff, Tsvetan R. Delwiche, Charles F. TI Complex Ancestries of Isoprenoid Synthesis in Dinoflagellates SO JOURNAL OF EUKARYOTIC MICROBIOLOGY LA English DT Article DE Dinoflagellata; DOXP; endosymbiont gene transfer; Haptophyta; MEP; mevalonate; MVA ID PHYLOGENETIC TREE SELECTION; HORIZONTAL GENE-TRANSFER; NON-MEVALONATE PATHWAY; PLASTID-DERIVED GENES; TERTIARY ENDOSYMBIOSIS; KARLODINIUM-VENEFICUM; RIBOSOMAL-PROTEINS; SEQUENCE ALIGNMENT; PERKINSUS-MARINUS; GENOME EVOLUTION AB Isoprenoid metabolism occupies a central position in the anabolic metabolism of all living cells. In plastid-bearing organisms, two pathways may be present for de novo isoprenoid synthesis, the cytosolic mevalonate pathway (MVA) and nuclear-encoded, plastid-targeted nonmevalonate pathway (DOXP). Using transcriptomic data we find that dinoflagellates apparently make exclusive use of the DOXP pathway. Using phylogenetic analyses of all DOXP genes we inferred the evolutionary origins of DOXP genes in dinoflagellates. Plastid replacements led to a DOXP pathway of multiple evolutionary origins. Dinoflagellates commonly referred to as dinotoms due to their relatively recent acquisition of a diatom plastid, express two completely redundant DOXP pathways. Dinoflagellates with a tertiary plastid of haptophyte origin, by contrast, express a hybrid pathway of dual evolutionary origin. Here, changes in the targeting motif of signal/transit peptide likely allow for targeting the new plastid by the proteins of core isoprenoid metabolism proteins. Parasitic dinoflagellates of the Amoebophyra species complex appear to have lost the DOXP pathway, suggesting that they may rely on their host for sterol synthesis. C1 [Bentlage, Bastian; Rogers, Travis S.; Delwiche, Charles F.] Univ Maryland, CMNS Cell Biol & Mol Genet, College Pk, MD 20742 USA. [Bachvaroff, Tsvetan R.] Univ Maryland, Ctr Environm Sci, Inst Marine & Environm Technol, Baltimore, MD 21202 USA. [Delwiche, Charles F.] Univ Maryland, Maryland Agr Expt Stn, AGNR, College Pk, MD 20742 USA. RP Bentlage, B (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Invertebrate Zool, MRC 163,POB 37012, Washington, DC 20013 USA. EM bastian.bentlage@gmail.com FU NSF [DEB-1036506, DEB-1046075, DEB-0629624] FX We thank Endymion Cooper for generously sharing unpublished green algal transcriptome assemblies and Gregory Mendez for insightful discussions. We are also indebted for two reviewers who provided critical comments that helped us improve an earlier version of this manuscript. Funding for this project came through NSF grants DEB-1036506, DEB-1046075, and DEB-0629624. TR wishes to acknowledge an HHMI International Research Program Supplement. NR 80 TC 0 Z9 0 U1 2 U2 7 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1066-5234 EI 1550-7408 J9 J EUKARYOT MICROBIOL JI J. Eukaryot. Microbiol. PD JAN-FEB PY 2016 VL 63 IS 1 BP 123 EP 137 DI 10.1111/jeu.12261 PG 15 WC Microbiology SC Microbiology GA DA9LZ UT WOS:000368131600013 PM 26291956 ER PT J AU Yap, SL Davies, SJ Condit, R AF Yap, Sandra L. Davies, Stuart J. Condit, Richard TI Dynamic response of a Philippine dipterocarp forest to typhoon disturbance SO JOURNAL OF VEGETATION SCIENCE LA English DT Article DE Biomass; Dipterocarp forest; Forest dynamics; Forest resilience; Mortality and recruitment; Regeneration; Tree demography; Typhoon disturbance ID LUQUILLO-EXPERIMENTAL-FOREST; BISLEY EXPERIMENTAL WATERSHEDS; SUBTROPICAL WET FOREST; TROPICAL RAIN-FOREST; PUERTO-RICO; HURRICANE-HUGO; ABOVEGROUND BIOMASS; CATASTROPHIC WIND; DAMAGE; RECOVERY AB Questions: Natural hazards can wreak catastrophic damage to forest ecosystems. Here, the effects of typhoon disturbance on forest structure and demography of the 16- ha Palanan Forest Dynamics Plot in the northeast Philippines were examined by comparing census intervals with ( 1998- 2004) and without ( 2004- 2010) a strong typhoon. Category 4 Typhoon Imbudo, with wind gusts exceeding 210 kph, hit Palanan in July 2003. In this study, we ask: ( 1) was there an effect of the typhoon on stand structure and biomass; ( 2) was there an impact on species diversity; ( 3) did annual mortality, growth and recruitment change significantly between typhoon and non- typhoon periods; and ( 4) did the typhoon's impact vary with local topography, from leeward to windward sides of a ridge? Location: Lowland mixed dipterocarp forest, Palanan, Isabela, Philippines. Methods: Census data from 1998, 2004 and 2010 for all trees >= 1 cm DBH in a 16- ha permanent plot in Palanan, Isabela, were used to assess tree demography. Recorded in the census were species identification and measurements of DBH and tree locations. Biomass was calculated frompublished allometry. Results: Species diversity and stand structure remained stable, except for an increase in small- sized trees ( 1- 2 cm) recorded in the census conducted within a year of the typhoon disturbance. Treemortality was significantly higher during the typhoon interval at 2.27% yr-1 and more so in windward than leeward habitats. Above- ground biomass loss in the typhoon interval was minimal ( 2.64%) and biomass exceeded pre- typhoon levels after 6 yrs. Recruitment rate during the typhoon interval was almost four times the rate in the non- typhoon interval that followed, attributed to the rapid growth of seeds and seedlings of pioneer species due to the open, defoliated canopy. Negative population growth was recorded for the early successional species in the non- typhoon interval. Significantly higher growth rates of trees in the non- typhoon interval also contributed to biomass gain. Conclusions: Mortality, recruitment and growth rates vary across a heterogeneous landscape and are related to typhoon disturbances. The relatively low mortality and fast recovery of the Palanan forest demonstrates the resistance and resilience of the forest to intense episodic typhoon disturbances. C1 [Yap, Sandra L.] Univ Philippines, Inst Biol, PH-1101 Quezon City, Philippines. [Davies, Stuart J.] Smithsonian Trop Res Inst, Ctr Trop Forest Sci, Forest Global Earth Observ, Washington, DC 20013 USA. [Condit, Richard] Smithsonian Trop Res Inst, Balboa, Ancon, Panama. RP Davies, SJ (reprint author), Smithsonian Trop Res Inst, Ctr Trop Forest Sci, Forest Global Earth Observ, POB 37012, Washington, DC 20013 USA. EM slimyap@gmail.com; DaviesS@si.edu; conditr@gmail.com FU University of the Philippines; Conservation International-Philippines; Isabela State University; Center for Tropical Forest Science (CTFS) of the Smithsonian Tropical Research Institute; NSF [DEB-1046113] FX We thank the Department of Environment and Natural Resources (Reg. 2) for permission to conduct long-term studies in the Northern Sierra Madre Natural Park. The Palanan FDP has been supported by the University of the Philippines, Conservation International-Philippines, Isabela State University and the Center for Tropical Forest Science (CTFS) of the Smithsonian Tropical Research Institute. We also acknowledge the helpful feedback from participants of the CTFS-ForestGEO workshops (supported by NSF grant DEB-1046113 to S.J. Davies), especially G. Chuyong, D. Kenfack, Y. Lin, S. Lum, S. McMahon, N. Pongpattananurak and S. Pulla, during the preliminary analysis of data. S. Russo provided insightful comments that improved the manuscript. SLY especially thanks the field workers in Palanan and the invaluable support and dedication given by the late Leonardo L. Co and Daniel A. Lagunzad, former principal investigators of the Palanan FDP, and Perry S. Ong, current plot principal investigator. SLY participated in the collection and management of census data, conducted statistical analyses and drafted the manuscript. SJD helped conceive the study, reviewed data interpretation and significantly contributed to the manuscript. RC oversaw data analysis and made important revisions to the manuscript. All authors read and approved the final manuscript. The authors declare that they have no conflict of interest. NR 44 TC 0 Z9 0 U1 2 U2 12 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1100-9233 EI 1654-1103 J9 J VEG SCI JI J. Veg. Sci. PD JAN PY 2016 VL 27 IS 1 BP 133 EP 143 DI 10.1111/jvs.12358 PG 11 WC Plant Sciences; Ecology; Forestry SC Plant Sciences; Environmental Sciences & Ecology; Forestry GA DA5BF UT WOS:000367816400016 ER PT J AU Hong, T AF Hong, Terry TI Shelter SO LIBRARY JOURNAL LA English DT Book Review C1 [Hong, Terry] Smithsonian BookDragon, Washington, DC USA. RP Hong, T (reprint author), Smithsonian BookDragon, Washington, DC USA. NR 1 TC 0 Z9 0 U1 0 U2 0 PU REED BUSINESS INFORMATION PI NEW YORK PA 360 PARK AVENUE SOUTH, NEW YORK, NY 10010 USA SN 0363-0277 J9 LIBR J JI Libr. J. PD JAN PY 2016 VL 141 IS 1 BP 101 EP 101 PG 1 WC Information Science & Library Science SC Information Science & Library Science GA DA5SN UT WOS:000367862900147 ER PT J AU Lunning, NG Welten, KC McSween, HY Caffee, MW Beck, AW AF Lunning, Nicole G. Welten, Kees C. McSween, Harry Y., Jr. Caffee, Marc W. Beck, Andrew W. TI Grosvenor Mountains 95 howardite pairing group: Insights into the surface regolith of asteroid 4 Vesta SO METEORITICS & PLANETARY SCIENCE LA English DT Article ID CARBONACEOUS CHONDRITE CLASTS; DIOGENITE PARENT BODY; DARK MATERIAL; NOBLE-GASES; SUBSURFACE STRUCTURE; COLLISIONAL HISTORY; FRONTIER MOUNTAIN; POLYMICT BRECCIAS; EXPOSURE HISTORY; NORTHWEST AFRICA AB Regolithic howardites are analogs for the surface materials of asteroid 4 Vesta, recently mapped by the Dawn spacecraft. Rigorously evaluating pairing of howardites recovered in 1995 in the Grosvenor Mountains (GRO 95), Antarctica, enables an examination of a larger, more representative regolith sample. Previous work on two of the howardites studied here concluded that GRO 95602 and GRO 95535 are solar wind-rich surface regolith samples and that they are not paired with each other, leading to uncertainty regarding pairing relationships between the other GRO 95 howardites. Based on petrology, cosmic-ray exposure history, and terrestrial age, four GRO 95 howardites are paired. The paired howardites (GRO 95534, 95535, 95574, 95581) were from a meteoroid with radius of 10-15 cm, a preatmospheric size comparable to that of Kapoeta, the largest known regolithic howardite. The paired GRO 95 howardites contain clasts of at least 18 separate HED lithologies, providing evidence they were assembled from diverse source materials. The total eucrite: diogenite mixing ratio (ratio of all eucrite lithologies to all diogenite lithologies) in the paired GRO 95 howardites is similar to 2:1. Petrographically determined basaltic eucrite: cumulate eucrite ratios in regolithic howardites, studied here and previously, vary more widely than total eucrite: diogenite ratios. Relative to eucritic pyroxene, plagioclase is depleted in these howardites, which provides evidence that plagioclase is preferentially comminuted in the vestan regolith. The extent of plagioclase depletion could be an indicator of regolith maturity. C1 [Lunning, Nicole G.] Natl Museum Nat Hist, Smithsonian Inst, Dept Mineral Sci, Washington, DC 20560 USA. [Lunning, Nicole G.; McSween, Harry Y., Jr.] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN 37996 USA. [Lunning, Nicole G.; McSween, Harry Y., Jr.] Univ Tennessee, Planetary Geosci Inst, Knoxville, TN 37996 USA. [Welten, Kees C.] Univ Calif Berkeley, Space Sci Lab, Berkeley, CA 94720 USA. [Caffee, Marc W.] Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA. [Beck, Andrew W.] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA. RP Lunning, NG (reprint author), Natl Museum Nat Hist, Smithsonian Inst, Dept Mineral Sci, POB 37012,MRC 119, Washington, DC 20560 USA. EM lunningn@si.edu RI Beck, Andrew/J-7215-2015; OI Beck, Andrew/0000-0003-4455-2299; Lunning, Nicole/0000-0002-9845-5104 FU NASA through UCLA Dawn subcontract [2090-S-JB694]; NASA through Cosmochemistry grant [NNX13AN86G] FX We thank the Meteorite Working Group for allocation of samples, Ralph Harvey and John Schutt for guidance regarding meteorite find locations, and Allan Patchen for assistance with EMP analyses. We thank our reviewers, Dr. Paul Buchanan and Dr. Julia Cartwright, for constructive comments. We also thank Dr. Tim McCoy and Dr. Josh Emery for helpful discussions regarding this project. This research was supported in part by NASA through UCLA Dawn subcontract 2090-S-JB694 and Cosmochemistry grant NNX13AN86G to HYM. NR 108 TC 3 Z9 3 U1 3 U2 7 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 1086-9379 EI 1945-5100 J9 METEORIT PLANET SCI JI Meteorit. Planet. Sci. PD JAN PY 2016 VL 51 IS 1 BP 167 EP 194 DI 10.1111/maps.12580 PG 28 WC Geochemistry & Geophysics SC Geochemistry & Geophysics GA DA7XO UT WOS:000368019100010 ER PT J AU Bray, AD Pillepich, A Sales, LV Zhu, E Genel, S Rodriguez-Gomez, V Torrey, P Nelson, D Vogelsberger, M Springel, V Eisenstein, DJ Hernquist, L AF Bray, Aaron D. Pillepich, Annalisa Sales, Laura V. Zhu, Emily Genel, Shy Rodriguez-Gomez, Vicente Torrey, Paul Nelson, Dylan Vogelsberger, Mark Springel, Volker Eisenstein, Daniel J. Hernquist, Lars TI Modelling galactic conformity with the colour-halo age relation in the Illustris simulation SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE galaxies: formation; galaxies: haloes; cosmology: theory; dark matter ID DIGITAL SKY SURVEY; GALAXY ASSEMBLY BIAS; STAR-FORMATION; COSMOLOGICAL SIMULATIONS; FORMATION HISTORY; FORMATION PHYSICS; DARK-MATTER; COSMIC TIME; BLACK-HOLES; LUMINOSITY AB Comparisons between observational surveys and galaxy formation models find that dark matter haloes' mass can largely explain their galaxies' stellar mass. However, it remains uncertain whether additional environmental variables, known as assembly bias, are necessary to explain other galaxy properties. We use the Illustris simulation to investigate the role of assembly bias in producing galactic conformity by considering 18 000 galaxies with M-stellar > 2 x 10(9) M-circle dot. We find a significant signal of galactic conformity: out to distances of about 10 Mpc, the mean red fraction of galaxies around redder galaxies is higher than around bluer galaxies at fixed stellar mass. Dark matter haloes exhibit an analogous conformity signal, in which the fraction of haloes formed at earlier times (old haloes) is higher around old haloes than around younger ones at fixed halo mass. A plausible interpretation of galactic conformity is the combination of the halo conformity signal with the galaxy colour-halo age relation: at fixed stellar mass, particularly towards the low-mass end, Illustris' galaxy colours correlate with halo age, with the reddest galaxies (often satellites) preferentially found in the oldest haloes. We explain the galactic conformity effect with a simple semi-empirical model, assigning stellar mass via halo mass (abundance matching) and galaxy colour via halo age (age matching). Regarding comparison to observations, we conclude that the adopted selection/isolation criteria, projection effects, and stacking techniques can have a significant impact on the measured amplitude of the conformity signal. C1 [Bray, Aaron D.; Pillepich, Annalisa; Rodriguez-Gomez, Vicente; Nelson, Dylan; Eisenstein, Daniel J.; Hernquist, Lars] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Sales, Laura V.] Univ Calif Riverside, Riverside, CA 92521 USA. [Zhu, Emily] Phillips Acad, Andover, MA 01810 USA. [Zhu, Emily] Harvard Univ, Cambridge, MA 02138 USA. [Genel, Shy] Columbia Univ, New York, NY 10027 USA. [Torrey, Paul; Vogelsberger, Mark] MIT, Cambridge, MA 02139 USA. [Torrey, Paul] CALTECH, TAPIR, Pasadena, CA 91125 USA. [Springel, Volker] Heidelberg Inst Theoret Studies, D-69118 Heidelberg, Germany. [Springel, Volker] Heidelberg Univ, Zentrum Astron, ARI, D-69120 Heidelberg, Germany. RP Bray, AD (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM abray@cfa.harvard.edu OI Torrey, Paul/0000-0002-5653-0786; Rodriguez-Gomez, Vicente/0000-0002-9495-0079 FU HST [HST-AR-13897]; NASA - STScI [HST-HF2-51341.001-A]; NASA [NAS5-26555, NNX12AC67G]; NASA ATP Grant [NNX14AH35G]; European Research Council [EXAGAL-308037]; NSF [AST-1312095]; PRACE project [RA0844]; GCS-project [pr85je] FX ADB, AP, and SG thank Andrew Hearin for helpful discussions and comments on the manuscript and thank Frank van den Bosch, Jeremy Tinker, Guinevere Kauffmann, Alexie Leauthaud, and Cameron McBride for useful discussions. ADB thanks the OSU CCAPP for hosting its 2014 HOD workshop. AP acknowledges support from the HST grant HST-AR-13897. SG acknowledges support provided by NASA through Hubble Fellowship grant HST-HF2-51341.001-A awarded by the STScI, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. PT acknowledges support from NASA ATP Grant NNX14AH35G. VS acknowledges support through the European Research Council under ERC-StG grant EXAGAL-308037. LH acknowledges support from NASA grant NNX12AC67G and NSF grant AST-1312095.; The Illustris-1 simulation was run on the CURIE supercomputer at CEA/France as part of PRACE project RA0844, and the Super-MUC computer at the Leibniz Computing Centre, Germany, as part of GCS-project pr85je. The further simulations were run on the Harvard Odyssey and CfA/ITC clusters, the Ranger and Stampede supercomputers at the Texas Advanced Computing Center through XSEDE, and the Kraken supercomputer at Oak Ridge National Laboratory through XSEDE. The analysis presented in this paper was conducted on the Harvard Odyssey and CfA/ITC clusters. NR 58 TC 3 Z9 3 U1 0 U2 1 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 185 EP 198 DI 10.1093/mnras/stv2316 PG 14 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900037 ER PT J AU Richardson, ND Moffat, AFJ Maltais-Tariant, R Pablo, H Gies, DR Saio, H St-Louis, N Schaefer, G Miroshnichenko, AS Farrington, C Aldoretta, EJ Artigau, E Boyajian, TS Gordon, K Jones, J Matson, R McAlister, HA O'Brien, D Raghavan, D Ramiaramanantsoa, T Ridgway, ST Scott, N Sturmann, J Sturmann, L ten Brummelaar, T Thomas, JD Turner, N Vargas, N Zharikov, S Matthews, J Cameron, C Guenther, D Kuschnig, R Rowe, J Rucinski, S Sasselov, D Weiss, W AF Richardson, Noel D. Moffat, Anthony F. J. Maltais-Tariant, Raphael Pablo, Herbert Gies, Douglas R. Saio, Hideyuki St-Louis, Nicole Schaefer, Gail Miroshnichenko, Anatoly S. Farrington, Chris Aldoretta, Emily J. Artigau, Etienne Boyajian, Tabetha S. Gordon, Kathryn Jones, Jeremy Matson, Rachel McAlister, Harold A. O'Brien, David Raghavan, Deepak Ramiaramanantsoa, Tahina Ridgway, Stephen T. Scott, Nic Sturmann, Judit Sturmann, Laszlo ten Brummelaar, Theo Thomas, Joshua D. Turner, Nils Vargas, Norm Zharikov, Sergey Matthews, Jaymie Cameron, Chris Guenther, David Kuschnig, Rainer Rowe, Jason Rucinski, Slavek Sasselov, Dimitar Weiss, Werner TI Spectroscopy, MOST photometry, and interferometry of MWC 314: is it an LBV or an interacting binary? SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE binaries: close; stars: early-type; stars: individual: MWC 314; stars: massloss; stars: variables: S Doradus; stars: winds, outflows ID SECULAR ORBITAL EVOLUTION; CHARA ARRAY; MASSIVE STARS; P-CYGNI; SYSTEM; SUPERGIANTS; VARIABLES; SPECTROPHOTOMETRY; SPECTROMETER; VARIABILITY AB MWC 314 is a bright candidate luminous blue variable (LBV) that resides in a fairly close binary system, with an orbital period of 60.753 +/- 0.003 d. We observed MWC 314 with a combination of optical spectroscopy, broad-band ground-and space-based photometry, as well as with long baseline, near-infrared interferometry. We have revised the single-lined spectroscopic orbit and explored the photometric variability. The orbital light curve displays two minima each orbit that can be partially explained in terms of the tidal distortion of the primary that occurs around the time of periastron. The emission lines in the system are often double-peaked and stationary in their kinematics, indicative of a circumbinary disc. We find that the stellar wind or circumbinary disc is partially resolved in the K' -band with the longest baselines of the CHARA Array. From this analysis, we provide a simple, qualitative model in an attempt to explain the observations. From the assumption of Roche Lobe overflow and tidal synchronization at periastron, we estimate the component masses to be M-1 approximate to 5M(circle dot) and M-2 approximate to 15M(circle dot), which indicates a mass of the LBV that is extremely low. In addition to the orbital modulation, we discovered two pulsational modes with the MOST satellite. These modes are easily supported by a low-mass hydrogen-poor star, but cannot be easily supported by a star with the parameters of an LBV. The combination of these results provides evidence that the primary star was likely never a normal LBV, but rather is the product of binary interactions. As such, this system presents opportunities for studying mass-transfer and binary evolution with many observational techniques. C1 [Richardson, Noel D.; Moffat, Anthony F. J.; Maltais-Tariant, Raphael; Pablo, Herbert; St-Louis, Nicole; Aldoretta, Emily J.; Artigau, Etienne; Ramiaramanantsoa, Tahina] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada. [Richardson, Noel D.; Moffat, Anthony F. J.; Maltais-Tariant, Raphael; Pablo, Herbert; St-Louis, Nicole; Aldoretta, Emily J.; Artigau, Etienne; Ramiaramanantsoa, Tahina] Univ Montreal, CRAQ, Montreal, PQ H3C 3J7, Canada. [Gies, Douglas R.; Gordon, Kathryn; Jones, Jeremy; Matson, Rachel; McAlister, Harold A.; Raghavan, Deepak] Georgia State Univ, Dept Phys & Astron, Ctr High Angular Resolut Astron, Atlanta, GA 30302 USA. [Saio, Hideyuki] Tohoku Univ, Grad Sch Sci, Astron Inst, Sendai, Miyagi 9808578, Japan. [Schaefer, Gail; Farrington, Chris; Scott, Nic; Sturmann, Judit; Sturmann, Laszlo; ten Brummelaar, Theo; Turner, Nils; Vargas, Norm] Mt Wilson Observ, CHARA Array, Mt Wilson, CA 91023 USA. [Miroshnichenko, Anatoly S.] Univ N Carolina, Dept Phys & Astron, Greensboro, NC 27402 USA. [Boyajian, Tabetha S.] Yale Univ, New Haven, CT 06520 USA. [O'Brien, David] Max Planck Inst Radio Astron, D-53010 Bonn, Germany. [Ridgway, Stephen T.] Natl Opt Astron Observ, Tucson, AZ 85719 USA. [Thomas, Joshua D.] Clarkson Univ, Dept Phys, Potsdam, NY 13699 USA. [Zharikov, Sergey] Univ Nacl Autonoma Mexico, Inst Astron, Ensenada 22860, BC, Mexico. [Matthews, Jaymie; Kuschnig, Rainer] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada. [Cameron, Chris] Cape Breton Univ, Dept Math Phys & Geol, Sydney, NS B1P 6L2, Australia. [Guenther, David] St Marys Univ, Inst Computat Astrophys, Dept Phys & Astron, Halifax, NS B3H 3C3, Canada. [Kuschnig, Rainer] Univ Vienna, Inst Astron, A-1180 Vienna, Austria. [Rowe, Jason] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA. [Rucinski, Slavek] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada. [Sasselov, Dimitar] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. RP Richardson, ND (reprint author), Univ Montreal, Dept Phys, CP 6128,Succ Ctr Ville, Montreal, PQ H3C 3J7, Canada. EM richardson@astro.umontreal.ca OI Richardson, Noel/0000-0002-2806-9339 FU CRAQ (Centre de Recherche en Astrophysique du Quebec); NSERC (Canada); FRQNT (Quebec); NSF [AST-1411654]; DGAPA/PAPIIT project [IN100614]; NASA [ADAP12-0172]; NOAO Programs [2009B-0153, 2012A-0216]; Robert Martin Ayers Sciences Fund; GSU College of Arts and Sciences; National Science Foundation [AST-0606958, AST-0908253, AST-1211129]; W. M. Keck Foundation; NASA Exoplanet Science Institute; Georgia State University; David and Lucile Packard Foundation FX We thank the anonymous referee for helping the analysis and presentation of this paper. We are grateful to Fred Walter (Stony Brook University) for his scheduling of spectroscopic observations with the CTIO 1.5 m, to the CTIO SMARTS staff for queue observing support, and to Todd Henry (Georgia State University) for assistance in scheduling the initial observations with the SMARTS echelle spectrograph. We are also grateful to John Monnier (Univ. of Michigan) for contributions to data reduction and analysis. We thank Pierre-Luc Levesque, Bernard Malenfant, Ghislain Turcotte, and Philippe Vallee for their assistance in obtaining data at the OMM. Some spectra with the CTIO 1.5 m were obtained through the NOAO Programs 2009B-0153 and 2012A-0216. This work was partially based on observations obtained at the 2.1-m Otto Struve and 2.7-m Harlan. J. Smith telescopes of the McDonald Observatory of the University of Texas at Austin. This work was also based partially on observations obtained at the Mercator telescopes and HERMES spectrograph of the Instituto de Astrofisica de Canarias. This research was made possible through the use of the APASS, funded by the Robert Martin Ayers Sciences Fund. Operational funding for the CHARA Array is provided by the GSU College of Arts and Sciences, by the National Science Foundation through grants AST-0606958, AST-0908253, and AST-1211129, by the W. M. Keck Foundation, and by the NASA Exoplanet Science Institute. We thank the Mount Wilson Institute for providing infrastructure support at Mount Wilson Observatory. The CHARA Array, operated by Georgia State University, was built with funding provided by the National Science Foundation, Georgia State University, the W. M. Keck Foundation, and the David and Lucile Packard Foundation. This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France.; NDR is grateful for his CRAQ (Centre de Recherche en Astrophysique du Quebec) postdoctoral fellowship. AFJM and NSL are grateful for financial support from NSERC (Canada) and FRQNT (Quebec). DRG and GS acknowledge support from NSF grant AST-1411654. AM and SZ acknowledge support from DGAPA/PAPIIT project IN100614. TSB acknowledges support provided through NASA grant ADAP12-0172. NR 68 TC 3 Z9 3 U1 2 U2 2 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 244 EP 257 DI 10.1093/mnras/stv2291 PG 14 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900042 ER PT J AU Chiu, I Mohr, J McDonald, M Bocquet, S Ashby, MLN Bayliss, M Benson, BA Bleem, LE Brodwin, M Desai, S Dietrich, JP Forman, WR Gangkofner, C Gonzalez, AH Hennig, C Liu, J Reichardt, CL Saro, A Stalder, B Stanford, SA Song, J Schrabback, T Suhada, R Strazzullo, V Zenteno, A AF Chiu, I. Mohr, J. McDonald, M. Bocquet, S. Ashby, M. L. N. Bayliss, M. Benson, B. A. Bleem, L. E. Brodwin, M. Desai, S. Dietrich, J. P. Forman, W. R. Gangkofner, C. Gonzalez, A. H. Hennig, C. Liu, J. Reichardt, C. L. Saro, A. Stalder, B. Stanford, S. A. Song, J. Schrabback, T. Suhada, R. Strazzullo, V. Zenteno, A. TI Baryon content of massive galaxy clusters at 0.57 < z < 1.33 SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE Galaxy: evolution; galaxies: clusters: general; large-scale structure of Universe; X-rays: galaxies: clusters ID SOUTH-POLE TELESCOPE; ATACAMA COSMOLOGY TELESCOPE; SPT-SZ SURVEY; ZELDOVICH EFFECT SURVEY; DIGITAL SKY SURVEY; 720 SQUARE DEGREES; ACT-CL J0102-4915; K-BAND PROPERTIES; SIMILAR-TO 1; LUMINOSITY FUNCTION AB We study the stellar, brightest cluster galaxy (BCG) and intracluster medium (ICM) masses of 14 South Pole Telescope (SPT) selected galaxy clusters with median redshift z = 0.9 and mass M-500 = 6 x 10(14) M-circle dot. We estimate stellar masses for each cluster and BCG using six photometric bands, the ICM mass using X-ray observations and the virial masses using the SPT Sunyaev-Zel'dovich effect signature. At z = 0.9, the BCG mass M-*(BCG) constitutes 0.12 +/- 0.01 per cent of the halo mass for a 6 x 10(14) M-circle dot cluster, and this fraction falls as M-500(-0.58 +/- 0.07). The cluster stellar mass function has a characteristic mass M-0 = 10(11.0 +/- 0.1) M-circle dot, and the number of galaxies per unit mass in clusters is larger than in the field by a factor of 1.65 +/- 0.20. We combine our SPT sample with previously published samples at low redshift and correct to a common initial mass function and for systematic virial mass differences. We then explore mass and redshift trends in the stellar fraction f(*), the ICM fraction f(ICM), the collapsed baryon fraction f(c) and the baryon fraction f(b). At a pivot mass of 6 x 10(14) M-circle dot and redshift z = 0.9, the characteristic values are f(*) = 1.1 +/- 0.1 per cent, f(ICM) = 9.6 +/- 0.5 per cent, f(c) = 10.7 +/- 1.1 per cent and f(b) = 10.7 +/- 0.6 per cent. These fractions all vary with cluster mass at high significance, with higher mass clusters having lower f(*) and f(c) and higher f(ICM) and f(b). When accounting for a 15 per cent systematic virial mass uncertainty, there is no statistically significant redshift trend at fixed mass. Our results support the scenario where clusters grow through accretion from subclusters (higher f(*), lower f(ICM)) and the field (lower f(*), higher f(ICM)), balancing to keep f(*) and f(ICM) approximately constant since z similar to 0.9. C1 [Chiu, I.; Mohr, J.; Bocquet, S.; Desai, S.; Dietrich, J. P.; Gangkofner, C.; Hennig, C.; Liu, J.; Saro, A.; Suhada, R.; Strazzullo, V.; Zenteno, A.] Univ Munich, Dept Phys, D-81679 Munich, Germany. [Chiu, I.; Mohr, J.; Bocquet, S.; Desai, S.; Dietrich, J. P.; Gangkofner, C.; Hennig, C.; Liu, J.; Saro, A.] Excellence Cluster Universe, D-85748 Garching, Germany. [Mohr, J.] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany. [McDonald, M.] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA. [Ashby, M. L. N.; Bayliss, M.; Forman, W. R.; Stalder, B.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Bayliss, M.] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Benson, B. A.] Fermilab Natl Accelerator Lab, Batavia, IL 60510 USA. [Benson, B. A.] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA. [Benson, B. A.] Univ Chicago, Dept Astron & Astrophys, Chicago, IL 60637 USA. [Bleem, L. E.] Univ Chicago, Dept Phys, Chicago, IL 60637 USA. [Bleem, L. E.] Argonne Natl Lab, Argonne, IL 60439 USA. [Brodwin, M.] Univ Missouri, Dept Phys & Astron, Kansas City, MO 64110 USA. [Gonzalez, A. H.] Univ Florida, Dept Astron, Gainesville, FL 32611 USA. [Reichardt, C. L.] Univ Melbourne, Sch Phys, Melbourne, Vic 3010, Australia. [Stalder, B.] Univ Hawaii, Inst Astron, Honolulu, HI 96822 USA. [Stanford, S. A.] Univ Calif Davis, Dept Phys, Davis, CA 95616 USA. [Stanford, S. A.] Lawrence Livermore Natl Lab, Inst Geophys & Planetary Phys, Livermore, CA 94550 USA. [Song, J.] Korea Astron & Space Sci Inst, Daejeon 305348, South Korea. [Schrabback, T.] Argelander Inst Astron, D-53121 Bonn, Germany. [Zenteno, A.] Cerro Tololo Interamer Observ, La Serena, Chile. RP Chiu, I (reprint author), Univ Munich, Dept Phys, Scheinerstr 1, D-81679 Munich, Germany. EM inonchiu@usm.lmu.de OI Dietrich, Jorg/0000-0002-8134-9591; Reichardt, Christian/0000-0003-2226-9169; Stern, Corvin/0000-0003-4406-6127; Forman, William/0000-0002-9478-1682 FU VLT programmes [088.A-0889, 089.A-0824]; DFG Cluster of Excellence 'Origin and Structure of the Universe'; Transregio programme TR33 'The Dark Universe'; Fermi Research Alliance, LLC [De-AC02-07CH11359]; United States Department of Energy; NSF [AST-1009012, AST-1009649, MRI-0723073]; German Federal Ministry of Economics and Technology (BMWi) [50 OR 1210]; National Science Foundation [ANT-0638937]; NSF Physics Frontier Center [PHY-0114422]; Kavli Foundation; Gordon and Betty Moore Foundation; [C18-12246]; [C19-12447]; [60099]; [70053]; [80012] FX We acknowledge the support by the DFG Cluster of Excellence 'Origin and Structure of the Universe' and the Transregio programme TR33 'The Dark Universe'. The calculations have been carried out on the computing facilities of the Computational Center for Particle and Astrophysics (C2PAP) and of the Leibniz Supercomputer Center (LRZ). BB is supported by the Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the United States Department of Energy. BS acknowledges the support of the NSF grants at Harvard and SAO (AST-1009012, AST-1009649 and MRI-0723073). TS acknowledges the support from the German Federal Ministry of Economics and Technology (BMWi) provided through DLR under project 50 OR 1210. The South Pole Telescope is supported by the National Science Foundation through grant ANT-0638937. Partial support is also provided by the NSF Physics Frontier Center grant PHY-0114422 to the Kavli Institute of Cosmological Physics at the University of Chicago, the Kavli Foundation and the Gordon and Betty Moore Foundation.; Optical imaging data from the VLT programmes 088.A-0889 and 089.A-0824, HST imaging data from programmes C18-12246 and C19-12447, and Spitzer Space Telescope imaging from programmes 60099, 70053 and 80012 enable the SED fitting in this analysis. X-ray data obtained with Chandra X-ray Observatory programmes and XMM-Newton Observatory programme 067501 enable the ICM mass measurements. The SPT survey programme SPT-SZ enabled the discovery of these high-redshift clusters and subsequent analyses have enabled virial mass estimates of these systems. Optical spectroscopic data from VLT programmes 086.A-0741 and 286.A-5021 and Gemini programme GS-2009B-Q-16, GS-2011A-C-3 and GS-2011B-C-6 were included in this work. Additional spectroscopic data were obtained with the 6.5 m Magellan Telescopes. NR 100 TC 7 Z9 7 U1 0 U2 1 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 258 EP 275 DI 10.1093/mnras/stv2303 PG 18 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900043 ER PT J AU de Witt, A Bietenholz, MF Kamble, A Soderberg, AM Brunthaler, A Zauderer, B Bartel, N Rupen, MP AF de Witt, A. Bietenholz, M. F. Kamble, A. Soderberg, A. M. Brunthaler, A. Zauderer, B. Bartel, N. Rupen, M. P. TI Imaging the expanding shell of SN 2011dh SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE supernovae: individual: SN2011dh; radio continuum: general ID IIB SUPERNOVA 2011DH; VLBI OBSERVATIONS; X-RAY; SUPERGIANT PROGENITOR; BINARY COMPANION; RADIO-EMISSION; LIGHT CURVES; 1993J VLBI; M51; EVOLUTION AB We report on the third epoch of very long baseline interferometry (VLBI) observations of the radio-bright supernova SN 2011dh, located in the nearby (7.8 Mpc) galaxy M51. The observations took place at t = 453 d after the explosion and at a frequency of 8.4 GHz. We obtained a fairly well-resolved image of the shell of SN 2011dh, making it one of only six recent supernovae for which resolved images of the ejecta are available. SN 2011dh has a relatively clear shell morphology, being almost circular in outline, although there may be some asymmetry in brightness around the ridge. By fitting a spherical shell model directly to the visibility measurements we determine the angular radius of SN 2011dh's radio emission to be 636 +/- 29 mu as. At a distance of 7.8 Mpc, this angular radius corresponds to a linear radius of (7.4 +/- 0.3) x 10(16) cm and an average expansion velocity since the explosion of 19 000(-2400)(+2800) km s(-1). We combine our VLBI measurements of SN 2011dh's radius with values determined from the radio spectral energy distribution under the assumption of a synchrotron-self-absorbed spectrum, and find all the radii are consistent with a power-law evolution, with R similar to t(0.97 +/- 0.01), implying almost free expansion over the period t = 4 d to 453 d. C1 [de Witt, A.; Bietenholz, M. F.] Hartebeesthoek Radio Observ, ZA-1740 Krugersdorp, South Africa. [Bietenholz, M. F.; Bartel, N.] York Univ, Dept Phys & Astron, Toronto, ON M3J 1P3, Canada. [Kamble, A.; Soderberg, A. M.; Zauderer, B.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Brunthaler, A.] Max Planck Inst Radioastron, D-53121 Bonn, Germany. [Rupen, M. P.] Natl Res Council Canada, Herzberg Astron & Astrophys Programs, Domin Radio Astrophys Observ, Penticton, BC V2A 6J9, Canada. RP de Witt, A (reprint author), Hartebeesthoek Radio Observ, POB 443, ZA-1740 Krugersdorp, South Africa. EM alet@hartrao.ac.za; michael@hartrao.ac.za FU National Research Foundation (NRF) of South Africa; NSERC FX Research at Hartebeesthoek Radio Astronomy Observatory was partly supported by National Research Foundation (NRF) of South Africa. Research at York University was partly supported by NSERC. We have made use of NASA's Astrophysics Data System Bibliographic Service. NR 54 TC 3 Z9 3 U1 1 U2 1 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 511 EP 517 DI 10.1093/mnras/stv2306 PG 7 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900064 ER PT J AU Lipunov, VM Gorosabel, J Pruzhinskaya, MV Postigo, AD Pelassa, V Tsvetkova, AE Sokolov, IV Kann, DA Xu, D Gorbovskoy, ES Krushinski, VV Kornilov, VG Balanutsa, PV Boronina, SV Budnev, NM Cano, Z Castro-Tirado, AJ Chazov, VV Connaughton, V Delvaux, C Frederiks, DD Fynbo, JFU Gabovich, AV Goldstein, A Greiner, J Gress, OA Ivanov, KI Jakobsson, P Klose, S Knust, F Komarova, VN Konstantinov, E Krylov, AV Kuvshinov, DA Kuznetsov, AS Lipunova, GV Moskvitin, AS Pal'shin, VD Pandey, SB Poleshchuk, VA Schmidl, S Sergienko, YP Sinyakov, EV Schulze, S Sokolov, VV Sokolova, TN Sparre, M Thone, CC Tlatov, AG Tyurina, NV Ulanov, MV Yazev, SA Yurkov, VV AF Lipunov, V. M. Gorosabel, J. Pruzhinskaya, M. V. de Ugarte Postigo, A. Pelassa, V. Tsvetkova, A. E. Sokolov, I. V. Kann, D. A. Xu, Dong Gorbovskoy, E. S. Krushinski, V. V. Kornilov, V. G. Balanutsa, P. V. Boronina, S. V. Budnev, N. M. Cano, Z. Castro-Tirado, A. J. Chazov, V. V. Connaughton, V. Delvaux, C. Frederiks, D. D. Fynbo, J. F. U. Gabovich, A. V. Goldstein, A. Greiner, J. Gress, O. A. Ivanov, K. I. Jakobsson, P. Klose, S. Knust, F. Komarova, V. N. Konstantinov, E. Krylov, A. V. Kuvshinov, D. A. Kuznetsov, A. S. Lipunova, G. V. Moskvitin, A. S. Pal'shin, V. D. Pandey, S. B. Poleshchuk, V. A. Schmidl, S. Sergienko, Yu. P. Sinyakov, E. V. Schulze, S. Sokolov, V. V. Sokolova, T. N. Sparre, M. Thoene, C. C. Tlatov, A. G. Tyurina, N. V. Ulanov, M. V. Yazev, S. A. Yurkov, V. V. TI The optical identification of events with poorly defined locations: the case of the Fermi GBM GRB 140801A SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE acceleration of particles; black hole physics; magnetic field; gamma-ray: general; X-ray: general ID GAMMA-RAY BURSTS; COMPLETE SAMPLE; LIGHT CURVES; AFTERGLOWS; SPECTRA; MASTER; TELESCOPE; LUMINOSITY; CATALOG; NETWORK AB We report the early discovery of the optical afterglow of gamma-ray burst (GRB) 140801A in the 137 deg(2) 3-sigma error-box of the Fermi Gamma-ray Burst Monitor (GBM). MASTER is the only observatory that automatically reacts to all Fermi alerts. GRB 140801A is one of the few GRBs whose optical counterpart was discovered solely from its GBM localization. The optical afterglow of GRB 140801A was found by MASTER Global Robotic Net 53 s after receiving the alert, making it the fastest optical detection of a GRB from a GBM error-box. Spectroscopy obtained with the 10.4-m Gran Telescopio Canarias and the 6-m Big Telescope Alt-azimuth of the Special Astrophysical Observatory of the Russian Academy of Sciences reveals a redshift of z = 1.32. We performed optical and near-infrared photometry of GRB 140801A using different telescopes with apertures ranging from 0.4 to 10.4 m. GRB 140801A is a typical burst in many ways. The rest-frame bolometric isotropic energy release and peak energy of the burst are E-iso = 5.54(-0.24)(+0.26) x 10(52) erg and E-p,E- rest similar or equal to 280 keV, respectively, which is consistent with the Amati relation. The absence of a jet break in the optical light curve provides a lower limit on the half-opening angle of the jet theta = 6 degrees.1. The observed E-peak is consistent with the limit derived from the Ghirlanda relation. The joint Fermi GBM and Konus-Wind analysis show that GRB 140801A could belong to the class of intermediate duration. The rapid detection of the optical counterpart of GRB 140801A is especially important regarding the upcoming experiments with large coordinate error-box areas. C1 [Lipunov, V. M.; Kornilov, V. G.; Kuvshinov, D. A.] Moscow MV Lomonosov State Univ, Fac Phys, Moscow 119991, Russia. [Lipunov, V. M.; Pruzhinskaya, M. V.; Gorbovskoy, E. S.; Kornilov, V. G.; Balanutsa, P. V.; Chazov, V. V.; Krylov, A. V.; Kuvshinov, D. A.; Kuznetsov, A. S.; Lipunova, G. V.; Tyurina, N. V.] Moscow MV Lomonosov State Univ, Sternberg Astron Inst, Moscow 119234, Russia. [Lipunov, V. M.; Gorbovskoy, E. S.] Moscow MV Lomonosov State Univ, Extreme Universe Lab, Inst Nucl Phys, Moscow 119991, Russia. [Gorosabel, J.; de Ugarte Postigo, A.; Castro-Tirado, A. J.; Thoene, C. C.] Inst Astrofis Andalucia, E-18008 Granada, Spain. [Gorosabel, J.] Ikerbasque, Basque Fdn Sci, E-48008 Bilbao, Spain. [Gorosabel, J.] Univ Basque Country, Grp Ciencias Planetarias, ETS Ingn, Dept Fis Aplicada 1,UPV EHU IAA CSIC,Unidad Asoci, E-48013 Bilbao, Spain. [de Ugarte Postigo, A.; Xu, Dong; Fynbo, J. F. U.; Sparre, M.] Univ Copenhagen, Niels Bohr Inst, Dark Cosmol Ctr, DK-2100 Copenhagen O, Denmark. [Pelassa, V.; Connaughton, V.] Univ Alabama, CSPAR, Huntsville, AL 35899 USA. [Pelassa, V.; Pal'shin, V. D.] Harvard Smithsonian Ctr Astrophys, Fred Lawrence Whipple Observ, Amado, AZ 85645 USA. [Tsvetkova, A. E.; Frederiks, D. D.; Ulanov, M. V.] Ioffe Inst, St Petersburg 194021, Russia. [Sokolov, I. V.] Russian AS, Terskol Branch, Inst Astron, Tyrnyauz 361623, Russia. [Kann, D. A.; Klose, S.; Schmidl, S.] Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany. [Xu, Dong] Chinese Acad Sci, Natl Astron Observ, Beijing 100012, Peoples R China. [Xu, Dong] Chinese Acad Sci, Natl Astron Observ, Key Lab Space Astron & Technol, Beijing 100012, Peoples R China. [Krushinski, V. V.] Ural Fed Univ, Kourovka Astron Observ, Ekaterinburg 620000, Russia. [Boronina, S. V.] St Petersburg State Univ, St Petersburg 199034, Russia. [Budnev, N. M.; Gress, O. A.; Ivanov, K. I.; Konstantinov, E.; Poleshchuk, V. A.; Yazev, S. A.] Irkutsk State Univ, Inst Appl Phys, Irkutsk 664003, Russia. [Cano, Z.; Jakobsson, P.] Univ Iceland, Ctr Astrophys & Cosmol, Inst Sci, IS-107 Reykjavik, Iceland. [Castro-Tirado, A. J.] Univ Malaga, Unidad Asociada, Dept Ingn Sistemas & Automiat, E-29071 Malaga, Spain. [Connaughton, V.] Univ Space Res Assoc, Huntsville, AL 35805 USA. [Delvaux, C.; Greiner, J.; Knust, F.] Max Planck Inst Extraterr Phys, D-85748 Garching, Germany. [Gabovich, A. V.; Sergienko, Yu. P.; Sinyakov, E. V.; Yurkov, V. V.] Blagoveschensk State Pedag Univ, Blagoveshchensk 675000, Amur Region, Russia. [Goldstein, A.] NASA, Space Sci Off, Marshall Space Flight Ctr, Huntsville, AL 35812 USA. [Greiner, J.] Tech Univ Munich, Excellence Cluster Universe, D-85748 Garching, Germany. [Komarova, V. N.; Sokolov, V. V.; Sokolova, T. N.] Russian AS, Special Astrophys Observ, Nizhnii Arkhyz 369167, Russia. [Pandey, S. B.] Aryabhatta Res Inst Observat Sci, Manora Peak 263002, Nainital, India. [Schulze, S.] Pontificia Univ Catolica Chile, Fac Fis, Inst Astrofis, Santiago 7820436, Chile. [Schulze, S.] Millennium Inst Astrophys, Santiago 7820436, Chile. [Tlatov, A. G.] RAS, Main Pulkovo Observ, Kislovodsk Solar Stn, Kislovodsk 357700, Russia. [Ulanov, M. V.] Peter Great St Petersburg Polytech Univ, St Petersburg 195251, Russia. RP Lipunov, VM (reprint author), Moscow MV Lomonosov State Univ, Fac Phys, GSP 1, Moscow 119991, Russia. EM lipunov2007@gmail.com RI Ivanov, Kirill/O-9236-2015; Gorbovskoy, Evgeny/O-8845-2015; OI Gorbovskoy, Evgeny/0000-0002-4368-9237; de Ugarte Postigo, Antonio/0000-0001-7717-5085; Frederiks, Dmitry/0000-0002-1153-6340; Sparre, Martin/0000-0002-9735-3851; Thone, Christina/0000-0002-7978-7648; Schulze, Steve/0000-0001-6797-1889 FU Development Programme of Lomonosov Moscow State University; RFBR [15-02-07875, 14-32-50547]; Russian Federation Ministry of Education and Science [14.B25.31.0010, 2014/51, 1366]; NASA; Russian Foundation of Fundamental Research [RFBR 14-02-31546, 14-02-91172]; Russian Space Agency, RFBR [15-02-00532a, 13-02-12017 ofi-m]; DFG [HA 1850/28-1, Kl 766/16-1, 766/16-3]; Spanish Ministry Grant [AYA 2012-39727-C03-01]; EXTraS from European Union [607452]; Thuringer Ministerium fur Bildung, Wissenschaft und Kultur [FKZ 12010-514]; Division of Physics, Russian Academy of Sciences [OFN-17]; Russian Federation [MK-1699.2014.2]; CONICYT-Chile FONDECYT [3140534]; Basal-CATA [PFB-06/2007]; 'Millennium Institute of Astrophysics (MAS) of Iniciativa Cientifica Milenio del Ministerio de Economia, Fomento y Turismo' [IC120009]; [3.615.2014/K] FX MASTER Global Robotic Net is supported in part by the Development Programme of Lomonosov Moscow State University. This work was also supported in part by RFBR 15-02-07875 grant.; This work is also partially supported by the Russian Federation Ministry of Education and Science (agreement 14.B25.31.0010 and government assignment 2014/51, project 1366) and by state order No. 3.615.2014/K in relation to scientific activity (design part).; The Fermi GBM collaboration acknowledges support for GBM development, operations, and data analysis from NASA in the U.S.A and BMWi/DLR in Germany. AG is supported by an appointment to the NASA Postdoctoral Program at MSFC, administered by Oak Ridge Associated Universities through a contract with NASA.; This work was supported in part by Russian Foundation of Fundamental Research, grant RFBR 14-02-31546, 14-02-91172.; The KW experiment is partially supported by a Russian Space Agency contract, RFBR grants 15-02-00532a and 13-02-12017 ofi-m.; Part of the funding for GROND (both hardware and personnel) was generously granted from the Leibniz-Prize to Professor G. Hasinger (DFG grant HA 1850/28-1).; AJC acknowledges support from the Spanish Ministry Grant AYA 2012-39727-C03-01.; CD acknowledges support through EXTraS, funded from the European Union's Seventh Framework Programme for research, technological development and demonstration under grant agreement no 607452.; DAK, SK, and SS acknowledge support by DFG grants Kl 766/16-1 and 766/16-3. In addition, SS acknowledges support by the Thuringer Ministerium fur Bildung, Wissenschaft und Kultur under FKZ 12010-514.; We acknowledge A. Burenkov, V. Vlasyuk and T. Fatkhullin for the help in observations. AM, VK and TS are partially supported by the Research Program OFN-17 of the Division of Physics, Russian Academy of Sciences. AM is also partially supported by the grant MK-1699.2014.2 of the President of Russian Federation and by RFBR 14-32-50547.; SS acknowledges support from CONICYT-Chile FONDECYT 3140534, Basal-CATA PFB-06/2007, and Project IC120009 'Millennium Institute of Astrophysics (MAS) of Iniciativa Cientifica Milenio del Ministerio de Economia, Fomento y Turismo'. NR 57 TC 4 Z9 4 U1 4 U2 11 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 712 EP 724 DI 10.1093/mnras/stv2228 PG 13 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900082 ER PT J AU Pakmor, R Springel, V Bauer, A Mocz, P Munoz, DJ Ohlmann, ST Schaal, K Zhu, CC AF Pakmor, Ruediger Springel, Volker Bauer, Andreas Mocz, Philip Munoz, Diego J. Ohlmann, Sebastian T. Schaal, Kevin Zhu, Chenchong TI Improving the convergence properties of the moving-mesh code AREPO SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE hydrodynamics; methods: numerical; galaxy: formation ID SMOOTHED PARTICLE HYDRODYNAMICS; GEOMETRIC CONSERVATION LAW; WHITE-DWARF MERGERS; COSMOLOGICAL SIMULATIONS; FLOW COMPUTATIONS; STELLAR FEEDBACK; GALAXY FORMATION; IA SUPERNOVAE; DISC GALAXIES; EVOLUTION AB Accurate numerical solutions of the equations of hydrodynamics play an ever more important role in many fields of astrophysics. In this work, we reinvestigate the accuracy of the movingmesh code AREPO and show how its convergence order can be improved for general problems. In particular, we clarify that for certain problems AREPO only reaches first-order convergence for its original formulation. This can be rectified by simple modifications we propose to the time integration scheme and the spatial gradient estimates of the code, both improving the accuracy of the code. We demonstrate that the new implementation is indeed second-order accurate under the L-1 norm, and in particular substantially improves conservation of angular momentum. Interestingly, whereas these improvements can significantly change the results of smooth test problems, we also find that cosmological simulations of galaxy formation are unaffected, demonstrating that the numerical errors eliminated by the new formulation do not impact these simulations. In contrast, simulations of binary stars followed over a large number of orbital times are strongly affected, as here it is particularly crucial to avoid a long-term build up of errors in angular momentum conservation. C1 [Pakmor, Ruediger; Springel, Volker; Bauer, Andreas; Ohlmann, Sebastian T.; Schaal, Kevin] Heidelberger Inst Theoret Studien, D-69118 Heidelberg, Germany. [Springel, Volker; Schaal, Kevin] Heidelberg Univ, Zentrum Astron, Astronom Recheninst, D-69120 Heidelberg, Germany. [Mocz, Philip] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. [Munoz, Diego J.] Cornell Univ, Dept Astron, Ctr Space Res, Ithaca, NY 14853 USA. [Ohlmann, Sebastian T.] Univ Wurzburg, Inst Theoret Phys, D-97074 Wurzburg, Germany. [Zhu, Chenchong] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada. RP Pakmor, R (reprint author), Heidelberger Inst Theoret Studien, Schloss Wolfsbrunnenweg 35, D-69118 Heidelberg, Germany. EM ruediger.pakmor@h-its.org FU European Research Council [EXAGAL-308037]; Klaus Tschira Foundation; German Science Foundation [1648]; National Science Foundation [DGE-1144152]; Studienstiftung des deutschen Volkes; IMPRS for Astronomy & Cosmic Physics at the University of Heidelberg FX This work has been supported by the European Research Council under ERC-StG grant EXAGAL-308037 and by the Klaus Tschira Foundation. VS and KS acknowledge support through subproject EXAMAG of the Priority Programme 1648 'Software for Exascale Computing' of the German Science Foundation. Part of the simulations of this paper used the SuperMUC system at the Leibniz Computing Centre, Garching. PM acknowledges support by the National Science Foundation Graduate Research Fellowship under grant no. DGE-1144152. STO acknowledges financial support from Studienstiftung des deutschen Volkes. AB and KS acknowledge support by the IMPRS for Astronomy & Cosmic Physics at the University of Heidelberg. NR 47 TC 21 Z9 21 U1 1 U2 1 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP 1134 EP 1143 DI 10.1093/mnras/stv2380 PG 10 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900110 ER PT J AU Slepian, Z Eisenstein, DJ AF Slepian, Zachary Eisenstein, Daniel J. TI Accelerating the two-point and three-point galaxy correlation functions using Fourier transforms SO MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY LA English DT Article DE methods: data analysis; methods: statistical; large-scale structure of Universe ID REDSHIFT-SPACE DISTORTIONS; LUMINOUS RED GALAXIES; BARYON ACOUSTIC-OSCILLATIONS; POWER-SPECTRUM; SDSS-III; DATA RELEASES; FINAL DATA; H(Z); DEPENDENCE; D-A(Z) AB Though Fourier transforms (FTs) are a common technique for finding correlation functions, they are not typically used in computations of the anisotropy of the two-point correlation function (2PCF) about the line of sight in wide-angle surveys because the line-of-sight direction is not constant on the Cartesian grid. Here we show how FTs can be used to compute the multipole moments of the anisotropic 2PCF. We also show how FTs can be used to accelerate the 3PCF algorithm of Slepian & Eisenstein. In both cases, these FT methods allow one to avoid the computational cost of pair counting, which scales as the square of the number density of objects in the survey. With the upcoming large data sets of Dark Energy Spectroscopic Instrument, Euclid, and Large Synoptic Survey Telescope, FT techniques will therefore offer an important complement to simple pair or triplet counts. C1 [Slepian, Zachary; Eisenstein, Daniel J.] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA. RP Slepian, Z (reprint author), Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA. EM zslepian@cfa.harvard.edu; deisenstein@cfa.harvard.edu FU National Science Foundation [DGE-1144152]; Department of Energy [DE-SC0013718] FX The authors gratefully acknowledge useful discussions with Blakesley Burkhart, Charles-Antoine Collins Fekete, Doug Finkbeiner, Nikhil Padmanabhan, Stephen Portillo, and Martin White. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under grant no. DGE-1144152 and by the Department of Energy under grant DE-SC0013718. NR 46 TC 1 Z9 1 U1 0 U2 0 PU OXFORD UNIV PRESS PI OXFORD PA GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND SN 0035-8711 EI 1365-2966 J9 MON NOT R ASTRON SOC JI Mon. Not. Roy. Astron. Soc. PD JAN 1 PY 2016 VL 455 IS 1 BP L31 EP L35 DI 10.1093/mnrasl/slv133 PG 5 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA7TB UT WOS:000368005900007 ER PT J AU Thompson, FC Pape, T AF Thompson, F. Christian Pape, Thomas TI Sherborn's influence on Systema Dipterorum SO ZOOKEYS LA English DT Article DE Flies; nomenclator; taxonomic catalog; identification; biodiversity informatics infrastructure; quality assurance standard ID WORLD LIST; NAMES; TAXONOMY AB Flies make up more than 10% of the planetary biota and our well-being depends on how we manage our coexistence with flies. Storing and accessing relevant knowledge about flies is intimately connected with using correct names, and Systema Dipterorum provides a single authoritative classification for flies developed by consensus among contributors. The 160,000 species of flies currently known are distributed among 160 recent families and some 12,000 genera, which with their synonyms encompass a total of more than a quarter of a million names. These names and their associated classification are shared with relevant global solutions. Sherborn appears to have done remarkably well indexing Diptera names with an overall error rate estimated to be close to 1%. C1 [Thompson, F. Christian] Smithsonian Inst, Dept Entomol, Washington, DC 20560 USA. [Pape, Thomas] Nat Hist Museum Denmark, Dept Biosystemat, DK-2100 Copenhagen, Denmark. RP Pape, T (reprint author), Nat Hist Museum Denmark, Dept Biosystemat, Univ Pk 15, DK-2100 Copenhagen, Denmark. EM tpape@snm.ku.dk RI Pape, Thomas/E-7520-2011 OI Pape, Thomas/0000-0001-6609-0609 FU Schlinger Foundation; Global Biodiversity Information Facility; United States Department of Agriculture; our home institutions FX We express our thanks to the entire Systema Dipterorum team of contributors and to all others who have supplied information over the years, and to the Schlinger Foundation, the Global Biodiversity Information Facility, the United States Department of Agriculture, and our home institutions, all of which provided financial support at various times. Neal Evenhuis, Dan Bickel and Steve Gaimari skillfully commented on the manuscript. NR 82 TC 0 Z9 0 U1 0 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 550 SI SI BP 135 EP 152 DI 10.3897/zookeys.550.9447 PG 18 WC Zoology SC Zoology GA DA5YV UT WOS:000367879500008 PM 26877656 ER PT J AU Pilsk, SC Kalfatovic, MR Richard, JM AF Pilsk, Suzanne C. Kalfatovic, Martin R. Richard, Joel M. TI Unlocking Index Animalium: From paper slips to bytes and bits SO ZOOKEYS LA English DT Article DE Metadata; Digitization; Linked Open Data ID INFORMATICS AB In 1996 Smithsonian Libraries (SIL) embarked on the digitization of its collections. By 1999, a full-scale digitization center was in place and rare volumes from the natural history collections, often of high illustrative value, were the focus for the first years of the program. The resulting beautiful books made available for online display were successful to a certain extent, but it soon became clear that the data locked within the texts needed to be converted to more usable and re-purposable form via digitization methods that went beyond simple page imaging and included text conversion elements. Library staff met with researchers from the taxonomic community to understand their path to the literature and identified tools (indexes and bibliographies) used to connect to the library holdings. The traditional library metadata describing the titles, which made them easily retrievable from the shelves of libraries, was not meeting the needs of the researcher looking for more detailed and granular data within the texts. The result was to identify proper print tools that could potential assist researchers in digital form. This paper outlines the project undertaken to convert Charles Davies Sherborn's Index Animalium into a tool to connect researchers to the library holdings: from a print index to a database to eventually a dataset. Sherborn's microcitation of a species name and his bibliographies help bridge the gap between taxonomist and literature holdings of libraries. In 2004, SIL received funding from the Smithsonian's Atherton Seidell Endowment to create an online version of Sherborn's Index Animalium. The initial project was to digitize the page images and re-key the data into a simple data structure. As the project evolved, a more complex database was developed which enabled quality field searching to retrieve species names and to search the bibliography. Problems with inconsistent abbreviations and styling of his bibliographies made the parsing of the data difficult. Coinciding with the development of the Biodiversity Heritage Library (BHL) in 2005, it became obvious there was a need to integrate the database converted Index Animalium, BHL's scanned taxonomic literature, and taxonomic intelligence (the algorithmic identification of binomial, Latinate name-strings). The challenges of working with legacy taxonomic citation, computer matching algorithms, and making connections have brought us to today's goal of making Sherborn available and linked to other datasets. Partnering with others to allow machine-to-machine communications the data is being examined for possible transformation into RDF markup and meeting the standards of Linked Open Data. SIL staff have partnered with Thomson Reuters and the Global Names Initiative to further enhance the Index Animalium data set. Thomson Reuters' staff is now working on integrating the species microcitation and species name in the ION: Index to Organism Names project; Richard Pyle (The Bishop Museum) is also working on further parsing of the text. The Index Animalium collaborative project's ultimate goal is to successful have researchers go seamlessly from the species name in either ION or the scanned pages of Index Animalium to the digitized original description in BHL - connecting taxonomic researchers to original authored species descriptions with just a click. C1 [Pilsk, Suzanne C.; Kalfatovic, Martin R.; Richard, Joel M.] Smithsonian Lib, Washington, DC 20560 USA. RP Pilsk, SC (reprint author), Smithsonian Lib, Washington, DC 20560 USA. EM PilskS@si.edu NR 25 TC 1 Z9 1 U1 3 U2 80 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1313-2989 EI 1313-2970 J9 ZOOKEYS JI ZooKeys PY 2016 IS 550 SI SI BP 153 EP 171 DI 10.3897/zookeys.550.9673 PG 19 WC Zoology SC Zoology GA DA5YV UT WOS:000367879500009 PM 26877657 ER PT J AU Renner, E Price, EE Subiaul, F AF Renner, Elizabeth Price, Elizabeth E. Subiaul, Francys TI Sequential recall of meaningful and arbitrary sequences by orangutans and human children: Does content matter? SO ANIMAL COGNITION LA English DT Article DE Sequential learning; Great apes; Children; Development; Memory; Monotonicity ID MACAQUES MACACA-MULATTA; RHESUS MACAQUES; NUMERICAL COMPETENCE; SERIAL-ORDER; TRICHROMATIC VISION; COGNITIVE IMITATION; FOOD PREFERENCES; HOMO-SAPIENS; 4-ITEM LISTS; MONKEYS AB Do visual cues such as size, color, and number facilitate sequential recall in orangutans and human children? In Experiment 1, children and adult orangutans solved two types of sequences, arbitrary (unrelated pictures) and meaningful (pictures varied along a spectrum according to the size, color, or number of items shown), in a touchscreen paradigm. It was found that visual cues did not increase the percentage of correct responses for either children or orangutans. In order to demonstrate that the failure to spontaneously seriate along these dimensions was not due to a general inability to perceive the dimensions nor to an inability to seriate items, in Experiment 2, orangutans were trained on one type of sequence and tested on novel sequences organized according to the same rule (i.e., pictures varied on the number spectrum only). The orangutans performed significantly better on novel meaningful sequences in this task than on novel arbitrary sequences. These results indicate that, while orangutans and human children share the ability to learn how to order items according to their size, color, or number, both orangutans and humans lack a cognitive propensity to spontaneously (i.e., without prior training or enculturation) order multiple items by size, color, or number. C1 [Renner, Elizabeth; Subiaul, Francys] George Washington Univ, Ctr Adv Study Human Paleobiol, Dept Anthropol, Washington, DC 20052 USA. [Renner, Elizabeth; Price, Elizabeth E.; Subiaul, Francys] Smithsonian Inst, Natl Zool Pk, Washington, DC 20008 USA. [Subiaul, Francys] George Washington Univ, Dept Speech & Hearing Sci, Washington, DC 20052 USA. RP Renner, E (reprint author), George Washington Univ, Ctr Adv Study Human Paleobiol, Dept Anthropol, 800 22nd St NW, Washington, DC 20052 USA. EM lrenner@gwmail.gwu.edu NR 46 TC 2 Z9 2 U1 7 U2 12 PU SPRINGER HEIDELBERG PI HEIDELBERG PA TIERGARTENSTRASSE 17, D-69121 HEIDELBERG, GERMANY SN 1435-9448 EI 1435-9456 J9 ANIM COGN JI Anim. Cogn. PD JAN PY 2016 VL 19 IS 1 BP 39 EP 52 DI 10.1007/s10071-015-0911-z PG 14 WC Behavioral Sciences; Zoology SC Behavioral Sciences; Zoology GA DA3JX UT WOS:000367694100004 PM 26298671 ER PT J AU Patrick, CJ Weller, DE Ryder, M AF Patrick, Christopher J. Weller, Donald E. Ryder, Micah TI The Relationship Between Shoreline Armoring and Adjacent Submerged Aquatic Vegetation in Chesapeake Bay and Nearby Atlantic Coastal Bays SO ESTUARIES AND COASTS LA English DT Article DE Shoreline hardening; Armoring; Riprap; Bulkhead; SAV; Land use; Land cover ID EELGRASS ZOSTERA-MARINA; WATER-QUALITY; LIGHT AVAILABILITY; SEAGRASS MEADOWS; NURSERY ROLE; ABUNDANCE; COMMUNITIES; SURVIVAL; USA; EUTROPHICATION AB Shoreline armoring is an ancient and globally used engineering strategy to prevent shoreline erosion along marine, estuarine, and freshwater coastlines. Armoring alters the land water interface and has the potential to affect nearshore submerged aquatic vegetation (SAV) by changing nearshore hydrology, morphology, water clarity, and sediment composition. We quantified the relationships between the condition (bulkhead, riprap, or natural) of individual shoreline segments and three measures of directly adjacent SAV (the area of potential SAV habitat, the area occupied by SAV, and the proportion of potential habitat area that was occupied) in the Chesapeake Bay and nearby Atlantic coastal bays. Bulkhead had negative relationships with SAV in the polyhaline and mesohaline zones. Salinity and watershed land cover significantly modified the effect of shoreline armoring on nearshore SAV beds, and the effects of armoring were strongest in polyhaline subestuaries with forested watersheds. In high salinity systems, distance from shore modified the relationship between shoreline and SAV. The negative relationship between bulkhead and SAV was greater further off shore. By using individual shoreline segments as the study units, our analysis separated the effects of armoring and land cover, which were confounded in previous analyses that quantified average armoring and SAV abundance for much larger study units (subestuaries). Our findings suggest that redesigning or removing shoreline armoring structures may benefit nearshore SAV in some settings. Because armoring is ubiquitous, such information can inform efforts to reverse the global decline in SAV and the loss of the ecosystem services that SAV provides. C1 [Patrick, Christopher J.; Weller, Donald E.; Ryder, Micah] Smithsonian Environm Res Ctr, Edgewater, MD 21037 USA. RP Patrick, CJ (reprint author), Smithsonian Environm Res Ctr, 647 Contees Wharf Rd,POB 28, Edgewater, MD 21037 USA. EM cjpatster@gmail.com OI Weller, Donald/0000-0002-7629-5437 FU National Oceanic and Atmospheric Administration (NOAA) Center for Sponsored Coastal Ocean Research (CSCOR) [NA09NOS4780214] FX We thank the Virginia Institute of Marine Sciences, the Maryland Department of Natural Resources, and the Chesapeake Bay Program for providing data used in our analysis. This work was supported by award number NA09NOS4780214 from the National Oceanic and Atmospheric Administration (NOAA) Center for Sponsored Coastal Ocean Research (CSCOR). NR 68 TC 3 Z9 3 U1 7 U2 24 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 1559-2723 EI 1559-2731 J9 ESTUAR COAST JI Estuaries Coasts PD JAN PY 2016 VL 39 IS 1 BP 158 EP 170 DI 10.1007/s12237-015-9970-2 PG 13 WC Environmental Sciences; Marine & Freshwater Biology SC Environmental Sciences & Ecology; Marine & Freshwater Biology GA DA0ZK UT WOS:000367525900013 ER PT J AU Yamato, M Khidas, K Pyenson, ND Fordyce, RE Mead, JG AF Yamato, Maya Khidas, Kamal Pyenson, Nicholas D. Fordyce, R. Ewan Mead, James G. TI Extensively remodeled, fractured cetacean tympanic bullae show that whales can survive traumatic injury to the ears SO JOURNAL OF ANATOMY LA English DT Article DE bone pathology; marine mammal; seismic testing; sonar; tympanic bulla ID HEARING; EVOLUTION; PORPOISE; CALCIUM; SNEEZE; GAS AB Underwater human activities and anthropogenic noise in our oceans may be a major source of habitat degradation for marine life. This issue was highlighted by the opening of the United States Eastern Seaboard for seismic oil and gas exploration in 2014, which generated massive media coverage and widespread concern that seismic surveys could kill or deafen whales. We discovered 11 new specimens of fractured and healed cetacean ear bones, out of a survey of 2127 specimens housed in museum collections. This rare condition has been previously reported only in two specimens of blue whales (Balaenoptera musculus) from the early 1900s, summarized by Fraser & Purves (1953). All of our new specimens are represented by species for which this condition had never been reported previously, including both baleen and toothed whales. The baleen whale specimens (Balaenoptera physalus, Balaenoptera borealis, Balaenoptera acutorostrata) were collected during Canadian commercial whaling operations in the Atlantic Ocean in the 1970s; the specimens include ear bones with well-healed fractures, demonstrating that baleen whales are capable of overcoming traumatic injury to the ears. The toothed whale specimens (Delphinus sp., Berardius bairdii) were found dead on beaches in 1972 and 2001, respectively, with less remodeled fractures. Thus, ear injuries may be more lethal to the echolocating toothed whales, which rely on hearing for navigation and foraging. We explore several hypotheses regarding how these injuries could have occurred, and conclude that the most parsimonious explanations appear to be both direct and indirect effects of lytic processes from disease or calcium depletion, or damage from external pressure waves. Although further research is required to confirm whether the fractures resulted from natural or human-induced events, this study underscores the importance of museum collections and the work of stranding networks in understanding the potential effects of modern human activities on marine mammal health. C1 [Yamato, Maya; Fordyce, R. Ewan; Mead, James G.] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. [Yamato, Maya; Pyenson, Nicholas D.; Fordyce, R. Ewan] Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol, Washington, DC 20560 USA. [Khidas, Kamal] Canadian Museum Nat, Ottawa, ON K1P 6P4, Canada. [Pyenson, Nicholas D.] Burke Museum Nat Hist & Culture, Dept Mammal, Seattle, WA USA. [Pyenson, Nicholas D.] Burke Museum Nat Hist & Culture, Dept Paleontol, Seattle, WA USA. [Fordyce, R. Ewan] Univ Otago, Dept Geol, Dunedin, New Zealand. RP Yamato, M (reprint author), 1000 Constitut Ave NW, Washington, DC 20004 USA. EM yamatom@si.edu FU Peter Buck Postdoctoral Fellowship; Becky Mead Memorial Fund; Smithsonian Women's Committee [32]; Smithsonian Institution's Remington Kellogg Fund; Basis Foundation FX We would like to thank Philippe Ste-Marie and Suzie-Anne Monast (CMN) for helping K. Khidas in sorting the CMN mysticete specimens described in this manuscript, and the work of Edward D. Mitchell, Jr. (formerly of the Arctic Biological Station, Department of Fisheries and Oceans, Canada), for building these collections. Charles W. Potter (USNM) provided critical expertise and assistance throughout this project. Moe Flannery and Laura Wilkinson (CAS) and Chris Conroy (MVZ) kindly provided us with access to the Delphinus and Berardius specimens. Robert E. Jones was instrumental in contacting Ulan McKnight and Adam P. Summers for field photos and notes of MVZ 208600. Bill Walker (formerly of National Marine Mammal Laboratory) provided essential information for finding the Delphinus specimen. We also thank David Hunt (USNM) and Rachel Roston (Duke University) for insight regarding bone pathologies, and Raphaela Stimmelmayr (North Slope Borough Department of Wildlife Management) for providing us with relevant literature. Sentiel Rommel (University of North Carolina, Wilmington), Alex Werth (Hampden-Sydney College), and two anonymous reviewers provided insightful comments, which greatly improved this manuscript. Special thanks to Kristofer Helgen (USNM), whose mentorship of Maya Yamato allowed this project to take place. Yamato was supported by the Peter Buck Postdoctoral Fellowship, Becky Mead Memorial Fund, and along with Pyenson was supported with funding from the Smithsonian Women's Committee (Award #32), the Smithsonian Institution's Remington Kellogg Fund, and the Basis Foundation. Fordyce acknowledges the excellent library resources of the University of Otago, and support for research travel to MVZ. The authors declare no conflicts of interest. NR 44 TC 0 Z9 0 U1 7 U2 24 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0021-8782 EI 1469-7580 J9 J ANAT JI J. Anat. PD JAN PY 2016 VL 228 IS 1 BP 125 EP 136 DI 10.1111/joa.12385 PG 12 WC Anatomy & Morphology SC Anatomy & Morphology GA DA3FH UT WOS:000367681800012 PM 26391309 ER PT J AU Ashton, LA Nakamura, A Basset, Y Burwell, CJ Cao, M Eastwood, R Odell, E de Oliveira, EG Hurley, K Katabuchi, M Maunsell, S McBroom, J Schmidl, J Sun, ZH Tang, Y Whitaker, T Laidlaw, MJ McDonald, WJF Kitching, RL AF Ashton, Louise A. Nakamura, Akihiro Basset, Yves Burwell, Chris J. Cao, Min Eastwood, Rodney Odell, Erica de Oliveira, Evandro Gama Hurley, Karen Katabuchi, Masatoshi Maunsell, Sarah McBroom, James Schmidl, Juergen Sun, Zhenhua Tang, Yong Whitaker, Terry Laidlaw, Melinda J. McDonald, William J. F. Kitching, Roger L. TI Vertical stratification of moths across elevation and latitude SO JOURNAL OF BIOGEOGRAPHY LA English DT Article DE beta diversity; biodiversity; canopy; elevation; IBISCA; Lepidoptera; macroecology; macrolepidoptera; tropical rain forest; vertical compartmentalization ID LOWLAND RAIN-FOREST; BETA-DIVERSITY; LARGE-SCALE; SPECIES-DIVERSITY; TROPICAL FOREST; BIODIVERSITY; PATTERNS; INSECTS; ASSEMBLAGES; GRADIENTS AB Aim There is little consensus as to whether stratification of arthropods between canopy and understorey in tropical and subtropical forests is commonplace and if the magnitude of stratification changes across different elevations and latitudes. We investigated broad-scale patterns of vertical stratification of moths collected from extensive cross-continental fieldwork in a variety of forest types, climates, elevations, latitudes and areas with differing biogeographical history. Location Tropical and subtropical rain forest in eastern Australia; tropical, subtropical and subalpine forest in Yunnan Province, China; and tropical rain forest in Panama, Vietnam, Brunei and Papua New Guinea. Methods Night-flying moths were trapped from the upper canopy and understorey. We generated a total of 64 data sets to quantify vertical stratification of moths in terms of their species richness, using coverage-based rarefaction, and assemblage composition, using standardized hierarchical beta diversity. Based on the average temperature lapse rate, we incorporated latitudinal differences into elevation and generated 'corrected' elevation for each location, and analysed its relationships with the magnitude of stratification. Results We found consistent differences between canopy and understorey assemblages at almost all rain forest locations across corrected elevational gradients. The magnitude of vertical stratification in species richness did not change with increasing corrected elevation. In contrast, the difference in assemblage composition increased with increasing corrected elevation in the Northern Hemisphere, while the opposite, albeit weak, trend was found in the Southern Hemisphere. Main conclusions Clear vertical stratification was evident in moth assemblages regardless of elevation and latitude. However, the degree to which assemblages are stratified between canopy and understorey is not uniformly related to elevation and latitude. Inconsistencies in the magnitude of vertical stratification between the Northern and Southern Hemisphere, may reflect, on one hand, deep-time biogeographical differences between the land masses studied and, on the other, place-to-place differences in resource availability underpinning the observed moth assemblages. C1 [Ashton, Louise A.; Nakamura, Akihiro; Burwell, Chris J.; Eastwood, Rodney; Odell, Erica; Hurley, Karen; Maunsell, Sarah; McBroom, James; Kitching, Roger L.] Griffith Univ, Environm Futures Res Inst, Nathan, Qld 4111, Australia. [Ashton, Louise A.; Nakamura, Akihiro; Burwell, Chris J.; Eastwood, Rodney; Odell, Erica; Hurley, Karen; Maunsell, Sarah; McBroom, James; Kitching, Roger L.] Griffith Univ, Griffith Sch Environm, Nathan, Qld 4111, Australia. [Ashton, Louise A.; Nakamura, Akihiro; Cao, Min; Katabuchi, Masatoshi; Sun, Zhenhua; Tang, Yong; Kitching, Roger L.] Chinese Acad Sci, Key Lab Trop Forest Ecol, Xishuangbanna Trop Bot Garden, Mengla 666303, Yunnan, Peoples R China. [Ashton, Louise A.] Nat Hist Museum, Dept Life Sci, London SW7 5BD, England. [Nakamura, Akihiro; Burwell, Chris J.] Queensland Museum, South Brisbane, Qld 4101, Australia. [Basset, Yves] Smithsonian Trop Res Inst, Panama City, Panama. [Eastwood, Rodney] ETH, CH-8092 Zurich, Switzerland. [de Oliveira, Evandro Gama] Ctr Univ Una, BR-30180100 Belo Horizonte, MG, Brazil. [Hurley, Karen] Univ Queensland, ARC Ctr Excellence Environm Decis, Brisbane, Qld 4067, Australia. [Katabuchi, Masatoshi] Univ Florida, Dept Biol, Gainesville, FL 32611 USA. [Schmidl, Juergen] Univ Erlangen Nurnberg, Dept Biol, D-91058 Erlangen, Bavaria, Germany. [Whitaker, Terry] Crowtrees, Lancaster LA27EE, England. [Laidlaw, Melinda J.; McDonald, William J. F.] Queensland Herbarium, Dept Sci Informat Technol & Innovat, Toowong, Qld 4066, Australia. RP Nakamura, A (reprint author), Chinese Acad Sci, Key Lab Trop Forest Ecol, Xishuangbanna Trop Bot Garden, Mengla 666303, Yunnan, Peoples R China. EM a.nakamura@xtbg.ac.cn RI Basset, Yves/B-6642-2014 FU Griffith University School of Environment; Environmental Futures Research Institute; Cooperative Research Centre for Tropical Rainforest Ecology and Management; Earthwatch Organisation; Terrestrial Ecosystem Research Network (TERN); Queensland Government Smart State Initiative; Queensland Museum; Queensland Herbarium; SEQ Catchments; Global Canopy Program; The Queensland National Parks Association; Conservation Volunteers Queensland; Queensland-Chinese Academy of Science Biotechnology Fund [GJHZ1130]; Xishuangbanna Tropical Botanic Garden; Chinese Academy of Sciences; Kunming Institute of Zoology; Czech Science Foundation (GACR grant) [41-14-36068G]; SolVin Solvay SA; STRI, the United Nations Environment Programme; Walcott Fund of the Smithsonian Institution; European Science Foundation; Global Canopy Programme FX This paper is the product of many different projects, and would not have been possible without many funding bodies and much volunteer help. Griffith University School of Environment and the Environmental Futures Research Institute supported all research presented here. Research on the one-hectare plots was supported financially over many years by the Cooperative Research Centre for Tropical Rainforest Ecology and Management and the Earthwatch Organisation. Atherton research was funded by the Terrestrial Ecosystem Research Network (TERN); these data are available for use by other researchers (http://tern.org.au/). Lamington National Park data were collected during the IBISCA-Queensland project, funded by the Queensland Government Smart State Initiative, Queensland Museum, Queensland Herbarium, SEQ Catchments, the Global Canopy Program and The Queensland National Parks Association. Border Ranges research would not have been possible without the botanical expertise of John Hunter and Stephanie Horton. Support was also provided by Conservation Volunteers Queensland. Work in China was funded by the Queensland-Chinese Academy of Science Biotechnology Fund (GJHZ1130), in collaboration with Xishuangbanna Tropical Botanic Garden, Chinese Academy of Sciences and the Kunming Institute of Zoology. The IBISCA-Panama study was an initiative of Pro-Natura International, Ocean Vert, Blaise-Pascal University, the University of Panama and the Smithsonian Tropical Research Institute (STRI), with core funding from Czech Science Foundation (GACR grant 41-14-36068G), SolVin Solvay SA, STRI, the United Nations Environment Programme, the Walcott Fund of the Smithsonian Institution, the European Science Foundation and the Global Canopy Programme. We thank Elliot Leach and Nigel Stork for their helpful comments on earlier drafts of the manuscript. NR 57 TC 2 Z9 2 U1 10 U2 36 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0305-0270 EI 1365-2699 J9 J BIOGEOGR JI J. Biogeogr. PD JAN PY 2016 VL 43 IS 1 BP 59 EP 69 DI 10.1111/jbi.12616 PG 11 WC Ecology; Geography, Physical SC Environmental Sciences & Ecology; Physical Geography GA DA3IT UT WOS:000367691100006 ER PT J AU McShea, WJ Forrester, T Costello, R He, ZH Kays, R AF McShea, William J. Forrester, Tavis Costello, Robert He, Zhihai Kays, Roland TI Volunteer-run cameras as distributed sensors for macrosystem mammal research SO LANDSCAPE ECOLOGY LA English DT Article DE Camera traps; Cyberinfrastructure; Standard metadata; Citizen science; eMammal; Macrosystem ID SPECIES DISTRIBUTION MODELS; ESTIMATING SITE OCCUPANCY; CITIZEN SCIENCE; ECOLOGICAL RESEARCH; PROTECTED AREAS; CONSERVATION; POPULATION; HABITAT; TOOL; PERFORMANCE AB Variation in the abundance of animals affects a broad range of ecosystem processes. However, patterns of abundance for large mammals, and the effects of human disturbances on them are not well understood because we lack data at the appropriate scales. We created eMammal to effectively camera-trap at landscape scale. Camera traps detect animals with infrared sensors that trigger the camera to take a photo, a sequence of photos, or a video clip. Through photography, camera traps create records of wildlife from known locations and dates, and can be set in arrays to quantify animal distribution across a landscape. This allows linkage to other distributed networks of ecological data. Through the eMammal program, we demonstrate that volunteer-based camera trapping can meet landscape scale spatial data needs, while also engaging the public in nature and science. We assert that camera surveys can be effectively scaled to a macrosystem level through citizen science, but only after solving challenges of data and volunteer management. We present study design and technology solutions for landscape scale camera trapping to effectively recruit, train and retain volunteers while providing efficient data workflows and quality control. Our initial work with > 400 volunteers across six contiguous U.S. states has proven that citizen scientists can deploy these camera traps properly (94 % of volunteer deployments correct) and tag the photos accurately for most species (67-100 %). Using these tools we processed 2.6 million images over a 2 year period. The eMammal cyberinfrastructure made it possible to process far more data than any participating researcher had previously achieved. The core components include an upload application using a standard metadata format, an expert review tool to ensure data quality, and a curated data repository. Macrosystem scale monitoring of wildlife by volunteer-run camera traps can produce the data needed to address questions concerning broadly distributed mammals, and also help to raise public awareness on the science of conservation. This scale of data will allow for linkage of large mammals to ecosystem processes now measured through national programs. C1 [McShea, William J.; Forrester, Tavis] Smithsonian Conservat Biol Inst, Conservat Ecol Ctr, Natl Zool Pk, Front Royal, VA 22630 USA. [Costello, Robert] Smithsonians Natl Museum Nat Hist, Off Educ & Outreach, Washington, DC 20560 USA. [He, Zhihai] Univ Missouri, Dept Elect & Comp Engn, Columbia, MO 65211 USA. [Kays, Roland] North Carolina Museum Nat Sci, Raleigh, NC 27601 USA. [Kays, Roland] N Carolina State Univ, Dept Forestry & Environm Resources, Raleigh, NC 27695 USA. RP McShea, WJ (reprint author), Smithsonian Conservat Biol Inst, Conservat Ecol Ctr, Natl Zool Pk, 1500 Remount Rd, Front Royal, VA 22630 USA. EM mcsheaw@si.edu NR 55 TC 9 Z9 10 U1 10 U2 52 PU SPRINGER PI DORDRECHT PA VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS SN 0921-2973 EI 1572-9761 J9 LANDSCAPE ECOL JI Landsc. Ecol. PD JAN PY 2016 VL 31 IS 1 BP 55 EP 66 DI 10.1007/s10980-015-0262-9 PG 12 WC Ecology; Geography, Physical; Geosciences, Multidisciplinary SC Environmental Sciences & Ecology; Physical Geography; Geology GA DA2AR UT WOS:000367598200006 ER PT J AU Corrales, A Arnold, AE Ferrer, A Turner, BL Dalling, JW AF Corrales, Adriana Arnold, A. Elizabeth Ferrer, Astrid Turner, Benjamin L. Dalling, James W. TI Variation in ectomycorrhizal fungal communities associated with Oreomunnea mexicana (Juglandaceae) in a Neotropical montane forest SO MYCORRHIZA LA English DT Article DE Beta diversity; Community structure; Fortuna; Forest Reserve; Mycorrhizal networks; Russula (Russulaccac) ID TROPICAL RAIN-FOREST; SUCCESSIONAL GLACIER FOREFRONT; MIXED-CONIFER FOREST; OAKS QUERCUS SPP.; FINE-ROOT BIOMASS; MYCORRHIZAL NETWORKS; SEEDLING SURVIVAL; CANOPY TREES; NUTRIENT GRADIENT; SOUTH CAMEROON AB Neotropical montane forests are often dominated by ectomycorrhizal (EM) tree species, yet the diversity of their EM fungal communities remains poorly explored. In lower montane forests in western Panama, the EM tree species Oreomunnea mexicana (Juglandaceae) forms locally dense populations in forest otherwise characterized by trees that form arbuscular mycorrhizal (AM) associations. The objective of this study was to compare the composition of EM fungal communities associated with Oreomunnea adults, saplings, and seedlings across sites differing in soil fertility and the amount and seasonality of rainfall. Analysis of fungal nrITS DNA (nuclear ribosomal internal transcribed spacers) revealed 115 EM fungi taxa from 234 EM root tips collected from adults, saplings, and seedlings in four sites. EM fungal communities were equally species-rich and diverse across Oreomunnea developmental stages and sites, regardless of soil conditions or rainfall patterns. However, ordination analysis revealed high compositional turnover between low and high fertility/rainfall sites located ca. 6 km apart. The EM fungal community was dominated by Russula (ca. 36 taxa). Cortinarius, represented by 14 species and previously reported to extract nitrogen from organic sources under low nitrogen availability, was found only in low fertility/high rainfall sites. Phylogenetic diversity analyses of Russula revealed greater evolutionary distance among taxa found on sites with contrasting fertility and rainfall than was expected by chance, suggesting that environmental differences among sites may be important in structuring EM fungal communities. More research is needed to evaluate whether EM fungal taxa associated with Oreomunnea form mycorrhizal networks that might account for local dominance of this tree species in otherwise diverse forest communities. C1 [Corrales, Adriana; Ferrer, Astrid; Dalling, James W.] Univ Illinois, Dept Plant Biol, Urbana, IL 61801 USA. [Arnold, A. Elizabeth] Univ Arizona, Sch Plant Sci, Tucson, AZ 85721 USA. [Arnold, A. Elizabeth] Univ Arizona, Dept Ecol & Evolutionary Biol, Tucson, AZ 85721 USA. [Turner, Benjamin L.; Dalling, James W.] Smithsonian Trop Res Inst, Panama City 084303092, Panama. RP Corrales, A (reprint author), Univ Illinois, Dept Plant Biol, Urbana, IL 61801 USA. EM corrlssr@illinois.edu RI Turner, Benjamin/E-5940-2011 OI Turner, Benjamin/0000-0002-6585-0722 FU Tinker Summer Research Fellowship; Francis M. and Harlie M. Clark Research support grant; University of Arizona; College of Agriculture and Life Sciences at The University of Arizona; Smithsonian Tropical Research Institute Short-Term Fellowship program; Government of Panama (SENACYT) [COLO08-003] FX Funding from a Tinker Summer Research Fellowship, a Francis M. and Harlie M. Clark Research support grant, a Robert L. Gilbertson Mycological Herbarium Grant (University of Arizona), the College of Agriculture and Life Sciences at The University of Arizona, and the Smithsonian Tropical Research Institute Short-Term Fellowship program is gratefully acknowledged. We sincerely thank two anonymous reviewers whose comments greatly improved the manuscript. Forest plot work was supported by grant COLO08-003 from the Government of Panama (SENACYT). We thank Kayla Arendt, Jana U'Ren, Katy Heath, and Pat Burke for assistance with molecular work, and Katie Heineman, Carmen Velasquez, Carlos Espinosa, and Marggie Rodriguez for their help in the field. NR 119 TC 3 Z9 3 U1 2 U2 25 PU SPRINGER PI NEW YORK PA 233 SPRING ST, NEW YORK, NY 10013 USA SN 0940-6360 EI 1432-1890 J9 MYCORRHIZA JI Mycorrhiza PD JAN PY 2016 VL 26 IS 1 BP 1 EP 17 DI 10.1007/s00572-015-0641-8 PG 17 WC Mycology SC Mycology GA DA5AH UT WOS:000367814000001 PM 25940407 ER PT J AU Pikovski, I Zych, M Costa, F Brukner, C AF Pikovski, Igor Zych, Magdalena Costa, Fabio Brukner, Caslav TI Reply to 'Questioning universal decoherence due to gravitational time dilation' SO NATURE PHYSICS LA English DT Letter C1 [Pikovski, Igor] Harvard Smithsonian Ctr Astrophys, ITAMP, Cambridge, MA 02138 USA. [Pikovski, Igor] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA. [Zych, Magdalena; Costa, Fabio] Univ Queensland, Sch Math & Phys, Ctr Engn Quantum Syst, St Lucia, Qld 4072, Australia. [Brukner, Caslav] Univ Vienna, Fac Phys, Vienna Ctr Quantum Sci & Technol VCQ, A-1090 Vienna, Austria. [Brukner, Caslav] Austrian Acad Sci, IQOQI, A-1090 Vienna, Austria. RP Pikovski, I (reprint author), Harvard Smithsonian Ctr Astrophys, ITAMP, 60 Garden St, Cambridge, MA 02138 USA. EM igor.pikovski@cfa.harvard.edu RI Costa, Fabio/G-3746-2014; Zych, Magdalena/G-4007-2014; OI Costa, Fabio/0000-0002-6547-6005; Zych, Magdalena/0000-0002-8356-7613; Pikovski, Igor/0000-0002-9441-2553 NR 7 TC 1 Z9 1 U1 1 U2 7 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 1745-2473 EI 1745-2481 J9 NAT PHYS JI Nat. Phys. PD JAN PY 2016 VL 12 IS 1 BP 2 EP 3 DI 10.1038/nphys3650 PG 3 WC Physics, Multidisciplinary SC Physics GA DA5IA UT WOS:000367835400003 ER PT J AU Leu, ST Farine, DR Wey, TW Sih, A Bull, CM AF Leu, Stephan T. Farine, Damien R. Wey, Tina W. Sih, Andrew Bull, C. Michael TI Environment modulates population social structure: experimental evidence from replicated social networks of wild lizards SO ANIMAL BEHAVIOUR LA English DT Article DE environmental variation; habitat complexity; lizard; movement; Scincidae; social network; social structure ID TILIQUA-RUGOSA; SLEEPY LIZARD; TRACHYDOSAURUS-RUGOSUS; AUSTRALIAN LIZARD; HABITAT COMPLEXITY; MOVEMENT PATTERNS; SELFISH HERD; GROUP-SIZE; BEHAVIOR; FOOD AB Social structure is a fundamental component of a population that drives ecological and evolutionary processes ranging from parasite transmission to sexual selection. Nevertheless, we have much to learn about factors that explain variation in social structure. We used advances in biologging and social network analysis to experimentally test how the local habitat, and specifically habitat complexity, modulates social structure at different levels in wild populations. Sleepy lizards, Tiliqua rugosa, establish nonrandom social networks that are characterized by avoidance of some neighbours and frequent interactions with one opposite-sex individual. Using synchronous GPS locations of all adult lizards, we constructed social networks based on spatial proximity of individuals. We increased habitat structural complexity in two study populations by adding 100 short fences across the landscape. We then compared the resulting movement behaviour and social structure between these populations and two unmanipulated populations. Social connectivity (network density) and social stability, measured at weekly intervals, were greater in populations with increased habitat structural complexity. The level of agonistic interaction (quantified as scale damage) was also higher, indicating a fitness cost of greater social connectivity. However, some network parameters were unaffected by increased complexity, including disassortative mixing by sex, and at the individual level, social differentiation among associates (coefficient of variation of edge weights) and maximal interaction frequencies (maximal edge weight). This suggests divergent effects of changed ecological conditions on individual association behaviour compared to the resulting social structure of the population. Our results contrast with those from studies of more gregarious species, in which higher structural complexity in the environment relaxed the social connectivity. This shows that the response to altered ecological conditions can differ fundamentally between species or between populations, and we suggest that it depends on their tendency for gregarious behaviour. (C) 2015 The Association for the Study of Animal Behaviour. Published by Elsevier Ltd. All rights reserved. C1 [Leu, Stephan T.; Bull, C. Michael] Flinders Univ S Australia, Sch Biol Sci, Adelaide, SA 5001, Australia. [Farine, Damien R.] Univ Oxford, Dept Zool, Edward Grey Inst Field Ornithol, Oxford, England. [Farine, Damien R.] Univ Calif Davis, Dept Anthropol, Davis, CA 95616 USA. [Farine, Damien R.] Smithsonian Trop Res Inst, Ancon, Panama. [Wey, Tina W.; Sih, Andrew] Univ Calif Davis, Dept Environm Sci & Policy, Davis, CA 95616 USA. [Wey, Tina W.] New Mexico State Univ, Dept Biol, Las Cruces, NM 88003 USA. RP Leu, ST (reprint author), Flinders Univ S Australia, Sch Biol Sci, POB 2100, Adelaide, SA 5001, Australia. EM stephan.leu@flinders.edu.au OI Wey, Tina/0000-0002-1928-5881; Bull, Michael/0000-0002-9350-5950 FU Australian Research Council [DP130100145]; National Science Foundation [EAGER-IOS-1250895]; Biotechnology and Biological Sciences Research Council [BB/L006081/1]; National Science Foundation postdoctoral fellowship in Biology [1003282] FX The research was funded by a grant from the Australian Research Council (DP130100145) to C.M.B. D.R.F. received additional funding from the National Science Foundation (EAGER-IOS-1250895) to Margaret Crofoot and the Biotechnology and Biological Sciences Research Council (BB/L006081/1) to Ben Sheldon. T.W.W. was supported by an National Science Foundation postdoctoral fellowship in Biology (1003282). We thank Lewis McPherson and Victor Etevenot for their assistance with fieldwork, Ron and Leona Clark for allowing access to their land, Geoff Cottrell for maintaining the data loggers and Dale Burzacott for logistical support at the field site. NR 70 TC 8 Z9 8 U1 17 U2 56 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0003-3472 EI 1095-8282 J9 ANIM BEHAV JI Anim. Behav. PD JAN PY 2016 VL 111 BP 23 EP 31 DI 10.1016/j.anbehav.2015.10.001 PG 9 WC Behavioral Sciences; Zoology SC Behavioral Sciences; Zoology GA CZ8UG UT WOS:000367374000005 ER PT J AU Kralj-Fiser, S Candek, K Lokovsek, T Celik, T Cheng, RC Elgar, MA Kuntner, M AF Kralj-Fiser, Simona Candek, Klemen Lokovsek, Tjasa Celik, Tatjana Cheng, Ren-Chung Elgar, Mark A. Kuntner, Matjaz TI Mate choice and sexual size dimorphism, not personality, explain female aggression and sexual cannibalism in raft spiders SO ANIMAL BEHAVIOUR LA English DT Article DE aggressive spillover; mate size difference; mating; personality; sexual cannibalism; voracity ID SOCIALLY POLYMORPHIC SPIDER; ORB-WEB SPIDER; BEHAVIORAL SYNDROMES; DOLOMEDES-TRITON; FISHING SPIDER; SPILLOVER HYPOTHESIS; FITNESS CONSEQUENCES; EVOLUTION; REPEATABILITY; PLASTICITY AB Intersexual agonistic encounters prior to mating are thought to result from the 'spillover' of the advantages of a voracious personality within a foraging context that is maladaptive in a mating context. We tested this idea by examining the repeatability and cross-context consistency of aggressive behaviours associated with foraging and mating in the raft spider, Dolomedes fimbriatus, in which some, highly voracious females reportedly kill approaching males and thus remain unmated. We failed to find support for a maladaptive spillover of voracious female personality. While females exhibited consistent inter-individual differences in voracity towards prey, voracity did not correlate with female aggressiveness towards males. Instead, we show that female D. fimbriatus adjusted their tendency to attack courting males according to their size relative to the male. Females commonly attacked males during or after copulation, but sexual cannibalism depended on relative mate size difference, with mating success tending to be compromised in females with lower body weight. (C) 2015 The Association for the Study of Animal Behaviour. Published by Elsevier Ltd. All rights reserved. C1 [Kralj-Fiser, Simona; Candek, Klemen; Lokovsek, Tjasa; Celik, Tatjana; Cheng, Ren-Chung; Kuntner, Matjaz] Biol Inst ZRC SAZU, Evolutionary Zool Lab, Ljubljana 1000, Slovenia. [Kralj-Fiser, Simona] Univ Primorska, Fac Math Nat Sci & Informat Technol, Koper, Slovenia. [Elgar, Mark A.] Univ Melbourne, Sch Biosci, Melbourne, Vic, Australia. [Kuntner, Matjaz] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. [Kuntner, Matjaz] Hubei Univ, Coll Life Sci, CBEE, Wuhan, Hubei, Peoples R China. RP Kralj-Fiser, S (reprint author), Biol Inst ZRC SAZU, Evolutionary Zool Lab, Novi Trg 2, Ljubljana 1000, Slovenia. EM simonakf@gmail.com OI Elgar, Mark/0000-0003-0861-6064 FU Slovenian Research Agency [P1-0236, J1-6729] FX We thank Petri T. Niemela for calculations of adjusted repeatability and Raphael Royaute for helping us with statistics. We thank M. Gregoric, K. Suen, C. Fiser and U. Pristovsek for their help in the lab and in the field. We thank J.M. Schneider for numerous discussions. S.K.F., K.C., T.L., T.C. and M.K. were supported by the Slovenian Research Agency (grants P1-0236, J1-6729). NR 50 TC 5 Z9 5 U1 29 U2 73 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0003-3472 EI 1095-8282 J9 ANIM BEHAV JI Anim. Behav. PD JAN PY 2016 VL 111 BP 49 EP 55 DI 10.1016/j.anbehav.2015.10.013 PG 7 WC Behavioral Sciences; Zoology SC Behavioral Sciences; Zoology GA CZ8UG UT WOS:000367374000008 ER PT J AU Robinson, H AF Robinson, Harold TI The genus Fleischmannia in Argentina, Bolivia, Brazil and Paraguay (Eupatorieae, Asteraceae) SO PHYTOKEYS LA English DT Article DE Fleischmannia; Argentina; Bolivia; Brazil; Paraguay; new taxa AB Species of the genus Fleischmannia from Argentina, Bolivia, Brazil and Paraguay are reviewed, and keys are provided that cover the species in each country. New taxa described are Fleischmannia hatschbachii, F. matogrosensis, F. microstemon var paniculata from Brazil, F. hassleri from Paraguay and F. neei and F. steinbachii from Bolivia, and one new combination for a F. prasiifolia variety is provided. The additions bring the total known species of the genus to 102. C1 [Robinson, Harold] Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, Washington, DC 20013 USA. RP Robinson, H (reprint author), Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, MRC 166,POB 37012, Washington, DC 20013 USA. EM robinsoh@si.edu NR 5 TC 0 Z9 0 U1 0 U2 1 PU PENSOFT PUBL PI SOFIA PA 12 PROF GEORGI ZLATARSKI ST, SOFIA, 1700, BULGARIA SN 1314-2011 EI 1314-2003 J9 PHYTOKEYS JI PhytoKeys PY 2016 VL 57 BP 61 EP 92 DI 10.3897/phytokeys.57.5784 PG 32 WC Plant Sciences SC Plant Sciences GA DA1FG UT WOS:000367541100004 ER PT J AU Herman, RDK AF Herman, R. D. K. TI Traditional knowledge in a time of crisis: climate change, culture and communication SO SUSTAINABILITY SCIENCE LA English DT Article DE Sustainability; Values; Scientism; Indigenous; Wisdom ID GEOGRAPHIES; DISENCHANTMENT; POSTHUMAN; SCIENCE; WORLD AB Science as it has come to be defined in Western thought is at the root of our current environmental problems. This article reviews the historical trajectory of specific facets in Western thought, including the disenchantment of nature, the apotheosis of reason, the technological domination of nature, and the Puritan temper. Illuminating this history points out that what is called "rational" and what popularly acceptable as "science" is in fact a by-product of specific historical, cultural, and political circumstances, and has produced a culture of "scientism" that is ideological, not value-free, and is in fact contrary to the open inquiry of science. These ideas are linked to economic rationality, colonialism, and human rights, severing modern humans from our Indigenous roots and fostering an ideology of rapacious environmental exploitation. The author proposes "indigeneity" as embracing the holistic knowledge and wisdom found in traditional cultures while also utilizing the advances in science and other areas of human endeavor. Specifically, the paper argues for bringing about a new cultural discourse that helps reshape human behavior into a more sustainable direction. The role of communication and storytelling is emphasized, with an example given in the story of Polynesian voyaging and the five values of the voyaging canoe. C1 [Herman, R. D. K.] Smithsonian Natl Museum Amer Indian, Washington, DC 20013 USA. RP Herman, RDK (reprint author), Smithsonian Natl Museum Amer Indian, POB 37012,MRC 590, Washington, DC 20013 USA. EM hermand@si.edu NR 60 TC 2 Z9 2 U1 5 U2 23 PU SPRINGER JAPAN KK PI TOKYO PA CHIYODA FIRST BLDG EAST, 3-8-1 NISHI-KANDA, CHIYODA-KU, TOKYO, 101-0065, JAPAN SN 1862-4065 EI 1862-4057 J9 SUSTAIN SCI JI Sustain. Sci. PD JAN PY 2016 VL 11 IS 1 BP 163 EP 176 DI 10.1007/s11625-015-0305-9 PG 14 WC GREEN & SUSTAINABLE SCIENCE & TECHNOLOGY; Environmental Sciences SC Science & Technology - Other Topics; Environmental Sciences & Ecology GA CZ8JZ UT WOS:000367347300014 ER PT J AU Edwards, KL Trotter, J Jones, M Brown, JL Steinmetz, HW Walker, SL AF Edwards, Katie L. Trotter, Jessica Jones, Martin Brown, Janine L. Steinmetz, Hanspeter W. Walker, Susan L. TI Investigating temporary acyclicity in a captive group of Asian elephants (Elephas maximus): Relationship between management, adrenal activity and social factors SO GENERAL AND COMPARATIVE ENDOCRINOLOGY LA English DT Article DE Temporary acyclicity; Animal welfare; Asian elephant; Glucocorticoids; Management; Oestrous synchrony; Reproduction ID LOXODONTA-AFRICANA ELEPHANTS; OVARIAN ACTIVITY; ZOO ELEPHANTS; REPRODUCTIVE CYCLICITY; CHEMICAL COMMUNICATION; ENZYME-IMMUNOASSAY; CENTRAL MECHANISMS; ESTROUS SYNCHRONY; DOMINANCE STATUS; BIRTH SYNCHRONY AB Routine faecal steroid monitoring has been used to aid the management of five captive Asian elephant (Elephas maximus) females at Chester Zoo, UK, since 2007. Progestagen analysis initially revealed synchronised oestrous cycles among all females. However, a 14- to 20-week period of temporary acyclicity subsequently occurred in three females, following several management changes (increased training, foot-care and intermittent matriarch removal for health reasons) and the initiation of pregnancy in another female. The aim of this study was to retrospectively investigate whether these management changes were related to increased adrenal activity and disruption of ovarian activity, or whether social factors may have been involved in the temporary cessation of cyclicity. Faecal samples collected every other day were analysed to investigate whether glucocorticoid metabolites were related to reproductive status (pregnant, cycling, acyclic) or management (training, foot-care, matriarch presence). Routine training and foot-care were not associated with adrenal activity; however, intensive foot-care to treat an abscess in one female was associated with increased glucocorticoid concentration. Matriarch presence influenced adrenal activity in three females, being lower when the matriarch was separated from the group at night compared to being always present. However, in the females that exhibited temporary acyclicity, there was no consistent relationship between glucocorticoids and cyclicity state. Although the results of this study do not fully explain this occurrence, the highly synchronised nature of oestrous cycles within this group, and the concurrent acyclicity in three females, raises the question of whether social factors could have been involved in the temporary disruption of ovarian activity. (C) 2015 Elsevier Inc. All rights reserved. C1 [Edwards, Katie L.; Trotter, Jessica; Steinmetz, Hanspeter W.; Walker, Susan L.] Chester Zoo, North England Zool Soc, Upton By Chester CH2 1LH, Cheshire, England. [Edwards, Katie L.; Brown, Janine L.] Smithsonian Conservat Biol Inst, Ctr Species Survival, Front Royal, VA 22630 USA. [Trotter, Jessica; Jones, Martin] Manchester Metropolitan Univ, Manchester M1 5G, Lancs, England. [Steinmetz, Hanspeter W.] Schweizer Natl Circus AG, Gebruder Knie, CH-8640 Rapperswil, Switzerland. RP Edwards, KL (reprint author), Smithsonian Conservat Biol Inst, Ctr Species Survival, 1500 Remount Rd, Front Royal, VA 22630 USA. EM edwardskl@si.edu; s.walker@chesterzoo.org FU Chester Zoo, UK FX This research was funded by Chester Zoo, UK. We would like to thank the elephant team at Chester Zoo, UK for collection of faecal samples and detailed husbandry information. We also thank the endocrine laboratory technicians and volunteers for processing and extracting faecal samples. NR 79 TC 0 Z9 0 U1 4 U2 31 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 0016-6480 EI 1095-6840 J9 GEN COMP ENDOCR JI Gen. Comp. Endocrinol. PD JAN 1 PY 2016 VL 225 BP 104 EP 116 DI 10.1016/j.ygcen.2015.09.011 PG 13 WC Endocrinology & Metabolism SC Endocrinology & Metabolism GA CZ2RT UT WOS:000366953000011 PM 26393308 ER PT J AU Wagreich, M Haq, BU Melinte-Dobrinescu, M Sames, B Yilmaz, IO AF Wagreich, Michael Haq, Bilal U. Melinte-Dobrinescu, Mihaela Sames, Benjamin Yilmaz, Ismail O. TI Advances and Perspectives in Understanding Cretaceous Sea-level Change Preface SO PALAEOGEOGRAPHY PALAEOCLIMATOLOGY PALAEOECOLOGY LA English DT Editorial Material C1 [Wagreich, Michael; Sames, Benjamin] Univ Vienna, Ctr Earth Sci, Dept Geodynam & Sedimentol, A-1090 Vienna, Austria. [Haq, Bilal U.] Smithsonian Inst, Washington, DC 20560 USA. [Haq, Bilal U.] Sorbonne Pierre & Marie Curie Univ, Paris, France. [Melinte-Dobrinescu, Mihaela] Natl Inst Geol & Geoecol GeoEcoMar, Bucharest 024053, Romania. [Yilmaz, Ismail O.] Middle E Tech Univ, Dept Geol Engn, TR-06800 Ankara, Turkey. RP Wagreich, M (reprint author), Univ Vienna, Ctr Earth Sci, Dept Geodynam & Sedimentol, Althanstr 14, A-1090 Vienna, Austria. EM michael.wagreich@univie.ac.at; bhaq@inbox.com; melinte@geoecomar.ro; benjamin.sames@univie.ac.at; ioyilmaz@metu.edu.tr NR 0 TC 3 Z9 3 U1 2 U2 11 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0031-0182 EI 1872-616X J9 PALAEOGEOGR PALAEOCL JI Paleogeogr. Paleoclimatol. Paleoecol. PD JAN 1 PY 2016 VL 441 SI SI BP 391 EP 392 DI 10.1016/j.palaeo.2015.10.040 PN 3 PG 2 WC Geography, Physical; Geosciences, Multidisciplinary; Paleontology SC Physical Geography; Geology; Paleontology GA CZ5AF UT WOS:000367113800001 ER PT J AU Sames, B Wagreich, M Wendler, JE Haq, BU Conrad, CP Melinte-Dobrinescu, MC Hu, X Wendler, I Wolfgring, E Yilmaz, IO Zorina, SO AF Sames, B. Wagreich, M. Wendler, J. E. Haq, B. U. Conrad, C. P. Melinte-Dobrinescu, M. C. Hu, X. Wendler, I. Wolfgring, E. Yilmaz, I. O. Zorina, S. O. TI Review: Short-term sea-level changes in a greenhouse world - A view from the Cretaceous SO PALAEOGEOGRAPHY PALAEOCLIMATOLOGY PALAEOECOLOGY LA English DT Review DE Cretaceous greenhouse; Eustasy; Relative sea-level change; Aquifer-eustasy; Sequence stratigraphy; Orbital cycles ID ORBITAL TIME-SCALE; DYNAMIC TOPOGRAPHY; ICE SHEETS; SEQUENCE STRATIGRAPHY; OCEAN CIRCULATION; MANTLE CONVECTION; ATLANTIC-OCEAN; CLIMATE-CHANGE; RISE; EUSTASY AB This review provides a synopsis of ongoing research and our understanding of the fundamentals of sea-level change today and in the geologic record, especially as illustrated by conditions and processes during the Cretaceous greenhouse climate episode. We give an overview of the state of the art of our understanding on eustatic (global) versus relative (regional) sea level, as well as long-term versus short-term fluctuations and their drivers. In the context of the focus of UNESCO-IUGS/IGCP project 609 on Cretaceous eustatic, short-term sea-level and climate changes, we evaluate the possible evidence for glacio-eustasy versus alternative or additional mechanisms for continental water storage and release for the Cretaceous greenhouse and hothouse phases during which the presence of larger continental ice shields is considered unlikely. Increasing evidence in the literature suggests a correlation between long-period orbital cycles and depositional cycles that reflect sea-level fluctuations, implying a globally synchronized forcing of (eustatic) sea level. Fourth-order depositional sequences seem to be related to a similar to 405 ka periodicity, which most likely represents long-period orbital eccentricity control on sea level and depositional cycles. Third-order cyclidty, expressed as time-synchronous sea level falls of similar to 20 to 110 m on similar to 0.5 to 3.0 Ma timescales in the Cretaceous, are increasingly recognized as connected to climate cycles triggered by long-term astronomical cycles that have periodicity ranging from similar to 1.0 to 2.4 Ma. Future perspectives of research on greenhouse sea-level changes comprise a high-precision time-scale for sequence stratigraphy and eustatic sea-level changes and high-resolution marine to non-marine stratigraphic correlation. (C) 2015 Published by Elsevier B.V. C1 [Sames, B.; Wagreich, M.; Wolfgring, E.] Univ Vienna, Dept Geodynam & Sedimentol, Geozentrum, A-1090 Vienna, Austria. [Sames, B.] Sam Noble Oklahoma Museum Nat Hist, Norman, OK 73072 USA. [Wendler, J. E.; Wendler, I.] Univ Bremen, Dept Geosci, D-28334 Bremen, Germany. [Haq, B. U.] Smithsonian Inst, Washington, DC 20560 USA. [Haq, B. U.] Sorbonne Pierre & Marie Curie Univ, Paris, France. [Conrad, C. P.] Univ Hawaii Manoa, Dept Geol & Geophys, Sch Ocean & Earth Sci & Technol, Honolulu, HI 96822 USA. [Melinte-Dobrinescu, M. C.] Natl Inst Marine Geol & Geoecol GeoEcoMar, Bucharest 024053, Romania. [Hu, X.] Nanjing Univ, Sch Earth Sci & Engn, Nanjing 210093, Jiangsu, Peoples R China. [Yilmaz, I. O.] Middle E Tech Univ, Dept Geol Engn, TR-06531 Ankara, Turkey. [Yilmaz, I. O.] Univ Texas Austin, Dept Geol Sci, Austin, TX 78712 USA. [Zorina, S. O.] Kazan Fed Univ, Dept Paleontol & Stratig, Kazan 420008, Russia. RP Sames, B (reprint author), Univ Vienna, Dept Geodynam & Sedimentol, Geozentrum, Althanstr 14, A-1090 Vienna, Austria. EM benjamin.sames@univie.ac.at RI Zorina, Svetlana/L-5404-2013 OI Zorina, Svetlana/0000-0001-6315-1672 FU OAW (Austrian Academy of Sciences) IGCP grant; Austrian Science Fund (FWF) [P 27687-N29, P 24044-N24]; NSF [EAR-1151241]; EARTHTIME-EU; Russian Government Program of Competitive Growth of Kazan Federal University; [609] FX This paper is a contribution to UNESCO-IUGS IGCP project 609 "Climate-environmental deteriorations during greenhouse phases: Causes and consequences of short-term Cretaceous sea-level changes" (MW, XH, IOY, SOZ, BS). It benefited from an OAW (Austrian Academy of Sciences) IGCP grant to Michael Wagreich (MW, BS), from Austrian Science Fund (FWF) projects P 27687-N29 (BS) and P 24044-N24 (MW, EW), NSF grant EAR-1151241 (CPC), EARTHTIME-EU workshop funding, and the Russian Government Program of Competitive Growth of Kazan Federal University (SOZ). NR 175 TC 10 Z9 11 U1 9 U2 32 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0031-0182 EI 1872-616X J9 PALAEOGEOGR PALAEOCL JI Paleogeogr. Paleoclimatol. Paleoecol. PD JAN 1 PY 2016 VL 441 SI SI BP 393 EP 411 DI 10.1016/j.palaeo.2015.10.045 PN 3 PG 19 WC Geography, Physical; Geosciences, Multidisciplinary; Paleontology SC Physical Geography; Geology; Paleontology GA CZ5AF UT WOS:000367113800002 ER PT J AU Lee, JSH Jaafar, Z Tan, AKJ Carrasco, LR Ewing, JJ Bickford, DP Webb, EL Koh, LP AF Lee, Janice Ser Huay Jaafar, Zeehan Tan, Alan Khee Jin Carrasco, Luis R. Ewing, J. Jackson Bickford, David P. Webb, Edward L. Koh, Lian Pin TI Toward clearer skies: Challenges in regulating transboundary haze in Southeast Asia SO ENVIRONMENTAL SCIENCE & POLICY LA English DT Article DE Environmental law; Deforestation; Fires; Governance; Industrial plantations; Indonesia ID PEAT SWAMP FORESTS; FIRE EMISSIONS; ENVIRONMENTAL GOVERNANCE; INDONESIA; POLLUTION; IMPACTS; BIODIVERSITY; LAND; DEFORESTATION; CLIMATE AB Addressing transboundary environmental problems, such as pollution, and climate change, hinge on strategies that often require both mandatory and voluntary participation of affected nations. Using an unprecedented approach, the Singapore government recently passed a Transboundary Haze Pollution Act (THPA) that financially penalizes companies for smoke-haze affecting the city-state but originating from activities outside her political boundaries. This Act may set a precedent for future actions against proximate actors of environmental degradation but is fraught with substantial challenges in implementation. In attempting to hold agri-business companies accountable, the THPA must present indisputable evidence of fire burning activities and positively identify the initiator of these fires. We further argue that small amendments to the THPA, and other similar laws, may result in environmental co-benefits related to carbon emissions, ecosystem services and biodiversity preservation. (C) 2015 Elsevier Ltd. All rights reserved. C1 [Lee, Janice Ser Huay] Princeton Univ, Woodrow Wilson Sch, Princeton, NJ 08544 USA. [Lee, Janice Ser Huay] Princeton Univ, Dept Ecol & Evolutionary Biol, Princeton, NJ 08544 USA. [Jaafar, Zeehan; Carrasco, Luis R.; Bickford, David P.; Webb, Edward L.] Natl Univ Singapore, Dept Biol Sci, Singapore 117548, Singapore. [Jaafar, Zeehan] Smithsonian Inst, Natl Museum Nat Hist, Dept Vertebrate Zool, Washington, DC 20560 USA. [Tan, Alan Khee Jin] Natl Univ Singapore, Fac Law, Singapore 117548, Singapore. [Ewing, J. Jackson] Nanyang Technol Univ, Ctr Nontradit Secur Studies, S Rajaratnam Sch Int Studies, Singapore 639798, Singapore. [Koh, Lian Pin] Univ Adelaide, Inst Environm, Adelaide, SA 5005, Australia. [Koh, Lian Pin] Univ Adelaide, Sch Earth & Environm Sci, Adelaide, SA 5005, Australia. RP Lee, JSH (reprint author), Princeton Univ, Woodrow Wilson Sch, Princeton, NJ 08544 USA. EM janice.jlsh@gmail.com; jaafarz@si.edu RI Koh, Lian Pin/A-5794-2010 OI Koh, Lian Pin/0000-0001-8152-3871 FU Swiss National Science Foundation; National University of Singapore; Smithsonian Institute; Australian Research Council FX We thank the National Environment Agency of Singapore and the Singapore Institute of International Affairs for hosting stakeholder meetings and workshops on the Southeast Asian haze. J.S.H.L. is funded by the Swiss National Science Foundation. Z.J. is funded by the National University of Singapore and the Smithsonian Institute. L.P.K. is supported by the Australian Research Council. NR 88 TC 8 Z9 8 U1 18 U2 62 PU ELSEVIER SCI LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, OXON, ENGLAND SN 1462-9011 EI 1873-6416 J9 ENVIRON SCI POLICY JI Environ. Sci. Policy PD JAN PY 2016 VL 55 BP 87 EP 95 DI 10.1016/j.envsci.2015.09.008 PN 1 PG 9 WC Environmental Sciences SC Environmental Sciences & Ecology GA CZ0DL UT WOS:000366775200009 ER PT J AU Capper, A Erickson, AA Ritson-Williams, R Becerro, MA Arthur, KA Paul, VJ AF Capper, Angela Erickson, Amy A. Ritson-Williams, Raphael Becerro, Mikel A. Arthur, Karen A. Paul, Valerie J. TI Palatability and chemical defences of benthic cyanobacteria to a suite of herbivores SO JOURNAL OF EXPERIMENTAL MARINE BIOLOGY AND ECOLOGY LA English DT Article DE Lyngbya; Secondary metabolites; Feeding deterrents; Generalist and specialist herbivorous grazers; Opisthobranch molluscs ID TROPICAL MARINE CYANOBACTERIA; LYNGBYA-MAJUSCULA GOMONT; SECONDARY METABOLITES; STYLOCHEILUS-LONGICAUDA; MORETON BAY; SEA HARES; OPISTHOBRANCH MOLLUSK; FEEDING PREFERENCE; GLOBAL EXPANSION; CLIMATE-CHANGE AB Nuisance blooms of toxic cyanobacteria are a common occurrence in many tropical and subtropical locations. Benthic marine cyanobacteria of the genera Lyngbya, Okeania, and Moorea are frequently observed in both Florida and throughout the Caribbean, sometimes forming large mats, and are prolific producers of bioactive secondary metabolites that often act as feeding deterrents to generalist herbivores. Little is known regarding the ecological roles of the secondary metabolite chemistry and the palatability of benthic cyanobacteria to grazers. This study examines the palatability of benthic cyanobacterial species from Florida (IRL1, IRL2, IRL3 and Okeania erythroflocculosa) and Belize (BEL1 BEL2) to a range of macro- and mesograzers in Florida and Belize. Pair-wise feeding assays using artificial diets of Gracilaria tikvahiae or fish food coated with cyanobacterial extracts and a control were used to determine palatability of extracts to Floridian and Belizean generalist grazers. The extracts of IRL1, IRL2, IRL3 and O. erythroflocculosa from Florida did not deter feeding by invertebrate grazers. Reef fish, however, were deterred by the non-polar extracts of IRL1, IRL3 and O. etythroflocculosa. Stylocheilus striatus was stimulated to feed on IRL2 extracts and non-polar extracts from IRL3. Non-polar extracts of BEL1 stimulated feeding in S. striatus; however, no significant difference was observed between BEL2 extracts and the control. Most generalist invertebrate grazers, sympatric and non-sympatric, appear indifferent to cyanobacteria extracts whilst reef fish are more likely to be deterred by cyanobacterial extracts, which may affect species interaction within communities with fluctuating or dominating benthic cyanobacterial blooms. (C) 2015 Elsevier B.V. All rights reserved. C1 [Capper, Angela] James Cook Univ, Coll Marine & Environm Sci, Townsville, Qld 4811, Australia. [Capper, Angela; Erickson, Amy A.; Ritson-Williams, Raphael; Becerro, Mikel A.; Arthur, Karen A.; Paul, Valerie J.] Smithsonian Marine Stn, Ft Pierce, FL 34949 USA. [Erickson, Amy A.] Louisiana State Univ, Dept Biol Sci, Shreveport, LA 71115 USA. [Ritson-Williams, Raphael] Univ Hawaii, Dept Biol, Honolulu, HI 96822 USA. [Becerro, Mikel A.] CSIC, IPNA, Nat Prod & Agrobiol Inst, Tenerife 38206, Canary Islands, Spain. [Arthur, Karen A.] Australian Natl Univ, Sch Res Biol, Canberra, ACT 0200, Australia. RP Capper, A (reprint author), James Cook Univ, Coll Marine & Environm Sci, Townsville, Qld 4811, Australia. EM angela.capper@jcu.edu.au; aerickso@lsus.edu; rrw33@hawaii.edu; mikel.becerro@csic.es; karen.arthur@anu.edu.au; Paul@si.edu OI Capper, Angela/0000-0002-4922-0253 FU Smithsonian Marine Station Fellowship; U.S. Department of Commerce (DoC, NOAA, ECOHAB programme), through UNCCH [NA05 NOS 4781194]; CCRE programme [980] FX This research was funded by a Smithsonian Marine Station Fellowship to A.C. and Grant Number NA05 NOS 4781194 from the U.S. Department of Commerce (DoC, NOAA, ECOHAB programme), through UNCCH. The findings, opinions and recommendations expressed in this publication are those of the authors and not necessarily those of the DoC. We thank Cliff Ross and Sherry Reed, Smithsonian Marine Station; and Ken Banks, Broward County Environment Protection Department, Fort Lauderdale, for their assistance with collections of cyanobacteria. We thank Dennis Hanisak at Harbor Branch Oceanographic Institute for supply of Gracilaria tikvahiae; Paula Mikkelson, at Paleontological Research Institution, Ithaca, NY for verifying the cephalaspidean used in the Belizean palatability assay as an undescribed species; Darryl Felder, University of Louisiana at Lafayette for identification of the crab species used in the assays. This is contribution 1009 of the Smithsonian Marine Station at Fort Pierce and contribution 980 of the CCRE programme. [SS] NR 57 TC 1 Z9 1 U1 8 U2 29 PU ELSEVIER SCIENCE BV PI AMSTERDAM PA PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS SN 0022-0981 EI 1879-1697 J9 J EXP MAR BIOL ECOL JI J. Exp. Mar. Biol. Ecol. PD JAN PY 2016 VL 474 BP 100 EP 108 DI 10.1016/j.jembe.2015.09.008 PG 9 WC Ecology; Marine & Freshwater Biology SC Environmental Sciences & Ecology; Marine & Freshwater Biology GA CZ0AU UT WOS:000366768300014 ER PT J AU Wohner, PJN Cooper, RJ Greenberg, RS Schweitzer, SH AF Wohner, Patti J. Newell Cooper, Robert J. Greenberg, Russell S. Schweitzer, Sara H. TI Weather affects diet composition of rusty blackbirds wintering in suburban landscapes SO JOURNAL OF WILDLIFE MANAGEMENT LA English DT Article DE acorn; diet isotope; Euphagus carolinus; invertebrates; Oligochaeta; pecan; rusty blackbird; SIAR; southeastern United States; wintering ID STABLE-ISOTOPES; MODEL SELECTION; UNITED-STATES; NITROGEN; ECOLOGY; BLOOD; FRACTIONATION; EARTHWORMS; SONGBIRDS; DECLINES AB The rusty blackbird (Euphagus carolinus) is a species of conservation concern throughout its range and the cause of the species' population decline is unknown. We studied diet composition of rusty blackbirds with stable isotope mixing models in suburban landscapes in the southeastern United States. We captured blackbirds in Georgia and South Carolina from 2009 to 2012, and estimated proportions of earthworm, other animals, pecan, and acorn incorporated into individual diets. On the Piedmont Plateau, terrestrial and aquatic earthworms constituted the largest proportion incorporated into the diet (39%+/- 2.9; mean +/- SD by site and year) and animals other than earthworms (mostly larval invertebrates Odonata and Diptera) constituted 27%+/- 12.9. In contrast, on the Coastal Plain, which featured milder winters than the Piedmont, earthworms constituted a lower proportion (19%+/- 1.2) of incorporated food items and animals other than earthworms comprised 62%+/- 3.3% of the diet. Increased incorporation of earthworms in the diet was related to increased upcoming precipitation and daily maximum temperature. Rusty blackbirds incorporated more tree mast into their diet on the Piedmont Plateau than the Coastal Plain. Increased incorporation of tree mast was related to advancing cold temperature. Mast, including crushed pecans (Carya illinoenensis) and pre-opened small-seeded red oak (Quercus spp.) acorns, is a high-lipid dietary component of blackbirds wintering in colder climates, and is incorporated prior to extreme cold weather. Therefore, planting mast trees, especially lipid-rich pecan, could be used to augment resources in known rusty blackbird wintering hotspots. Maintaining shallowly flooded wetlands with a fluctuating water regime and residential lawns with abundant red oak (Quercus spp.) leaf litter would promote acorn and invertebrate resources including earthworms. (c) 2015 The Wildlife Society. C1 [Wohner, Patti J. Newell; Cooper, Robert J.] Univ Georgia, Warnell Sch Forestry & Nat Resources, Athens, GA 30602 USA. [Greenberg, Russell S.] Smithsonian Migratory Bird Ctr, Washington, DC 20013 USA. [Schweitzer, Sara H.] North Carolina Wildlife Resources Commiss, Wildlife Div Program, New Bern, NC 28562 USA. RP Wohner, PJN (reprint author), Univ Georgia, Warnell Sch Forestry & Nat Resources, Athens, GA 30602 USA. EM pjwohner@gmail.com FU USFWS; Georgia Ornithological Society; Carolina Bird Club; Smithsonian Institution; University of Georgia; Natural Sciences and Engineering Research Council of Canada (NSERC) FX We would like to dedicate this paper to the memory of Russ Greenberg who passed away on 24 October 2013. Russ brought the decline of the rusty blackbird to the attention of ornithologists and initiated and organized research efforts throughout the bird's range. We thank C. A. France and T. R. Maddox for help with isotope analysis and preparation. A special thanks to field assistants, S. Hribal, D. Heath, D. Narango, J. Wilcox, and J. Bruce. Other supporters were P. Serridge, P. Doherty, Magnolia Plantation and Gardens, Conestee Foundation, Sandy Creek Nature Center, Greer Fire Department, Lake Cunningham County Park, and numerous private landowners and volunteers who allowed use of their yards and pecan groves for bird capture. Financial support was provided by the USFWS, Georgia Ornithological Society, Carolina Bird Club, Smithsonian Institution, University of Georgia, and Natural Sciences and Engineering Research Council of Canada (NSERC). NR 62 TC 0 Z9 0 U1 9 U2 32 PU WILEY-BLACKWELL PI HOBOKEN PA 111 RIVER ST, HOBOKEN 07030-5774, NJ USA SN 0022-541X EI 1937-2817 J9 J WILDLIFE MANAGE JI J. Wildl. Manage. PD JAN PY 2016 VL 80 IS 1 BP 91 EP 100 DI 10.1002/jwmg.984 PG 10 WC Ecology; Zoology SC Environmental Sciences & Ecology; Zoology GA CY6OC UT WOS:000366527700010 ER PT J AU He, K Hu, NQ Chen, X Li, JT Jiang, XL AF He, K. Hu, N-Q Chen, X. Li, J-T Jiang, X-L TI Interglacial refugia preserved high genetic diversity of the Chinese mole shrew in the mountains of southwest China SO HEREDITY LA English DT Article ID SEQUENCE; PHYLOGEOGRAPHY; PHYLOGENETICS; CONSEQUENCES; POLYMORPHISM; QUATERNARY; EVOLUTION; ACCURACY; SOFTWARE; MAMMALIA AB The mountains of southwest China (MSC) harbor extremely high species diversity; however, the mechanism behind this diversity is unknown. We investigated to what degree the topography and climate change shaped the genetic diversity and diversification in these mountains, and we also sought to identify the locations of microrefugia areas in these mountains. For these purposes, we sampled extensively to estimate the intraspecific phylogenetic pattern of the Chinese mole shrew (Anourosorex squamipes) in southwest China throughout its range of distribution. Two mitochondrial genes, namely, cytochrome b (CYT B) and NADH dehydrogenase subunit 2 (ND2), from 383 archived specimens from 43 localities were determined for phylogeographic and demographic analyses. We used the continuous-diffusion phylogeographic model, extensive Bayesian skyline plot species distribution modeling (SDM) and approximate Bayesian computation (ABC) to explore the changes in population size and distribution through time of the species. Two phylogenetic clades were identified, and significantly higher genetic diversity was preserved in the southern subregion of the mountains. The results of the SDM, continuous-diffusion phylogeographic model, extensive Bayesian skyline plot and ABC analyses were congruent and supported that the Last Interglacial Maximum (LIG) was an unfavorable period for the mole shrews because of a high degree of seasonality; A. squamipes survived in isolated interglacial refugia mainly located in the southern subregion during the LIG and rapidly expanded during the last glacial period. These results furnished the first evidence for major Pleistocene interglacial refugia and a latitudinal effect in southwest China, and the results shedding light on the higher level of species richness in the southern subregion. C1 [He, K.; Hu, N-Q; Jiang, X-L] Chinese Acad Sci, Kunming Inst Zool, State Key Lab Genet Resources & Evolut, Kunming 650223, Yunnan, Peoples R China. [He, K.] Smithsonian Inst, Natl Museum Nat Hist, Washington, DC 20560 USA. [Hu, N-Q] Univ Chinese Acad Sci, Beijing, Peoples R China. [Chen, X.] CUNY, CUNY Coll Staten Isl, Dept Biol, New York, NY USA. [Chen, X.] Dartmouth Coll, Dept Biol Sci, Hanover, NH 03755 USA. [Li, J-T] Chinese Acad Sci, Chengdu Inst Biol, Chengdu, Peoples R China. RP Jiang, XL (reprint author), Chinese Acad Sci, Kunming Inst Zool, State Key Lab Genet Resources & Evolut, 32 Jiaochangdonglu, Kunming 650223, Yunnan, Peoples R China. EM Jiangxl@mail.kiz.ac.cn OI He, Kai/0000-0002-6234-2589 FU Key Research Program of the Chinese Academy of Sciences [KJZD-EW-L07]; National Natural Science Foundation of China [31301869] FX We appreciate the constructive comments and suggestions from the two anonymous reviewers. We thank Dr Shaoying Liu, Dr Shunde Chen and Dr Qingyong Ni for providing us samples from Sichuan. We also thank Dr Filip Bielejec for providing us the newest version of SPREAD, Dr Philippe Lemey and Dr Arley Camargo for providing code for constructing dispersal rate through time plot and Dr Youbin Sun and Mr Peter Shum for their very useful discussions. We are grateful to Dr Shouli Yuan for many constructive discussions. This paper is modified from Chapter 6 of the PhD thesis of KH. The study is supported by the Key Research Program of the Chinese Academy of Sciences (KJZD-EW-L07) and the National Natural Science Foundation of China (31301869). NR 41 TC 1 Z9 1 U1 8 U2 29 PU NATURE PUBLISHING GROUP PI LONDON PA MACMILLAN BUILDING, 4 CRINAN ST, LONDON N1 9XW, ENGLAND SN 0018-067X EI 1365-2540 J9 HEREDITY JI Heredity PD JAN PY 2016 VL 116 IS 1 BP 23 EP 32 DI 10.1038/hdy.2015.62 PG 10 WC Ecology; Evolutionary Biology; Genetics & Heredity SC Environmental Sciences & Ecology; Evolutionary Biology; Genetics & Heredity GA CY3AR UT WOS:000366280700003 PM 26286667 ER PT J AU Brooke, JSA Bernath, PF Western, CM Sneden, C Afsar, M Li, G Gordon, IE AF Brooke, James S. A. Bernath, Peter F. Western, Colin M. Sneden, Christopher Afsar, Melike Li, Gang Gordon, Iouli E. TI Line strengths of rovibrational and rotational transitions in the X-2 Pi ground state of OH SO JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER LA English DT Article DE OH hydroxyl radical; Line intensities; Einstein A values; Dipole moment function; Meinel system; Line lists ID DIPOLE-MOMENT FUNCTION; B-2-SIGMA(+)-X-2-SIGMA(+) VIOLET SYSTEMS; SIZE-EXTENSIVE MODIFICATION; VIBRATIONALLY EXCITED OH; BEAM ELECTRIC RESONANCE; SOLAR OXYGEN ABUNDANCE; METAL-POOR STARS; MICROWAVE-SPECTRUM; DIATOMIC-MOLECULES; A(2)PI-X-2-SIGMA(+) RED AB A new line list including positions and absolute transition strengths (in the form of Einstein A values and oscillator strengths) has been produced for the OH ground X-2 Pi state rovibrational (Meinel system) and pure rotational transitions. All possible transitions are included with v' and v '' up to 13, and J up to between 9.5 and 59.5, depending on the band. An updated fit to determine molecular constants has been performed, which includes some new rotational data and a simultaneous fitting of all molecular constants. The absolute transition strengths are based on a new dipole moment function, which is a combination of two high level ab initio calculations. The calculations show good agreement with an experimental v = 1 lifetime, experimental mu(v) values, and Delta v =2 line intensity ratios from an observed spectrum. To achieve this good agreement, an alteration in the method of converting matrix elements from Hund's case (b) to (a) was made. Partitions sums have been calculated using the new energy levels, for the temperature range 5-6000 K, which extends the previously available (in HITRAN) 70-3000 K range. The resulting absolute transition strengths have been used to calculate 0 abundances in the Sun, Arcturus, and two red giants in the Galactic open and globular clusters M67 and M71. Literature data based mainly on [O I] lines are available for the Sun and Arcturus, and excellent agreement is found. (C) 2015 Elsevier Ltd. All rights reserved. C1 [Brooke, James S. A.; Bernath, Peter F.] Univ York, Dept Chem, York YO10 5DD, N Yorkshire, England. [Bernath, Peter F.] Old Dominion Univ, Dept Chem & Biochem, Norfolk, VA 23529 USA. [Western, Colin M.] Univ Bristol, Sch Chem, Bristol BS8 1TS, Avon, England. [Sneden, Christopher] Univ Texas Austin, Dept Astron, Austin, TX 78712 USA. [Afsar, Melike] Ege Univ, Dept Astron & Space Sci, TR-35100 Izmir, Turkey. [Li, Gang; Gordon, Iouli E.] Harvard Smithsonian Ctr Astrophys, Atom & Mol Phys Div, Cambridge, MA 02138 USA. RP Brooke, JSA (reprint author), Univ Leeds, Sch Chem, Leeds LS2 9JT, W Yorkshire, England. EM jsabrooke@gmail.com RI Bernath, Peter/B-6567-2012 OI Bernath, Peter/0000-0002-1255-396X FU Department of Chemistry (University of York); NASA Origins of Solar Systems program; Turkish Scientific and Technological Research Council (TUBITAK) [1121929]; Research Project Grant from the Leverhulme Trust FX Support for this work was provided by a Research Project Grant from the Leverhulme Trust and the Department of Chemistry (University of York) studentship. Some support was also provided by the NASA Origins of Solar Systems program. M.A. was supported by the Turkish Scientific and Technological Research Council (TUBITAK, Project 1121929). We are grateful to Gail Zasowski for assistance with the APOGEE database. Thanks also go to Jeremy J. Harrison for helpful discussions about the transformation equation. NR 106 TC 5 Z9 5 U1 5 U2 8 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0022-4073 EI 1879-1352 J9 J QUANT SPECTROSC RA JI J. Quant. Spectrosc. Radiat. Transf. PD JAN PY 2016 VL 168 BP 142 EP 157 DI 10.1016/j.jqsrt.2015.07.021 PG 16 WC Optics; Spectroscopy SC Optics; Spectroscopy GA CX9EE UT WOS:000366007000012 ER PT J AU Wilzewski, JS Gordon, IE Kochanov, RV Hill, C Rothman, LS AF Wilzewski, Jonas S. Gordon, Iouli E. Kochanov, Roman V. Hill, Christian Rothman, Laurence S. TI H-2, He, and CO2 line-broadening coefficients, pressure shifts and temperature-dependence exponents for the HITRAN database. Part 1: SO2, NH3, HF, HCl, OCS and C2H2 SO JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER LA English DT Article DE HITRAN database; Pressure broadening; Pressure shift; Temperature-dependence; Planetary atmospheres ID DIODE-LASER SPECTROSCOPY; PLANETARY ATMOSPHERIC TEMPERATURES; MOLECULAR QUADRUPOLE-MOMENTS; CROSS-RELAXATION RATES; FOREIGN-GAS PRESSURE; 1ST OVERTONE BAND; NU(4) BAND; FUNDAMENTAL-BAND; HALF-WIDTHS; H-2-BROADENING COEFFICIENTS AB To increase the potential for use of the HITRAN database in astronomy, experimental and theoretical line-broadening coefficients, line shifts and temperature-dependence exponents of molecules of planetary interest broadened by H-2, He, and CO2 have been assembled from available peer-reviewed sources. The collected data were used to create semi-empirical models so that every HITRAN line of the studied molecules has corresponding parameters. Since H-2 and He are major constituents in the atmospheres of gas giants, and CO2 predominates in atmospheres of some rocky planets with volcanic activity, these spectroscopic data are important for remote sensing studies of planetary atmospheres. In this paper we make the first step in assembling complete sets of these parameters, thereby creating datasets for SO2, NH3, HF, HCl, OCS and C2H2. Published by Elsevier Ltd. C1 [Wilzewski, Jonas S.; Gordon, Iouli E.; Kochanov, Roman V.; Hill, Christian; Rothman, Laurence S.] Harvard Smithsonian Ctr Astrophys, Atom & Mol Phys Div, Cambridge, MA 02138 USA. [Wilzewski, Jonas S.] Tech Univ Dresden, Dept Phys, D-01062 Dresden, Germany. [Wilzewski, Jonas S.] Harvard Astron Dept, Cambridge, MA 02138 USA. [Kochanov, Roman V.] Tomsk State Univ, Lab Quantum Mech Mol & Radiat Proc, Tomsk 634050, Russia. [Hill, Christian] UCL, London WC1E 6BT, England. RP Gordon, IE (reprint author), Harvard Smithsonian Ctr Astrophys, Atom & Mol Phys Div, 60 Garden St, Cambridge, MA 02138 USA. EM IGordon@cfa.harvard.edu RI Wilzewski, Jonas/M-7985-2016; Kochanov, Roman/E-8679-2014; OI Wilzewski, Jonas/0000-0002-1392-2966; Kochanov, Roman/0000-0001-5165-5099; Rothman, Laurence/0000-0002-3837-4847; Gordon, Iouli/0000-0003-4763-2841 FU NASA Planetary Atmospheres Grant [NNX13AI59G]; German-American Fulbright Commission FX Support from NASA Planetary Atmospheres Grant NNX13AI59G and the German-American Fulbright Commission is gratefully acknowledged. We are also indebted to L.R. Brown for providing unpublished computer programs and data files of OCS and NH3 that are currently being used by astronomers. We also thank F. Thibault for his advice on the generation of the C2H2 datasets. Further, we thank L.M. Eng and M.H. Soffel for supporting part of this project as Wilzewski's Bachelor's thesis. Many thanks to Mary Ann Smith (NASA) for providing data from Ref. [71]. We would like to thank P. Wcislo for his feedback in the development of HAPI and for reviewing the functions used in the calculation of the absorption coefficients in Fig. 1. Finally, we are thanks to Lorenzo Barrett for the help with uploading the new parameters into HITRANonline. NR 129 TC 5 Z9 5 U1 3 U2 16 PU PERGAMON-ELSEVIER SCIENCE LTD PI OXFORD PA THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND SN 0022-4073 EI 1879-1352 J9 J QUANT SPECTROSC RA JI J. Quant. Spectrosc. Radiat. Transf. PD JAN PY 2016 VL 168 BP 193 EP 206 DI 10.1016/j.jqsrt.2015.09.003 PG 14 WC Optics; Spectroscopy SC Optics; Spectroscopy GA CX9EE UT WOS:000366007000016 ER PT J AU Field, AR Testo, W Bostock, PD Holtum, JAM Waycott, M AF Field, Ashley R. Testo, Weston Bostock, Peter D. Holtum, Joseph A. M. Waycott, Michelle TI Molecular phylogenetics and the morphology of the Lycopodiaceae subfamily Huperzioideae supports three genera: Huperzia, Phlegmariurus and Phylloglossum SO MOLECULAR PHYLOGENETICS AND EVOLUTION LA English DT Article DE Lycopodiaceae; Phlegmariurus; Phylloglossum; Huperzia; Tassel-fern; Club-moss ID NEOTROPICAL LYCOPODIACEAE; AUSTRALASIAN HUPERZIA; RBCL SEQUENCES; SENSU-LATO; GAMETOPHYTE; CLASSIFICATION; COMBINATIONS; DRUMMONDII; FERNS; DIVERSIFICATION AB The generic classification of huperzioid Lycopodiaceae was tested using Bayesian inference and Maximum likelihood phylogenetic analyses of DNA sequences from four chloroplast loci for 119 taxa and optimisation of 29 morphological characteristics onto the phylogeny. Consistent with previous studies, the subfamilies Lycopodioideae and Huperzioideae are monophyletic and diagnosable by synapomorphies that correlate with differences in their life-histories. Within the Huperzioideae, the monophyly of the widely adopted genus Huperzia (excl. Phylloglossum) is poorly supported. Three clades of huperzioid Lycopodiaceae were recovered in all analyses of molecular data: Phylloglossum drummondii, Huperzia sensu stricto and Phlegmariurus sensu la to. These clades are strongly supported by morphological characters, including differences in spores, gametophytes, sporophyte macro-morphology, as well as growth habit and life-histories. Our findings indicate that either a one-genus (Huperzia s.l.) or a three-genus (Phylloglossum, Huperzia s.s. and Phlegrnariurus s.l.) classification of huperzioid Lycopods are equally supported by molecular evidence, but a two-genus system (Huperzia s.l. + Phylloglossum) is not. We recommend recognising three genera in the huperzioid Lycopodiaceae, as this classification best reflects evolutionary, ecological, and morphological divergence within the lineage. Crown Copyright (C) 2015 Published by Elsevier Inc. All rights reserved. C1 [Field, Ashley R.] Australian Trop Herbarium, Cairns, Qld 4878, Australia. [Field, Ashley R.; Bostock, Peter D.] Queensland Herbarium, Dept Sci Informat Technol & Innovat, Toowong, Qld 4066, Australia. [Field, Ashley R.; Holtum, Joseph A. M.; Waycott, Michelle] James Cook Univ, Coll Marine & Environm Sci, Douglas, Qld 4811, Australia. [Testo, Weston] Univ Vermont, Dept Plant Biol, Burlington, VT 05405 USA. [Holtum, Joseph A. M.] Smithsonian Trop Res Inst, Balboa, Anton, Panama. [Waycott, Michelle] Univ Adelaide, Sch Earth & Environm Sci, Adelaide, SA 5001, Australia. [Waycott, Michelle] State Herbarium South Australia, Adelaide, SA 5001, Australia. RP Field, AR (reprint author), Australian Trop Herbarium, POB 6811, Cairns, Qld 4878, Australia. EM ashley.field@jcu.edu.au FU Queensland Government Growing the Smart State PhD Funding Program; James Cook University School of Marine and Tropical Biology teaching stipend; Australian Biological Resource Study National Taxonomy Research Grant FX This research was supported by the Queensland Government Growing the Smart State PhD Funding Program, a James Cook University School of Marine and Tropical Biology teaching stipend and an Australian Biological Resource Study National Taxonomy Research Grant. Thank you to Holly Field and the Field, Kupke, Rawlins and Wilkinson families for assisting to maintain the living lycopod collection and to all field collectors and photographers of samples used in this study. NR 91 TC 5 Z9 5 U1 5 U2 25 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1055-7903 EI 1095-9513 J9 MOL PHYLOGENET EVOL JI Mol. Phylogenet. Evol. PD JAN PY 2016 VL 94 BP 635 EP 657 DI 10.1016/j.ympev.2015.09.024 PN B PG 23 WC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity SC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity GA CY5JG UT WOS:000366443300016 PM 26493224 ER PT J AU Liu, J May-Collado, LJ Pekar, S Agnarsson, I AF Liu, Jie May-Collado, Laura J. Pekar, Stano Agnarsson, Ingi TI A revised and dated phylogeny of cobweb spiders (Araneae, Araneoidea, Theridiidae): A predatory Cretaceous lineage diversifying in the era of the ants (Hymenoptera, Formicidae) SO MOLECULAR PHYLOGENETICS AND EVOLUTION LA English DT Article DE Cobweb spiders; Ants; Abundance; Formicidae; Ant hypothesis; Predator and prey; Molecular dating; Fossils ID ORB-WEAVING SPIDERS; BLACK-WIDOW SPIDER; TETRAGNATHA-LABORIOSA ARANEAE; IMPORTED FIRE ANT; SOCIAL SPIDER; PREY CAPTURE; KLEPTOPARASITIC SPIDER; SEXUAL CANNIBALISM; ANELOSIMUS-EXIMIUS; SPECIES RICHNESS AB Cobweb spiders (Theridiidae) are highly diverse from the perspective of species richness, morphological diversity, variety of web architecture, and behavioral repertoires. The family includes over 50% of social spiders, a behavioral rarity among the order, and members of the family are furthermore the subject of research on venom, silk biomechanics, kleptoparasitism and web building, among other traits. Theridiidae is one of the most abundant groups of spiders, and thus key insect predators in many different ecosystems and is among relatively few spider families that show high degree of myrmecophagy. Modern comparative studies on all these fronts are best buttressed on a phylogenetic foundation. Our goal here is to offer a revised, dated, phylogenetic hypothesis for the family by summarizing previously published data from multiple molecular and morphological studies through data-mining, and adding novel data from several genera. We also test the hypothesis that the origin and diversification of cobweb spiders coincides with that of ants on which many species specialize as prey. The new phylogeny is largely congruent with prior studies and current taxonomy and should provide a useful tool for theridiid classification and for comparative analyses. Nevertheless, we also highlight the limitations of currently available data the state of the art in Theridiidae phylogenetics offering weak support for most of the deeper nodes in the phylogeny. Thus the need is clear for modern phylogenomic approaches to obtain a more solid understanding, especially of relationships among subfamilies. We recover the monophyly of currently recognized theridiid subfamilies with the exception of some enigmatic 'pholcommatines' (Styposis, Phoroncidia) and putative 'hadrotarsines' (Audifia, Tekellina) whose placement is uncertain in our analyses. Theridiidae dates back some 100 mya to the Cretaceous, a period of diversification in flowering plants and many groups of insects, including ants. The origin of cobweb spiders, and hence the cobweb-a speciallized trap for pedestrian prey-coincides with a major diversification shift in ants. The family becomes abundant in fossil record 50-40 mya as ants also diversify and reach dominance and contemporary patterns of abundances of theridiids and ants show the same trends, with increasing relative abundance towards the equator and at lower altitudes. We find that among orbiculariae, lineages that specialize on ant prey are non-randomly clustered within Theridiidae. Given these findings we hypothesize that the origin of the gumfoot web was a stepping stone that facilitated the capture of ants and resulted in specialized myrmecophagy in a number of 'basal' theridiids. We also document a subsequent loss in myrmecophagy, and associated increase in speciation rates, as 'recent' theridiid groups evolve diverse web forms and many return to the capture of aerial prey. (C) 2015 Elsevier Inc. All rights reserved. C1 [Liu, Jie; May-Collado, Laura J.; Agnarsson, Ingi] Univ Vermont, Dept Biol, Burlington, VT 05405 USA. [Liu, Jie] Hubei Univ, Hubei Collaborat Innovat Ctr Green Transformat Bi, Ctr Behav Ecol & Evolut, Coll Life Sci, Wuhan 430062, Hubei, Peoples R China. [Pekar, Stano] Masaryk Univ, Fac Sci, Dept Bot & Zool, CS-61137 Brno, Czech Republic. [Agnarsson, Ingi] Smithsonian Inst, Dept Entomol, Natl Museum Nat Hist, Washington, DC 20560 USA. RP Agnarsson, I (reprint author), Univ Vermont, Dept Biol, Burlington, VT 05405 USA. EM iagnarsson@gmail.com OI Pekar, Stano/0000-0002-0197-5040 FU UVM; NSF [DEB-349205-1050187-1050253]; Wuhan Youth Chenguang Programe of Science and Technology [2015070404010188]; [NSFC-31272268] FX We thank Niclas Fritzen, Paula Cushing, Michael Hohner and berg Wunderlich for sending us specimens. Giselle Veve assisted with laboratory work. Thanks to Miguel Arnedo and two anonymous reviewers for comments that helped improve the manuscript. Funding for this research comes, in part, from UVM and NSF DEB-349205-1050187-1050253 to IA and G. Binford. Additional support came from NSFC-31272268 and the Wuhan Youth Chenguang Programe of Science and Technology (2015070404010188) to J. Liu. NR 232 TC 4 Z9 4 U1 10 U2 44 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1055-7903 EI 1095-9513 J9 MOL PHYLOGENET EVOL JI Mol. Phylogenet. Evol. PD JAN PY 2016 VL 94 BP 658 EP 675 DI 10.1016/j.ympev.2015.09.023 PN B PG 18 WC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity SC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity GA CY5JG UT WOS:000366443300017 PM 26454029 ER PT J AU Hawkins, MTR Helgen, KM Maldonado, JE Rockwood, LL Tsuchiya, MTN Leonard, JA AF Hawkins, Melissa T. R. Helgen, Kristofer M. Maldonado, Jesus E. Rockwood, Larry L. Tsuchiya, Mirian T. N. Leonard, Jennifer A. TI Phylogeny, biogeography and systematic revision of plain long-nosed squirrels (genus Dremomys, Nannosciurinae) SO MOLECULAR PHYLOGENETICS AND EVOLUTION LA English DT Article DE Convergent evolution; Sciuridae; Biogeography; Sundaland; Morphology; Molecular phylogeny ID MOLECULAR PHYLOGENY; MITOCHONDRIAL-DNA; GEOGRAPHICAL VARIATION; SKULL MORPHOLOGY; ENDEMIC RODENTS; RAIN-FORESTS; SEQUENCES; NUCLEAR; EVOLUTIONARY; MYC AB The plain long-nosed squirrels, genus Dremomys, are high elevation species in East and Southeast Asia. Here we present a complete molecular phylogeny for the genus based on nuclear and mitochondrial DNA sequences. Concatenated mitochondrial and nuclear gene trees were constructed to determine the tree topology, and date the tree. All speciation events within the plain-long nosed squirrels (genus Dremomys) were ancient (dated to the Pliocene or Miocene), and averaged older than many speciation events in the related Sunda squirrels, genus Sundasciurus. Within the plain long-nosed squirrels, the most recent interspecific split occurred 2.9 million years ago, older than some splits within Sunda squirrels, which dated to the Pleistocene. Our results demonstrate that the plain long-nosed squirrels are not monophyletic. The single species with a distinct distribution, the Bornean mountain ground squirrel (Dremomys everetti), which is endemic to the high mountains of Borneo, is nested within the Sunda squirrels with high support. This species diverged from its sister taxa in the Sunda squirrels 6.62 million years ago, and other plain long-nosed squirrels over 11 million years ago. Our analyses of morphological traits in these related genera support the re-classification of the Bornean mountain ground squirrel, Dremomys everetti, to the genus Sundasciurus, which changes its name to Sundasciurus everetti. Past inclusion in the plain long-nosed squirrels (Dremomys) reflects convergent evolution between these high elevation species. (C) 2015 Elsevier Inc. All rights reserved. C1 [Hawkins, Melissa T. R.; Maldonado, Jesus E.; Tsuchiya, Mirian T. N.] Smithsonian Conservat Biol Inst, Ctr Conservat & Evolutionary Genet, Washington, DC 20008 USA. [Hawkins, Melissa T. R.; Helgen, Kristofer M.; Maldonado, Jesus E.; Tsuchiya, Mirian T. N.] Smithsonian Inst, Div Mammals, Natl Museum Nat Hist, Washington, DC 20013 USA. [Hawkins, Melissa T. R.; Leonard, Jennifer A.] CSIC, Estn Biol Donana, Conservat & Evolutionary Genet Grp, Seville 41092, Spain. [Hawkins, Melissa T. R.; Tsuchiya, Mirian T. N.] George Mason Univ, Dept Environm Sci & Policy, Fairfax, VA 22030 USA. [Rockwood, Larry L.] George Mason Univ, Dept Biol, Fairfax, VA 22030 USA. RP Hawkins, MTR (reprint author), Smithsonian Conservat Biol Inst, Ctr Conservat & Evolutionary Genet, Natl Zool Pk, Washington, DC 20008 USA. EM robertsmt@si.edu RI CSIC, EBD Donana/C-4157-2011; Leonard, Jennifer/A-7894-2010 OI CSIC, EBD Donana/0000-0003-4318-6602; Leonard, Jennifer/0000-0003-0291-7819 FU Spanish Government [CGL2010-21524)] FX The authors thank Richard Thorington, Jr. and Larry Heaney for guidance, advice, and tissue samples. The field samples collected for this study would not have been possible without the help of Maklarin Lakim, Fred Tuh Yit Yuh, Paul Yambun, and Justin Sator (Sabah Parks, Sabah, Malaysia). The field expedition would not have been successful without the help of the field crew: Miguel Camacho Sanchez, Lyndon R. Hawkins, Flavia Porto Peter, Manuel Lopez Rivera, Francisco Alberto Carro Marino, and the incredible Malaysian staff-Yana Melody, Stephany Disna Ahyu, Foziah Ann, Ipe and Azly and all the porters who made this trip possible. We also extend gratitude to Louise Emmons, Han Kwai and Konstans Wells for the pre-expedition advice. Rose Ragai deserves special recognition for tremendous field assistance and serving as a translator. David Aragones from the GIS and Remote Sensing Laboratory (LAST-EBD) of the Doriana Biological Station, CSIC made the map. Megan Krol drew the auditory bulla illustrations. Eliecer Gutierrez and E. Grace Veatch assisted with generating the PCA, and associated R scripts. Dean Adams provided guidance for using geomorph for the PTA. C. Miguel Pinto and Richard Ree assisted with the Lagrange ancestral range reconstruction. Lyndon Hawkins provided the photograph from Mount Kinabalu, Sabah, Malaysia. Tabitha Viner and the National Zoological Park (Smithsonian Institution), Department of Pathology provided several zoo tissue samples. Tissues were also obtained from Linda Gordon, the National Museum of Natural History, Smithsonian Institution, Washington, D.C., USA; Bill Stanley, Field Museum of Natural History, Chicago; Chris Conroy, Museum of Vertebrate Zoology, Berkeley, USA; Paula Jenkins, Natural History Museum, London, U.K.; Burton Lim, Royal Ontario Museum, Toronto, Canada; and Robert Palmer Australian National Wildlife Collection (CSIRO), Canberra, Australia. Logistical support was provided by the Center for Conservation and Evolutionary Genetics, National Zoological Park, Smithsonian Institution, Washington DC, USA, and gratitude is extended to Robert Fleischer, Nancy Rotzel McInerney. Funding was provided by the Spanish Government (CGL2010-21524). Two anonymous reviewers and the associate editor provided comments that greatly improved the quality of this manuscript. NR 79 TC 2 Z9 2 U1 4 U2 27 PU ACADEMIC PRESS INC ELSEVIER SCIENCE PI SAN DIEGO PA 525 B ST, STE 1900, SAN DIEGO, CA 92101-4495 USA SN 1055-7903 EI 1095-9513 J9 MOL PHYLOGENET EVOL JI Mol. Phylogenet. Evol. PD JAN PY 2016 VL 94 BP 752 EP 764 DI 10.1016/j.ympev.2015.10.023 PN B PG 13 WC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity SC Biochemistry & Molecular Biology; Evolutionary Biology; Genetics & Heredity GA CY5JG UT WOS:000366443300025 PM 26524259 ER PT J AU Sues, HD Averianov, A AF Sues, Hans-Dieter Averianov, Alexander TI Ornithomimidae (Dinosauria: Theropoda) from the Bissekty Formation (Upper Cretaceous: Turonian) of Uzbekistan SO CRETACEOUS RESEARCH LA English DT Article DE Dinosauria; Theropoda; Omithomimidae; Cretaceous; Uzbekistan ID OSTRICH DINOSAURS; GIANT ORNITHOMIMOSAUR; MONGOLIA; CHINA; STRUTHIOMIMUS; SAURISCHIA; BARSBOLD; REMAINS; CANADA AB The stratigraphically oldest remains of omithomimid theropod dinosaurs are known from the Cenomanian Khodzhakul Formation and the Turonian Bissekty Formation of Uzbekistan. The ornithomimid from the Bissekty Formation is documented by more than 800 isolated bones that represent much of the skeleton. It shows at least three unambiguous synapomorphies of Ornithomimidae: length of anterior cervical centra three to five times greater than transverse width; low and rounded fibular crest of tibia; metatarsal III pinched between. metatarsals II and IV; and proximal end of metatarsal III not visible in anterior view. Phylogenetic analysis, based on a dataset with 568 morphological characters and including all known omithomimosaurian taxa, places the omithomimid from the Bissekty Formation near the base of the omithomimid radiation, between Archaeornithomimus asiaticus and Sinornithomimus dongi. Published by Elsevier Ltd. C1 [Sues, Hans-Dieter] Smithsonian Inst, Dept Paleobiol, Natl Museum Nat Hist, Washington, DC 20013 USA. [Averianov, Alexander] Russian Acad Sci, Inst Zool, St Petersburg 199034, Russia. [Averianov, Alexander] St Petersburg State Univ, Geol Fac, Dept Sedimentary Geol, St Petersburg 199178, Russia. RP Sues, HD (reprint author), Smithsonian Inst, Dept Paleobiol, Natl Museum Nat Hist, MRC 121,POB 37012, Washington, DC 20013 USA. EM suesh@si.edu; dzharakuduk@mail.ru RI Averianov, Alexander/M-8490-2013 OI Averianov, Alexander/0000-0001-5948-0799 FU National Science Foundation [EAR-9804771, EAR-0207004]; National Geographic Society [5901-97, 6281-98]; Navoi Mining and Metallurgy Combinat; Russian Scientific Fund [14-14-00015] FX Fieldwork in Uzbekistan was facilitated by and conducted in cooperation with the Zoological Institute of the National Academy of Sciences of Uzbekistan, particularly D.A. Azimov and Y.A. Chikin. For their efforts in the field, scientific expertise, and camaraderie, we thank A.V. Abramov, J.D. Archibald, G.O. Cherepanov, I.G. Danilov, S. Dominguez, C. King, N. Morris, C.M. Redman, A.S. Resvyi, C. Skrabec, P.P. Skutschas, E.V. Syromyatnikova, and D.J. Ward. We are indebted to N.R. Longrich, Editor E. Koutsoukos, and E.B. Sues for helpful comments on a draft of the manuscript. The field work in 1997-2006 was funded by the National Science Foundation (EAR-9804771 and EAR-0207004 to J.D. Archibald and H.-D. Sues), the National Geographic Society (5901-97 and 6281-98 to J.D. Archibald and H.-D. Sues), and the Navoi Mining and Metallurgy Combinat. The laboratory research by AA is supported by the Russian Scientific Fund (14-14-00015). NR 51 TC 4 Z9 4 U1 0 U2 7 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0195-6671 EI 1095-998X J9 CRETACEOUS RES JI Cretac. Res. PD JAN PY 2016 VL 57 BP 90 EP 110 DI 10.1016/j.cretres.2015.07.012 PG 21 WC Geology; Paleontology SC Geology; Paleontology GA CW5SA UT WOS:000365055700009 ER PT J AU Fastovsky, DE Bercovici, A AF Fastovsky, David E. Bercovici, Antoine TI The Hell Creek Formation and its contribution to the Cretaceous-Paleogene extinction: A short primer SO CRETACEOUS RESEARCH LA English DT Article DE Hell Creek Formation (HCF); Maastrichtian; Mass extinction; Cretaceous-Paleogene boundary; Dinosaurs; Paleoenvironment ID K-T-BOUNDARY; SOUTHWESTERN NORTH-DAKOTA; PERMIAN MASS-EXTINCTION; FLOOD-BASALT ERUPTIONS; PLANT FOSSIL RECORD; TERTIARY BOUNDARY; EASTERN MONTANA; NEW-MEXICO; NORTHEASTERN MONTANA; DINOSAUR EXTINCTION AB Although it represents but one geographic data point, the uppermost Maastrichtian Hell Creek Formation (HCF), exposed in the upper Great Plains of the North American craton, remains the most studied source for understanding the final similar to 1.5 Myr of the Mesozoic Era in the terrestrial realm. Because it lies conformably below the earliest Paleocene Fort Union Formation, and together these two units preserve a rich fauna and flora, much of what is understood about the terrestrial Cretaceous-Paleogene (K-Pg) boundary comes from this sequence. The HCF has been reconstructed as an expansive, fluvially drained, low coastal plain, built out, to the west, against the Laramide Orogen, and to the east, against the ultimate transgression (Cannonball) of the Western Interior Sea. Its meandering rivers and moist soils supported a multi-tiered angiosperm-dominated flora and rich insect and vertebrate faunas, including dinosaurs, crocodilians, squamates, turtles, and mammals. A dramatic fades change representing the initiation of catastrophic flooding is preserved, within available levels precision, at the K-Pg boundary. High-precision stratigraphy has proven difficult in this lenticular fluvial system. Where present, the boundary can be recognized by the bipartite boundary claystone; otherwise, palynostratigraphy has proven a powerful tool. Numerical dates have been successfully obtained from in tonsteins at the boundary and above, in the Fort Union; however, these have proven elusive below the boundary within the HCF. The K-Pg boundary in this region is dated at 66.043 Ma (Renne et al., 2013). Magnetostrati-graphic studies have been carried out in the HCF; although all but one have lacked numerical dates, these have been used for correlations of widespread, disjunct exposures and for the estimation of sedimentation rates. The palynoflora is largely homogenous through the HCF; at the K-Pg boundary, it shows an abrupt similar to 30% extinction. This makes it a powerful tool for identification of the K-Pg boundary, although because the boundary is identified on absence of Cretaceous taxa rather than presence of earliest Paleocene taxa, several competing methods have been applied to identifying the K-Pg boundary using pollen. The macroflora, consisting largely of leaves, consists of three successive floras, showing increasing diversity through the HCF. The ultimate of these three floras undergoes an abrupt 57% extinction; taken as a whole, however, the macroflora undergoes a 78% extinction at the K-Pg boundary. The best data available for dinosaurs - including archaic Ayes - show an abrupt extinction. By contrast, salamanders and other lissamphibians, as well as chelonians, cross the boundary virtually without perturbation. Squamates appear to have suffered significant extinctions at the K-Pg boundary, as did euselachians (elasmobranchs) and insects. Mammals suffered a 75% extinction; however, some of this figure cannot be shown to have occurred in less than the last 500 kyr of the Cretaceous, and thus has been potentially attributable to causes other than a bolide impact. Taken together, the survivorship patterns are concordant with the catastrophic inception of ubiquitous flooding characterizing the K-Pg boundary. While the key K-Pg boundary question in the HCF was once the rate of the biotic extinction, it has moved to the distinction between single-cause scenarios, with the Chicxulub bolide as agent of extinction, and multi-cause scenarios, uniting habitat partitioning, Deccan flood-basalt volcanism, climate change, competition, and bolide impact. Not every potential environmental perturbation need be a mechanism for the extinction: parsimony and the data continue to be concordant with a bolide impact as the single agent of the terrestrial K-Pg mass extinction. (C) 2015 Elsevier Ltd. All rights reserved. C1 [Fastovsky, David E.] Univ Vienna, Dept Lithospharenforsch, UZA 2, Vienna, Austria. [Fastovsky, David E.] Univ Rhode Isl, Dept Geosci, Kingston, RI 02881 USA. [Bercovici, Antoine] Smithsonian Inst, Natl Museum Nat Hist, Dept Paleobiol MRC 121, Washington, DC 20560 USA. RP Fastovsky, DE (reprint author), Univ Rhode Isl, Dept Geosci, Kingston, RI 02881 USA. EM defastov@uri.edu FU Austrian-American Education Commission; Department fur Lithospharenforschung at the University of Vienna (Austria); Department of Geosciences, University of Rhode Island (USA); Deep Time Peter Buck Postdoctoral Fellowship from the NMNH Smithsonian Institution FX David E. Fastovsky gratefully acknowledges the support of the Austrian-American Education Commission (through a Fulbright Scholarship), the Department fur Lithospharenforschung at the University of Vienna (Austria), and the Department of Geosciences, University of Rhode Island (USA). Antoine Bercovici is currently supported by a Deep Time Peter Buck Postdoctoral Fellowship from the NMNH Smithsonian Institution. We are thankful to Dean A. Pearson (Pioneer Trails Regional Museum, Bowman, ND), and to Tyler R. Lyson (Marmarth Research Foundation), for logistical support and assistance in the field. We are particularly grateful to the conveners of the September, 2014 Tremp (Spain) conference for both that event and for giving us the opportunity to contribute to this volume. Finally, our manuscript was aided significantly by the thoughtful, detailed reviews of Eric Buffetaut and Stephen Brusatte. NR 224 TC 1 Z9 1 U1 14 U2 46 PU ACADEMIC PRESS LTD- ELSEVIER SCIENCE LTD PI LONDON PA 24-28 OVAL RD, LONDON NW1 7DX, ENGLAND SN 0195-6671 EI 1095-998X J9 CRETACEOUS RES JI Cretac. Res. PD JAN PY 2016 VL 57 BP 368 EP 390 DI 10.1016/j.cretres.2015.07.007 PG 23 WC Geology; Paleontology SC Geology; Paleontology GA CW5SA UT WOS:000365055700031 ER PT J AU Jenks, KE Aikens, EO Songsasen, N Calabrese, J Fleming, C Bhumpakphan, N Wanghongsa, S Kanchanasaka, B Songer, M Leimgruber, P AF Jenks, Kate E. Aikens, Ellen O. Songsasen, Nucharin Calabrese, Justin Fleming, Chris Bhumpakphan, Naris Wanghongsa, Sawai Kanchanasaka, Budsabong Songer, Melissa Leimgruber, Peter TI Comparative movement analysis for a sympatric dhole and golden jackal in a human-dominated landscape SO RAFFLES BULLETIN OF ZOOLOGY LA English DT Article DE Animal movement; Canids; daily activity; K-means cluster analysis; local convex hull; semi-variograms ID CUON-ALPINUS CANIDAE; HOME RANGES; SPACE-USE; UTILIZATION DISTRIBUTIONS; SPATIAL ECOLOGY; NATIONAL-PARK; AUREUS; INDIA; RADIOTELEMETRY; POPULATION AB GPS tracking enables the collection of large quantities of data on animal movements which can help guide conservation efforts. Using movement data from a dhole (Cuon alpinus) and a golden jackal (Canis aureus), we demonstrate the efficacy of movement analysis techniques to explore and contrast the movement patterns of these two individuals. The jackal used a 151 km(2) local convex hull home ranged covering mostly agricultural lands during the monitoring period, but the dhole restricted its movements to protected forest and a home range size of 33 km2. Autocorrelation functions demonstrated consistent nocturnal activity for the jackal and diurnal activity for the dhole. K-means cluster analysis of step lengths and turning angles along with semi-variograms showed that the jackal utilised larger areas and traveled longer distances than the dhole. By combining a comparative approach with simple movement analysis techniques, insights into the space use strategies of canids can be gained in order to enhance our ability to develop effective conservation strategies for these largely persecuted species. C1 [Jenks, Kate E.; Aikens, Ellen O.; Songsasen, Nucharin; Calabrese, Justin; Fleming, Chris; Songer, Melissa; Leimgruber, Peter] Conservat Ecol Ctr, Natl Zool Pk, Smithsonian Conservat Biol Inst, 1500 Remount Rd, Front Royal, VA 22630 USA. [Jenks, Kate E.] Minnesota Zoo, Apple Valley, MN 55124 USA. [Fleming, Chris] Univ Maryland, Dept Biol, College Pk, MD 20742 USA. [Bhumpakphan, Naris] Kasetsart Univ, Dept Forest Biol, Bangkok, Thailand. [Wanghongsa, Sawai; Kanchanasaka, Budsabong] Thailand Dept Natl Pk Wildlife & Plant Conservat, Bangkok, Thailand. RP Jenks, KE (reprint author), Conservat Ecol Ctr, Natl Zool Pk, Smithsonian Conservat Biol Inst, 1500 Remount Rd, Front Royal, VA 22630 USA. EM kate.jenks@state.mn.us RI Calabrese, Justin/B-9131-2012; Leimgruber, Peter/O-1304-2015 OI Leimgruber, Peter/0000-0002-3682-0153 FU Thailand Department of National Parks, Wildlife, and Plant Conservation; Smithsonian; Association of Zoo and Aquarium's Conservation Endowment Fund; Minnesota Zoo Ulysses S. Seal Conservation Grant; Dickerson Park Zoo FX This study was supported by the Thailand Department of National Parks, Wildlife, and Plant Conservation. We thank S. Panda for his extensive assistance with animal trapping and tracking. L. Padilla, Y. Marnoch, B. Sangkharak, Boripat and the Zoological Park Organization of Thailand provided veterinary assistance. Field work and equipment was funded in part by the Smithsonian, Association of Zoo and Aquarium's Conservation Endowment Fund, and a Minnesota Zoo Ulysses S. Seal Conservation Grant. Additional funding was provided by the Dickerson Park Zoo. We would like to thank the Smithsonian Conservation Biology Institute's GIS Lab and internship program for supporting Ellen Aikens. Finally, we would like to thank Thomas Mueller for his data analysis advice and four anonymous reviewers for improving the manuscript. NR 55 TC 0 Z9 1 U1 14 U2 26 PU NATL UNIV SINGAPORE, SCHOOL BIOLOGICAL SCIENCES PI SINGAPORE PA DEPT ZOOLOGY, KENT RIDGE, SINGAPORE 0511, SINGAPORE SN 0217-2445 J9 RAFFLES B ZOOL JI Raffles Bull. Zool. PD DEC 31 PY 2015 VL 63 BP 546 EP 554 PG 9 WC Zoology SC Zoology GA DD3PC UT WOS:000369833600044 ER PT J AU Acevedo-Rodriguez, P AF Acevedo-Rodriguez, Pedro TI (2407) Proposal to conserve Paullinia thalictrifolia against P. bipinnata (Sapindaceae) SO TAXON LA English DT Editorial Material C1 [Acevedo-Rodriguez, Pedro] Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, POB 37012, Washington, DC 20013 USA. RP Acevedo-Rodriguez, P (reprint author), Smithsonian Inst, Dept Bot, Natl Museum Nat Hist, POB 37012, Washington, DC 20013 USA. EM acevedop@si.edu NR 0 TC 0 Z9 0 U1 2 U2 2 PU INT ASSOC PLANT TAXONOMY-IAPT PI BRATISLAVA PA C/O INST BOTANY, SLOVAK ACAD SCIENCES DUBRAVSKA CESTA 9, SK-845 23 BRATISLAVA, SLOVAKIA SN 0040-0262 EI 1996-8175 J9 TAXON JI Taxon PD DEC 31 PY 2015 VL 64 IS 6 BP 1330 EP U370 PG 2 WC Plant Sciences; Evolutionary Biology SC Plant Sciences; Evolutionary Biology GA DC7YA UT WOS:000369435700029 ER PT J AU Krupnick, GA Schuettpelz, E AF Krupnick, Gary A. Schuettpelz, Eric TI TWELFTH SYMPOSIUM OF THE IOPB SO TAXON LA English DT Editorial Material C1 [Krupnick, Gary A.; Schuettpelz, Eric] Smithsonian Inst, Dept Bot, NMNH, MRC 166, Washington, DC 20013 USA. RP Krupnick, GA (reprint author), Smithsonian Inst, Dept Bot, NMNH, MRC 166, Washington, DC 20013 USA. EM krupnick@si.edu; schuettpelze@si.edu OI Krupnick, Gary/0000-0002-1357-4826 NR 0 TC 0 Z9 0 U1 1 U2 1 PU INT ASSOC PLANT TAXONOMY-IAPT PI BRATISLAVA PA C/O INST BOTANY, SLOVAK ACAD SCIENCES DUBRAVSKA CESTA 9, SK-845 23 BRATISLAVA, SLOVAKIA SN 0040-0262 EI 1996-8175 J9 TAXON JI Taxon PD DEC 31 PY 2015 VL 64 IS 6 BP 1356 EP 1357 PG 2 WC Plant Sciences; Evolutionary Biology SC Plant Sciences; Evolutionary Biology GA DC7YA UT WOS:000369435700045 ER PT J AU Sohn, J Hwang, HS Geller, MJ Diaferio, A Rines, KJ Lee, MG Lee, GH AF Sohn, Jubee Hwang, Ho Seong Geller, Margaret J. Diaferio, Antonaldo Rines, Kenneth J. Lee, Myung Gyoon Lee, Gwang-Ho TI COMPACT GROUPS OF GALAXIES WITH COMPLETE SPECTROSCOPIC REDSHIFTS IN THE LOCAL UNIVERSE SO JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY LA English DT Article DE galaxies: evolution; galaxies: groups: general; galaxies: interactions; galaxies ID DIGITAL SKY SURVEY; 6TH DATA RELEASE; RICH CLUSTERS; VIRIAL-THEOREM; MASS PROFILES; SOUTHERN SKY; LOOSE GROUPS; DARK-MATTER; CATALOG; DYNAMICS AB Dynamical analysis of compact groups provides important tests of models of compact group formation and evolution. By compiling 2066 redshifts from FLWO/FAST, from the literature, and from SDSS DR12 in the fields of compact groups in McConnachie et al. (2009), we construct the largest sample of compact groups with complete spectroscopic redshifts in the redshift range 0.01 < z < 0.22. This large redshift sample shows that the interloper fraction in the McConnachie et al. (2009) compact group candidates is similar to 42%. A secure sample of 332 compact groups includes 192 groups with four or more member galaxies and 140 groups with three members. The fraction of early-type galaxies in these compact groups is 62%, higher than for the original Hickson compact groups. The velocity dispersions of early-and late-type galaxies in compact groups change little with groupcentric radius; the radii sampled are less than 100 h(-1) kpc, smaller than the radii typically sampled by members of massive clusters of galaxies. The physical properties of our sample compact groups include size, number density, velocity dispersion, and local environment; these properties slightly differ from those derived for the original Hickson compact groups and for the DPOSS II compact groups. Differences result from subtle differences in the way the group candidates were originally selected. The abundance of the compact groups changes little with redshift over the range covered by this sample. The approximate constancy of the abundance for this sample is a potential constraint on the evolution of compact groups on a few Gigayear timescale. C1 [Sohn, Jubee; Lee, Myung Gyoon; Lee, Gwang-Ho] Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea. [Hwang, Ho Seong] Korea Inst Adv Study, Sch Phys, Seoul 02455, South Korea. [Sohn, Jubee; Geller, Margaret J.] Smithsonian Astrophys Observ, Cambridge, MA 02138 USA. [Diaferio, Antonaldo] Univ Turin, Dipartimento Fis, I-10125 Turin, Italy. [Diaferio, Antonaldo] Ist Nazl Fis Nucl INFN, Sez Torino, I-10125 Turin, Italy. [Rines, Kenneth J.] Western Washington Univ, Dept Phys & Astron, Bellingham, WA 98225 USA. RP Sohn, J (reprint author), Seoul Natl Univ, Dept Phys & Astron, Seoul 08826, South Korea. EM jsohn@cfa.harvard.edu FU Smithsonian Astrophysical Observatory; National Research Foundation of Korea (NRF) grant - Korea Government (MSIP) [2013R1A2A2A05005120]; Global Ph.D. Fellowship Program through an NRF - MEST [20110007215]; Smithsonian Institution; INFN grant In Dark; grant Progetti di Ateneo TO Call of the University of Torino [2012 0011]; Italian Ministry of University and Research; National Research Foundation of Korea (NRF) Grant - Korean Government FX We thank the anonymous referee for a very prompt report. We thank Perry Berlind and Michael Calkins, the remote observers at the Fred Lawrence Whipple Observatory, Jessica Mink, who processed the spectroscopic data, and all FAST queue observers who took data for this program. This paper uses data products produced by the OIR Telescope Data Center, supported by the Smithsonian Astrophysical Observatory. This work was supported by the National Research Foundation of Korea (NRF) grant funded by the Korea Government (MSIP) (No.2013R1A2A2A05005120). J.S. was supported by Global Ph.D. Fellowship Program through an NRF funded by the MEST (No. 20110007215). The research of M.J.G. is supported by the Smithsonian Institution. AD acknowledges partial support from the INFN grant In Dark, the grant Progetti di Ateneo TO Call 2012 0011 'Marco Polo' of the University of Torino and the grant PRIN 2012 "Fisica Astroparticellare Teorica" of the Italian Ministry of University and Research. G.H.L. acknowledges the support by the National Research Foundation of Korea (NRF) Grant funded by the Korean Government (NRF-2012-Fostering Core Leaders of the Future Basic Science Program). NR 66 TC 2 Z9 2 U1 0 U2 3 PU KOREAN ASTRONOMICAL SOCIETY PI TAEJON PA 61-1 HWA-AM DONG, YUSUNG KU, TAEJON, 305-348, SOUTH KOREA SN 1225-4614 J9 J KOREAN ASTRON SOC JI J. Korean Astron. Soc. PD DEC 31 PY 2015 VL 48 IS 6 BP 381 EP 398 DI 10.5303/JKAS.2015.48.6.381 PG 18 WC Astronomy & Astrophysics SC Astronomy & Astrophysics GA DA0NS UT WOS:000367494900006 ER PT J AU Wilkerson, RC Linton, YM AF Wilkerson, Richard C. Linton, Yvonne-Marie TI Elevation of Pseudoskusea, Rusticoidus and Protomacleaya to valid subgenera in the mosquito genus Aedes based on taxon naming criteria recently applied to other members of the Tribe Aedini (Diptera: Culicidae) SO PARASITES & VECTORS LA English DT Article DE Tribe Aedini; Aedes; Subgenera; Elevation ID LIFE STAGES; MORPHOLOGICAL DATA; CLASSIFICATION; PHYLOGENY; OCHLEROTATUS AB Background: Pseudoskusea, Rusticoidus and Protomacleaya were well-recognized, morphologically distinct subgenera within the genus Aedes prior to a series of taxonomic changes over the past 15 years by Reinert, Harbach and Kitching, when they were recognized as subgenera of the genus Ochlerotatus. In our recent effort to stabilize the Tribe Aedini, we synonymized these subgenera and associated species back into the genus Aedes, but incorrectly assigned them as putative informal groups, instead of reinstating them to subgenera. Conclusion: Here we formally elevate three traditionally recognized subgenera (Pseudoskusea, Rusticoidus and Protomacleaya) within the genus Aedes. C1 [Wilkerson, Richard C.; Linton, Yvonne-Marie] Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. [Linton, Yvonne-Marie] Smithsonian Inst, Walter Reed Biosystemat Unit, Museum Support Ctr, Suitland, MD USA. [Linton, Yvonne-Marie] Walter Reed Army Inst Res, Dept Entomol, Silver Spring, MD USA. [Linton, Yvonne-Marie] Uniformed Serv Univ Hlth Sci, Fac Preventat Med & Biometr, Bethesda, MD 20814 USA. RP Wilkerson, RC (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Dept Entomol, Washington, DC 20560 USA. EM wilkersonr@si.edu FU National Research Council (NRC) FX We thank Bruce Harrison for careful review of the manuscript and his many helpful comments. This research was performed under a Memorandum of Understanding between the Walter Reed Army Institute of Research and the Smithsonian Institution, with institutional support provided by both organizations. This manuscript was prepared whilst YML held a National Research Council (NRC) Research Associateship Award at the Walter Reed Army Institute of Research. The material to be published reflects the views of the authors and should not be construed to represent those of the U.S. Department of the Army or the U.S. Department of Defense. NR 29 TC 1 Z9 1 U1 0 U2 0 PU BIOMED CENTRAL LTD PI LONDON PA 236 GRAYS INN RD, FLOOR 6, LONDON WC1X 8HL, ENGLAND SN 1756-3305 J9 PARASITE VECTOR JI Parasites Vectors PD DEC 30 PY 2015 VL 8 AR 668 DI 10.1186/s13071-015-1247-x PG 4 WC Parasitology SC Parasitology GA CZ8BY UT WOS:000367326200002 PM 26714624 ER PT J AU Macaluso, DA Aguilar, A Kilcoyne, ALD Red, EC Bilodeau, RC Phaneuf, RA Sterling, NC McLaughlin, BM AF Macaluso, D. A. Aguilar, A. Kilcoyne, A. L. D. Red, E. C. Bilodeau, R. C. Phaneuf, R. A. Sterling, N. C. McLaughlin, B. M. TI Absolute single-photoionization cross sections of Se2+: Experiment and theory SO PHYSICAL REVIEW A LA English DT Article ID NEUTRON-CAPTURE ELEMENTS; ATOMIC DATA; PLANETARY-NEBULAE; ABUNDANCE DETERMINATIONS; IONS; SPECTROSCOPY; EXCITATION; SELENIUM; IMPACT; STATES AB Absolute single-photoionization cross-section measurements for Se2+ ions were performed at the Advanced Light Source at Lawrence Berkeley National Laboratory using the merged-beams photo-ion technique. Measurements were made at a photon energy resolution of 24 +/- 3 meV in the photon energy range 23.5-42.5 eV, spanning the ground state and low-lying metastable state ionization thresholds. To clearly resolve the resonant structure near the ground-state threshold, high-resolution measurements were made from 30.0 to 31.9 eV at a photon energy resolution of 6.7 +/- 0.7 meV. Numerous resonance features observed in the experimental spectra are assigned and their energies and quantum defects tabulated. The high-resolution cross-section measurements are compared with large-scale, state-of-the-art theoretical cross-section calculations obtained from the Dirac Coulomb R-matrix method. Suitable agreement is obtained over the entire photon energy range investigated. These results are an experimental determination of the absolute photoionization cross section of doubly ionized selenium and include a detailed analysis of the photoionization resonance spectrum of this ion. C1 [Macaluso, D. A.] Univ Montana, Dept Phys & Astron, Missoula, MT 59812 USA. [Aguilar, A.; Kilcoyne, A. L. D.; Red, E. C.; Bilodeau, R. C.] Univ Calif Berkeley, Lawrence Berkeley Natl Lab, Adv Light Source, Berkeley, CA 94720 USA. [Bilodeau, R. C.] Western Michigan Univ, Dept Phys, Kalamazoo, MI 49008 USA. [Phaneuf, R. A.] Univ Nevada, Dept Phys, Reno, NV 89557 USA. [Sterling, N. C.] Univ West Georgia, Dept Phys, Carrollton, GA 30118 USA. [McLaughlin, B. M.] Queens Univ Belfast, CTAMOP, Sch Math & Phys, Belfast BT7 1NN, Antrim, North Ireland. [McLaughlin, B. M.] Harvard Smithsonian Ctr Astrophys, ITAMP, Cambridge, MA 02138 USA. RP Macaluso, DA (reprint author), Univ Montana, Dept Phys & Astron, Missoula, MT 59812 USA. EM david.macaluso@umontana.edu; bmclaughlin899@btinternet.com RI Kilcoyne, David/I-1465-2013 FU Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy (DOE) [DE-AC02-05CH11231, DE-AC03-76SF- 00098, DE-FG02-03ER15424]; Advanced Light Source; Montana Space Grant Consortium; NSF Astronomy and Astrophysics Postdoctoral Fellowship [AST-0901432]; NASA [06-APRA206-0049]; U.S. National Science Foundation under the visitors program; Harvard-Smithsonian Center for Astrophysics, Queen's University Belfast, through a visiting research fellowship (VRF); National Energy Research Scientific Computing Center [DE-AC02-05CH11231]; Oak Ridge National Laboratory [AC05-00OR22725] FX Support by the Office of Science, Office of Basic Energy Sciences, of the U.S. Department of Energy (DOE) under Contracts No. DE-AC02-05CH11231 and No. DE-AC03-76SF- 00098 and Grant No. DE-FG02-03ER15424 is gratefully acknowledged. D.M. acknowledges support from the Doctoral Fellowship in Residence Program at the Advanced Light Source and the Montana Space Grant Consortium. N.C.S. acknowledges support from an NSF Astronomy and Astrophysics Postdoctoral Fellowship under Award No. AST-0901432 and from NASA Grant No. 06-APRA206-0049. B.M.M. acknowledges support by the U.S. National Science Foundation under the visitors program and through a grant to ITAMP at the Harvard-Smithsonian Center for Astrophysics, Queen's University Belfast, through a visiting research fellowship (VRF). This research used resources of the National Energy Research Scientific Computing Center, which is supported by the Office of Science of the DOE under Contract No. DE-AC02-05CH11231. The computational work was performed at the National Energy Research Scientific Computing Center in Oakland, California, USA, and at The High Performance Computing Center Stuttgart (HLRS), University of Stuttgart, Stuttgart, Germany. This research also used resources of the Oak Ridge Leadership Computing Facility at the Oak Ridge National Laboratory, which is supported by the Office of Science of the DoE under Contract No. DE-AC05-00OR22725. NR 55 TC 3 Z9 3 U1 0 U2 10 PU AMER PHYSICAL SOC PI COLLEGE PK PA ONE PHYSICS ELLIPSE, COLLEGE PK, MD 20740-3844 USA SN 1050-2947 EI 1094-1622 J9 PHYS REV A JI Phys. Rev. A PD DEC 28 PY 2015 VL 92 IS 6 AR 063424 DI 10.1103/PhysRevA.92.063424 PG 11 WC Optics; Physics, Atomic, Molecular & Chemical SC Optics; Physics GA CZ8TD UT WOS:000367371100017 ER PT J AU Ho, HC McCosker, JE Smith, DG Shao, KT AF Ho, Hsuan-Ching McCosker, John E. Smith, David G. Shao, Kwang-Tsao TI Introduction to the systematics and biodiversity of eels (orders Anguilliformes and Saccopharyngiformes) of Taiwan SO ZOOTAXA LA English DT Article DE Biodiversity; Pisces; Anguilliformes; systematics; Taiwan ID MORAY EEL; SYNAPHOBRANCHID EEL; SOUTHEASTERN TAIWAN; NORTHEASTERN COAST; SOUTHERN TAIWAN; EASTERN TAIWAN; SNAKE-EEL; MURAENIDAE; OPHICHTHIDAE; GENUS AB The eel fauna (orders Anguilliformes and Saccopharyngiformes) of Taiwan is one of the richest in the world. Recent genetic and morphological studies have improved the taxonomic resolution and increased the known diversity of the eels of Taiwan, and the overall diversity is comparable to that of adjacent marine zoogeographic regions with rich biodiversity, such as Australia and the Philippines. In this special issue, we verified the historical records and examined numerous recently collected specimens, and conclude that the eel fauna of Taiwan is represented by 207 species in 75 genera and 14 families, with several undescribed species still likely to be discovered. The Muraenidae (71 species), Ophichthidae (60), Congridae (29) and Synaphobranchidae (17) are the most abundant and species-rich in Taiwanese waters. We add 42 species to the Taiwanese fish fauna, including one new genus and 13 new species. Two further species are newly described, one from the Philippines and one from Indonesia. C1 [Ho, Hsuan-Ching] Nat Museum Marine Biol & Aquarium, Pingtung, Taiwan. [Ho, Hsuan-Ching] Natl Dong Hwa Univ, Inst Marine Biol, Pingtung, Taiwan. [McCosker, John E.] Calif Acad Sci, San Francisco, CA 94118 USA. [Smith, David G.] Smithsonian Inst, Museum Support Ctr, Suitland, MD USA. [Shao, Kwang-Tsao] Acad Sinica, Biodivers Res Ctr, Taipei 115, Taiwan. RP Shao, KT (reprint author), Acad Sinica, Biodivers Res Ctr, Taipei 115, Taiwan. EM zoskt@gate.sinica.edu.tw FU National Museum of Marine Biology Aquarium; Ministry of Science and Technology FX This study is supported by the National Museum of Marine Biology & Aquarium and the Ministry of Science and Technology. We thank the chief editor, Z.-Q Zhang and the Zootaxa team for help in publishing this special issue and Eric Hilton (VIMS) and Wouter Holleman (SAIAB) for offering editorial assistance. We also thank the participants who contributed their study results to this special issue and all reviewers, subscribed or anonymous, who provide critical comments and valuable suggestions for the manuscripts. HCH especially thanks JEM, DGS and Yosuke Hibino (Mie University) for great help in verifying the species, valuable discussions and suggestions, and provided much help when preparing the manuscripts and this special issue. NR 45 TC 1 Z9 1 U1 1 U2 10 PU MAGNOLIA PRESS PI AUCKLAND PA PO BOX 41383, AUCKLAND, ST LUKES 1030, NEW ZEALAND SN 1175-5326 EI 1175-5334 J9 ZOOTAXA JI Zootaxa PD DEC 24 PY 2015 VL 4060 IS 1 BP 5 EP 18 PG 14 WC Zoology SC Zoology GA CZ4TR UT WOS:000367096100001 PM 26701585 ER PT J AU Tighe, KA Pogonoski, JJ Hibino, Y Ho, HC Nguyen, QV AF Tighe, Kenneth A. Pogonoski, John J. Hibino, Yusuke Ho, Hsuan-Ching Quan Van Nguyen TI Three new species of the genus Chlopsis (Anguilliformes: Chlopsidae) from the Indo-Pacific SO ZOOTAXA LA English DT Article DE taxonomy; Pisces; Chlopsis; nanhaiensis; orientalis; sagmacollaris ID XENOCONGRID EEL AB Three new species of false moray eels belonging to the genus Chlopsis, family Chlopsidae, are described and illustrated. Chlopsis sagmacollaris, from Western Australia, is characterized by its distinct color pattern with a unique dark saddle on the nape and paler body pigmentation than all other congeners. Chlopsis nanhaiensis, from Taiwan, has a bicolored body with its dorsal-fin origin behind a vertical through posterior margin of gill opening. These characters are shared with C. apterus, C. bicolor, C. bidentatus and C. orientalis sp. nov., but C. nanhaiensis has fewer total vertebrae than other bicolored species (ca. 120 in C. nanhaiensis vs. 125-140 in other four species). Chlopsis orientalis, from Vietnam, is distinguished from all other congeners except C. bicolor by its simple bicolored body, head length (ca. 10 % of total length), position of dorsal-fin origin (distinctly behind a vertical through posterior margin of gill opening), and counts of preanal and total vertebrae (35 and 135). Although C. orientalis resembles C. bicolor in meristics and morphometrics, it differs in its pigmentation and possession of stouter intermuscular bones. These new species represent the first records of the genus Chlopsis from the northwestern Pacific Ocean and the eastern Indian Ocean. C1 [Tighe, Kenneth A.] Smithsonian Inst, Natl Museum Nat Hist, Museum Support Ctr, Dept Vertebrate Zool, Suitland, MD 20746 USA. [Pogonoski, John J.] Australian Natl Fish Collect, CSIRO Natl Res Collect Australia, Hobart, Tas 7001, Australia. [Hibino, Yusuke] Mie Univ, Fisheries Res Lab, Shima, Mie 5170703, Japan. [Ho, Hsuan-Ching] Natl Museum Marine Biol & Aquarium, Pingtung, Taiwan. [Quan Van Nguyen] Vietnam Acad Sci & Technol, Inst Marine Environm & Resources, Hanoi, Vietnam. RP Tighe, KA (reprint author), Smithsonian Inst, Natl Museum Nat Hist, Museum Support Ctr, Dept Vertebrate Zool, MRC 534,4210 Silver Hill Rd, Suitland, MD 20746 USA. EM tighek@si.edu; john.pogonoski@csiro.au; 513d303@m.mie-u.ac.jp; ogcoho@gmail.com; quannv@imer.ac.nv RI Pogonoski, John /E-1710-2017 FU Asian Core Program of the Japan Society for the Promotion of Science; Japan Society for the Promotion of Science [11640696, 14540642]; Pham The Thu [KC.08.25]; [DC2: 15J02820] FX We would like to thank Martin F. Gomon and Dianne J. Bray (NMV), Alastair Graham (CSIRO), David G. Smith (USNM), and Seishi Kimura (FRLM) for making the specimens of C. sagmacollaris, C. nanhaiensis, and C. orientalis available. We would also like to thank John E. McCosker (CAS), David G. Smith, and Seishi Kimura for reviewing the manuscript. We express our gratitude to Seishi Kimura, Hiroyuki Motomura (KAUM), Keiichi Matsuura and Masanori Nakae (NSMT) for their help at the collecting site of the holotype of C. orientalis, and to Seishi Kimura for his suggestion of the collaborative work. Thanks to Pham The Thu (KC.08.25 project, IMER) for assists with organizing the fieldwork at Nha Trang, Vietnam. This study was supported in part by the Asian Core Program of the Japan Society for the Promotion of Science by the Japan Society for the Promotion of Science (11640696 and 14540642) and Grant-in-Aid for Japan Society for the Promotion of Science (JSPS) Fellows to Y.H. (DC2: 15J02820). NR 20 TC 1 Z9 1 U1 0 U2 2 PU MAGNOLIA PRESS PI AUCKLAND PA PO BOX 41383, AUCKLAND, ST LUKES 1030, NEW ZEALAND SN 1175-5326 EI 1175-5334 J9 ZOOTAXA JI Zootaxa PD DEC 24 PY 2015 VL 4060 IS 1 BP 19 EP 29 PG 11 WC Zoology SC Zoology GA CZ4TR UT WOS:000367096100002 PM 26701586 ER PT J AU Ho, HC McCosker, JE Smith, DG AF Ho, Hsuan-Ching McCosker, John E. Smith, David G. TI Renaming of three recently described eels of the genus Neenchelys (Teleostei: Anguilliformes: Ophichthidae) from the western Pacific SO ZOOTAXA LA English DT Article AB In our earlier paper (Ho et al., 2013), we described three new species of the eel genus Neenchelys Bamber, 1915. Unfortunately, the critical step of registering the work in ZooBank was omitted, thus rendering the names unavailable. In this paper, we present abbreviated descriptions of the new species in order to make these names available in accordance with the amended Article 8.5 of the International Code of Zoological Nomenclature. C1 [Ho, Hsuan-Ching] Nat Museum Marine Biol & Aquarium, Pingtung 944, Taiwan. [Ho, Hsuan-Ching] Natl Dong Hwa Univ, Inst Marine Biol, Pingtung 944, Taiwan. [McCosker, John E.] Calif Acad Sci, San Francisco, CA 94118 USA. [Smith, David G.] Smithsonian Inst, Museum Support Ctr, Suitland, MD 20746 USA. RP Ho, HC (reprint author), Nat Museum Marine Biol & Aquarium, Pingtung 94