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description Publicationkeyboard_double_arrow_right Article 2018 FrancePublisher:Public Library of Science (PLoS) Funded by:ANR | CRB-AnimANR| CRB-AnimYi-Chen Chen; Wei-Che Chang; Shau-Ping Lin; Masataka Minami; Christian Jean; Hisato Hayashi; Sylvie Rival-Gervier; Tatsuro Kanaki; Shinn-Chih Wu; Bertrand Pain;Scalable production of avian cell lines exhibits a valuable potential on therapeutic application by producing recombinant proteins and as the substrate for virus growth due to the special glycosylation occurs in avian species. Chicken primordial germ cells (cPGCs), a germinal pluripotent avian cell type, present the ability of self-renewal, an anchorage-independent cell growth and the ability to be genetically modified. This cell type could be an interesting bioreactor system for industrial purposes. This study sought to establish an expandable culture system with defined components for three-dimensional (3D) culture of cPGCs. cPGCs were cultured in medium supplemented with the functional polymer FP003. Viscoelasticity was low in this medium but cPGCs did not sediment in culture and efficiencies of space and nutrient utilization were thus enhanced and consequently their expansion was improved. The total number of cPGCs increased by 17-fold after 1 week of culture in 3D-FAot medium, an aseric defined medium containing FP003 polymer, FGF2 and Activin A as growth factors and Ovotransferrin as protein. Moreover, cPGC cell lines stably expressed the germline-specific reporter VASA:tdTOMATO, as well as other markers of cPGCs, for more than 1 month upon culture in 3D-FAot medium, indicating that the characteristics of these cells are maintained. In summary, this novel 3D culture system can be used to efficiently expand cPGCs in suspension without mechanical stirring, which is available for long-term culture and no loss of cellular properties was found. This system provides a platform for large-scale culture of cPGCs.
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6150485Data sources: PubMed CentralMémoires en Sciences de l'Information et de la CommunicationArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01906546/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0200515&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6150485Data sources: PubMed CentralMémoires en Sciences de l'Information et de la CommunicationArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01906546/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0200515&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2007 United States, FrancePublisher:American Geophysical Union (AGU) Martine Simoes; Jean Philippe Avouac; Olivier Beyssac; Bruno Goffé; Kenneth A. Farley; Yue-Gau Chen;doi: 10.1029/2006jb004824
The Taiwan mountain belt is classically viewed as a case example of a critical wedge growing essentially by frontal accretion and therefore submitted to distributed shortening. However, a number of observations call for a significant contribution of underplating to the growth of the orogenic wedge. We propose here a new thermokinematic model of the Taiwan mountain belt reconciling existing kinematic, thermometric and thermochronological constraints. In this model, shortening across the orogen is absorbed by slip on the most frontal faults of the foothills. Crustal thickening and exhumation are sustained by underplating beneath the easternmost portion of the wedge (Tananao Complex, TC), where the uplift rate is estimated to 6.3 mm a1, and beneath the westernmost internal region of the orogen (Hsueshan Range units, HR), where the uplift rate is estimated to 4.2 mm a1. Our model suggests that the TC units experienced a synchronous evolution along strike despite the southward propagation of the collision. It also indicates that they have reached a steady state in terms of cooling ages but not in terms of peak metamorphic temperatures. Exhumation of the HR units increases northward but has not yet reached an exhumational steady state. Presently, frontal accretion accounts for less than 10% of the incoming flux of material into the orogen, although there is indication that it was contributing substantially more (80%) before 4 Ma. The incoming flux of material accreted beneath the TC significantly increased 1.5 Ma ago. Our results also suggest that the flux of material accreted to the orogen corresponds to the top 7 km of the upper crust of the underthrust Chinese margin. This indicates that a significant amount (76%) of the underthrust material has been subducted into the mantle, probably because of the increase in density associated with metamorphism. We also show that the density distribution resulting from metamorphism within the orogenic wedge explains well the topography and the gravity field. By combining available geological data on the thermal and kinematic evolution of the wedge, our study sheds new light onto mountain building processes in Taiwan and allows for reappraising the initial structural architecture of the passive margin. International audience
HAL-Rennes 1; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2007 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-Rennes 1; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2007add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2006jb004824&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 93 citations 93 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!visibility 1visibility views 1 Powered bymore_vert HAL-Rennes 1; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2007 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-Rennes 1; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2007add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2006jb004824&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2018 FrancePublisher:Public Library of Science (PLoS) Authors: Callet, Thérèse; Dupont-Nivet, Mathilde; Cluzeaud, Marianne; Jaffrezic, Florence; +8 AuthorsCallet, Thérèse; Dupont-Nivet, Mathilde; Cluzeaud, Marianne; Jaffrezic, Florence; Laloë, Denis; Kerneis, Thierry; Labbé, Laurent; Quillet, Edwige; Geurden, Inge; Mazurais, David; Skiba-Cassy, Sandrine; Médale, Françoise;To meet the growing demand of fish feed for aquaculture, an increasing proportion of marine ingredients are being replaced by blends of plant products. However, the total replacement of marine ingredients in salmonid diets impairs fish performance. This is particularly true during the early fry stage and this stage is therefore considered of particular importance. In rainbow trout (RBT), the existence of a genetic variability to survive and grow with plant-based diets devoid of marine ingredients has now been proved, but the mechanisms behind are little studied especially at early stage. To investigate these, we analysed the whole transcriptome of three isogenic lines of RBT fry, which have similar growth when fed a marine resources-based diet (M diet) but which highly differ in their responses to a plant-based diet (V diet). Analysis of transcriptomes profiles revealed 1740, 1834 and 246 probes differentially expressed among the three genotypes when fed the V diet. The use of these lines led to the discovery of potential molecular markers linked to plant-based diet utilisation, some of them belonging to new pathways, never described before. An important number of genes was related to immunity, but further investigations are needed to better understand the difference between the genotypes in their immune status response to V diet exposure. Finally, differences in expression of genes related to feed intake and sensory perception among genotypes suggested that the mechanisms underlying the differences in growth on plant-based diet are closely linked to diet acceptance. Research on plants components affecting feed intake should be thus further explored. Unités expérimentales PEIMA et NuMeA-Donzacq International audience
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6067751Data sources: PubMed CentralArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01857986/documentArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of Ifremeradd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0201462&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 13 citations 13 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 10visibility views 10 download downloads 1 Powered bymore_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6067751Data sources: PubMed CentralArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01857986/documentArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of Ifremeradd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0201462&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2010 FrancePublisher:American Geophysical Union (AGU) Authors: Sebastien Boutareaud; Anne-Marie Boullier; Muriel Andreani; Dan-Gabriel Calugaru; +3 AuthorsSebastien Boutareaud; Anne-Marie Boullier; Muriel Andreani; Dan-Gabriel Calugaru; Pierre Beck; Sheng-Rong Song; Toshihiko Shimamoto;doi: 10.1029/2008jb006254
Spherical aggregates named clay-clast aggregates (CCAs) have been reported from recent investigations on retrieved clay-bearing fault gouges from shallow depth seismogenic faults and rotary shear experiments conducted on clay-bearing gouge at seismic slip rates. The formation of CCAs appears to be related to the shearing of a smectite-rich granular material that expands and becomes fluidized. We have conducted additional high-velocity rotary shear experiments and low-velocity double-shear experiments. We demonstrate that a critical temperature depending on dynamic pressure-temperature conditions is needed for the formation of CCAs. This temperature corresponds to the phase transition of pore water from liquid to vapor or to critical, which induced gouge pore fluid expansion and therefore a thermal pressurization of the fault. A detailed examination by energy dispersive X-ray spectrometry (EDX-SEM) element mapping, SEM, and transmission electron microscopy (TEM) shows strong similar characteristics of experimental and natural CCAs with a concentric well-organized fabric of the cortex and reveals that their development may result from the combination of electrostatic and capillary forces in a critical reactive medium during the dynamic slip weakening. Accordingly, the occurrence of CCAs in natural clay-rich fault gouges constitutes new unequivocal textural evidence for shallow depth thermal pressurization and consequently for past seismic faulting. International audience
HAL-ENS-LYON; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2010 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-ENS-LYON; Hal-DiderotArticle . 2010HAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2010add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2008jb006254&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 104 citations 104 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!more_vert HAL-ENS-LYON; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2010 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-ENS-LYON; Hal-DiderotArticle . 2010HAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2010add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2008jb006254&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2019 France, Netherlands, Netherlands, Netherlands, United Kingdom, Netherlands, Italy, Italy, United States, Netherlands, Finland, Japan, Spain, NetherlandsPublisher:American Astronomical Society Funded by:NSF | Center for Cosmological P..., NSERC, NSF | Graduate Research Fellows... +15 projectsNSF| Center for Cosmological Physics ,NSERC ,NSF| Graduate Research Fellowship Program (GRFP) ,EC| BLACKHOLECAM ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Arizona Radio Observatory: Surveying the ISM through Millimeter and Sub-millimeter Spectroscopy ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,NSF| PSCIC Full Proposal: The iPlant Collaborative: A Cyberinfrastructure-Centered Community for a New Plant Biology ,NWO| From micro- to mega-scales: understanding how black holes shape the local Universe ,AKA| Physics of Black Hole-Powered Jets ,NSF| The iPlant Collaborative: Cyberinfrastructure for the Life Sciences ,EC| AENEAS ,NSF| CyVerse: Cyberinfrastructure for the Life Sciences ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,NSF| MRI: Development of an ALMA Beamformer for Ultra High Resolution VLBI and High Frequency Phased Array Science ,EC| RadioNet ,AKA| Physics of Black Hole-Powered JetsKazunori Akiyama; Antxon Alberdi; Walter Alef; Keiichi Asada; Rebecca Azulay; Anne Kathrin Baczko; David Ball; Mislav Baloković; John E. Barrett; Dan Bintley; Lindy Blackburn; W. Boland; Katherine L. Bouman; Geoffrey C. Bower; Michael Bremer; Christiaan D. Brinkerink; Roger Brissenden; Silke Britzen; Avery E. Broderick; Thomas Bronzwaer; Do-Young Byun; Andrew Chael; Chi-kwan Chan; Shami Chatterjee; Koushik Chatterjee; Ming-Tang Chen; Yi Chen; Ilje Cho; Pierre Christian; John Conway; James M. Cordes; Geoffrey B. Crew; Yuzhu Cui; Jordy Davelaar; Mariafelicia De Laurentis; Roger Deane; Jessica Dempsey; Gregory Desvignes; Jason Dexter; Sheperd S. Doeleman; R. P. Eatough; Heino Falcke; Vincent L. Fish; Ed Fomalont; Raquel Fraga-Encinas; Per Friberg; José L. Gómez; Peter Galison; Charles F. Gammie; Roberto Garcia; Olivier Gentaz; Boris Georgiev; Ciriaco Goddi; Roman Gold; Minfeng Gu; Mark Gurwell; Kazuhiro Hada; Michael H. Hecht; Ronald Hesper; Luis C. Ho; Paul T. P. Ho; Mareki Honma; Chih-Wei Locutus Huang; Lei Huang; David H. Hughes; Shiro Ikeda; Makoto Inoue; Sara Issaoun; David J. James; Buell T. Jannuzi; Michael Janssen; Britton Jeter; Wu Jiang; Michael D. Johnson; Svetlana G. Jorstad; Taehyun Jung; Mansour Karami; Ramesh Karuppusamy; Tomohisa Kawashima; Garrett K. Keating; Mark Kettenis; Jae-Young Kim; Junhan Kim; Motoki Kino; Jun Yi Koay; Patrick M. Koch; Shoko Koyama; Michael Kramer; Carsten Kramer; Thomas P. Krichbaum; C. Y. Kuo; Tod R. Lauer; Sang-Sung Lee; Yan-Rong Li; Zhiyuan Li; Michael Lindqvist; Kuo Liu; Elisabetta Liuzzo; Andrei P. Lobanov; Laurent Loinard; Colin J. Lonsdale; Ru-Sen Lu; Nicholas R. MacDonald; Jirong Mao; Sera Markoff; Daniel P. Marrone; Alan P. Marscher; Satoki Matsushita; Lynn D. Matthews; Lia Medeiros; Karl M. Menten; Yosuke Mizuno; Izumi Mizuno; James M. Moran; Kotaro Moriyama; Monika Moscibrodzka; Cornelia Müller; Hiroshi Nagai; Neil M. Nagar; Masanori Nakamura; Ramesh Narayan; Gopal Narayanan; Iniyan Natarajan; Roberto Neri; Chunchong Ni; Aristeidis Noutsos; Hector Olivares; Gisela N. Ortiz-León; Feryal Özel; Daniel C. M. Palumbo; Nimesh A. Patel; Ue-Li Pen; Dominic W. Pesce; Richard L. Plambeck; Aleksandar Popstefanija; Oliver Porth; Ben Prather; Jorge A. Preciado-López; Dimitrios Psaltis; Hung Yi Pu; Venkatessh Ramakrishnan; Ramprasad Rao; Mark G. Rawlings; Alexander W. Raymond; Luciano Rezzolla; Bart Ripperda; Freek Roelofs; Alan E. E. Rogers; Eduardo Ros; Mel Rose; Arash Roshanineshat; Helge Rottmann; Alan L. Roy; Chet Ruszczyk; Benjamin R. Ryan; Kazi L.J. Rygl; David Sánchez-Arguelles; Mahito Sasada; Tuomas Savolainen; F. Peter Schloerb; Karl Friedrich Schuster; Lijing Shao; Zhiqiang Shen; Des Small; Bong Won Sohn; Jason SooHoo; Fumie Tazaki; Paul Tiede; Remo P. J. Tilanus; Michael Titus; Kenji Toma; Pablo Torne; Tyler Trent; Sascha Trippe; Ilse van Bemmel; Huib Jan van Langevelde; Daniel R. van Rossum; Jan Wagner; John Wardle; Jonathan Weintroub; Norbert Wex; Robert Wharton; Maciek Wielgus; George N. Wong; Qingwen Wu; André Young; Ken H. Young; Ziri Younsi; Feng Yuan; Ye-Fei Yuan; J. Anton Zensus; Guang-Yao Zhao; Shan Shan Zhao; Ziyan Zhu; Roger J. Cappallo; Joseph R. Farah; Thomas W. Folkers; Zheng Meyer-Zhao; Daniel Michalik; A. Nadolski; Hiroaki Nishioka; Nicolas Pradel; Rurik A. Primiani; Kamal Souccar; Paul Yamaguchi;Academy of Sciences (CAS, grants QYZDJ-SSW-SLH057, QYZDJ-SSW-SYS008); the Leverhulme Trust Early Career Research Fellowship; the Max-Planck-Gesellschaft (MPG); the Max Planck Partner Group of the MPG and the CAS; the MEXT/JSPS KAKENHI (grants 18KK0090, JP18K13594, JP18K03656, JP18H03721, 18K03709, 18H01245, 25120007); the MIT International Science and Technology Initiatives (MISTI) Funds; the Ministry of Science and Technology (MOST) of Taiwan (105-2112-M-001-025-MY3, 106-2112-M001-011, 106-2119-M-001-027, 107-2119-M-001-017, 107- 2119-M-001-020, and 107-2119-M-110-005); the National Aeronautics and Space Administration (NASA, Fermi Guest Investigator grant 80NSSC17K0649); the National Institute of Natural Sciences (NINS) of Japan; the National Key Research and Development Program of China (grant 2016YFA0400704, 2016YFA0400702); the National Science Foundation (NSF, grants AST-0096454, AST-0352953, AST-0521233, AST0705062, AST-0905844, AST-0922984, AST-1126433, AST1140030, DGE-1144085, AST-1207704, AST-1207730, AST1207752, MRI-1228509, OPP-1248097, AST-1310896, AST1312651, AST-1337663, AST-1440254, AST-1555365, AST1715061, AST-1615796, AST-1614868, AST-1716327, OISE1743747, AST-1816420); the Natural Science Foundation of China (grants 11573051, 11633006, 11650110427, 10625314, 11721303, 11725312, 11873028, 11873073, U1531245, 11473010); the Natural Sciences and Engineering Research Council of Canada (NSERC, including a Discovery Grant and the NSERC Alexander Graham Bell Canada Graduate Scholarships-Doctoral Program); the National Youth Thousand Talents Program of China; the National Research Foundation of Korea (grant 2015-R1D1A1A01056807, the Global PhD Fellowship Grant: NRF-2015H1A2A1033752, and the Korea Research Fellowship Program: NRF-2015H1D3A1066561); the Netherlands Organization for Scientific Research (NWO) VICI award (grant 639.043.513) and Spinoza Prize (SPI 78-409); the New Scientific Frontiers with Precision The authors of this Letter thank the following organizations and programs: the Academy of Finland (projects 274477, 284495, 312496); the Advanced European Network of E-infrastructures for Astronomy with the SKA (AENEAS) project, supported by the European Commission Framework Programme Horizon 2020 Research and Innovation action under grant agreement 731016; the Alexander von Humboldt Stiftung; the Black Hole Initiative at Harvard University, through a grant (60477) from the John Templeton Foundation; the China Scholarship Council; Comisión Nacional de Investigación Científica y Tecnológica (CONICYT, Chile, via PIA ACT172033, Fondecyt 1171506, BASAL AFB170002, ALMA-conicyt 31140007); Consejo Nacional de Ciencia y Tecnología (CONACYT, Mexico, projects 104497, 275201, 279006, 281692); the Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute; Dirección General de Asuntos del Personal Académico-Universidad Nacional 9 The Astrophysical Journal Letters, 875:L1 (17pp), 2019 April 10 The EHT Collaboration et al. Autónoma de México (DGAPA-UNAM, project IN112417); the European Research Council (ERC) Synergy Grant “BlackHoleCam: Imaging the Event Horizon of Black Holes” (grant 610058); the Generalitat Valenciana postdoctoral grant APOSTD/2018/177; the Gordon and Betty Moore Foundation (grants GBMF-3561, GBMF-5278); the Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV; the International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne; the Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO); the Japanese Government (Monbukagakusho: MEXT) Scholarship; the Japan Society for the Promotion of Science (JSPS) Grant-in-Aid for JSPS Research Fellowship (JP17J08829); JSPS Overseas Research Fellowships; the Key Research Program of Frontier Sciences, Chinese Radio Interferometry Fellowship awarded by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation (NRF), an agency of the Department of Science and Technology (DST) of South Africa; the Onsala Space Observatory (OSO) national infrastructure, for the provisioning of its facilities/observational support (OSO receives funding through the Swedish Research Council under grant 2017-00648); the Perimeter Institute for Theoretical Physics (research at Perimeter Institute is supported by the Government of Canada through the Department of Innovation, Science and Economic Development Canada and by the Province of Ontario through the Ministry of Economic Development, Job Creation and Trade); the Russian Science Foundation (grant 17-12-01029); the Spanish Ministerio de Economía y Competitividad (grants AYA2015-63939-C2-1-P, AYA2016-80889-P); the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709); the Toray Science Foundation; the US Department of Energy (USDOE) through the Los Alamos National Laboratory (operated by Triad National Security, LLC, for the National Nuclear Security Administration of the USDOE (Contract 89233218CNA000001)); the Italian Ministero dell’Istruzione Università e Ricerca through the grant Progetti Premiali 2012-iALMA (CUP C52I13000140001); the European Unionʼs Horizon 2020 research and innovation programme under grant agreement No 730562 RadioNet; ALMA North America Development Fund; Chandra TM6-17006X We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ~1 mJy on baselines to ALMA and ~10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, wide recording bandwidth, and highly heterogeneous array. In response, we developed three independent pipelines for phase calibration and fringe detection, each tailored to the specific needs of the EHT. The final data products include calibrated total intensity amplitude and phase information. They are validated through a series of quality assurance tests that show consistency across pipelines and set limits on baseline systematic errors of 2% in amplitude and 1° in phase. The M87 data reveal the presence of two nulls in correlated flux density at ~3.4 and ~8.3 Gλ and temporal evolution in closure quantities, indicating intrinsic variability of compact structure on a timescale of days, or several light-crossing times for a few billion solar-mass black hole. These measurements provide the first opportunity to image horizon-scale structure in M87.© 2019. The American Astronomical Society Peer reviewed
NARCIS arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019The Astrophysical Journal LettersArticle . 2019Radboud Repository; The Astrophysical Journal LettersArticle . 2019Aaltodoc Publication ArchiveArticle . 2019 . Peer-reviewedData sources: Aaltodoc Publication ArchiveOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019 . Peer-reviewedThe Astrophysical Journal; The Astrophysical Journal LettersArticle . 2019 . Peer-reviewedLicense: CC BYarXiv.org e-Print ArchiveOther literature type . Preprint . 2019Data sources: arXiv.org e-Print ArchiveHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab0c57&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 504 citations 504 popularity Top 0.1% influence Top 1% impulse Top 0.01% Powered by BIP!visibility 30visibility views 30 download downloads 32 Powered bymore_vert NARCIS arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019The Astrophysical Journal LettersArticle . 2019Radboud Repository; The Astrophysical Journal LettersArticle . 2019Aaltodoc Publication ArchiveArticle . 2019 . Peer-reviewedData sources: Aaltodoc Publication ArchiveOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019 . Peer-reviewedThe Astrophysical Journal; The Astrophysical Journal LettersArticle . 2019 . Peer-reviewedLicense: CC BYarXiv.org e-Print ArchiveOther literature type . Preprint . 2019Data sources: arXiv.org e-Print ArchiveHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab0c57&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2018 FrancePublisher:IOP Publishing Funded by:EC | TESTDE, EC | COGS, EC | COSMICDAWN +3 projectsEC| TESTDE ,EC| COGS ,EC| COSMICDAWN ,NSF| Sustained-Petascale In Action: Blue Waters Enabling Transformative Science And Engineering ,NSF| Leadership Class Scientific and Engineering Computing: Breaking Through the Limits ,NSF| Collaborative Research: The Dark Energy Survey Data Management OperationsEric Morganson; Robert A. Gruendl; Felipe Menanteau; M. Carrasco Kind; Y.-C. Chen; G. Daues; Alex Drlica-Wagner; Douglas N. Friedel; M. Gower; M. W. G. Johnson; M. D. Johnson; Richard Kessler; F. Paz-Chinchón; Don Petravick; C. Pond; Brian Yanny; S. Allam; Robert Armstrong; Wayne A. Barkhouse; Keith Bechtol; A. Benoit-Lévy; Gary Bernstein; E. Bertin; E. Buckley-Geer; R. Covarrubias; Shantanu Desai; H. T. Diehl; Daniel A. Goldstein; Daniel Gruen; T. S. Li; Huan Lin; J. P. Marriner; Joseph J. Mohr; Eric H. Neilsen; Chow-Choong Ngeow; K. Paech; Eli S. Rykoff; M. Sako; I. Sevilla-Noarbe; Erin Sheldon; Flavia Sobreira; Douglas L. Tucker; W. C. Wester;International audience; The Dark Energy Survey (DES) is a five-year optical imaging campaign with the goal of understanding the origin of cosmic acceleration. DES performs a 5000 square degree survey of the southern sky in five optical bands (g,r,i,z,Y) to a depth of ~24th magnitude. Contemporaneously, DES performs a deep, time-domain survey in four optical bands (g,r,i,z) over 27 square degrees. DES exposures are processed nightly with an evolving data reduction pipeline and evaluated for image quality to determine if they need to be retaken. Difference imaging and transient source detection are also performed in the time domain component nightly. On a bi-annual basis, DES exposures are reprocessed with a refined pipeline and coadded to maximize imaging depth. Here we describe the DES image processing pipeline in support of DES science, as a reference for users of archival DES data, and as a guide for future astronomical surveys.
arXiv.org e-Print Ar... arrow_drop_down arXiv.org e-Print ArchiveOther literature type . Preprint . 2018Data sources: arXiv.org e-Print ArchivePublications of the Astronomical Society of the PacificArticle . 2018 . Peer-reviewedLicense: IOP Copyright PoliciesData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1538-3873/aab4ef&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 166 citations 166 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down arXiv.org e-Print ArchiveOther literature type . Preprint . 2018Data sources: arXiv.org e-Print ArchivePublications of the Astronomical Society of the PacificArticle . 2018 . Peer-reviewedLicense: IOP Copyright PoliciesData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1538-3873/aab4ef&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2016 FrancePublisher:Public Library of Science (PLoS) Vincent Lesieur; Jean-François Martin; David K. Weaver; Kim A. Hoelmer; David R. Smith; Wendell L. Morrill; N. Kadiri; Frank B. Peairs; Darren M. Cockrell; Terri L. Randolph; Debra K. Waters; Marie-Claude Bon;The wheat stem sawfly, Cephus cinctus Norton (Hymenoptera: Cephidae), is a key pest of wheat in the northern Great Plains of North America, and damage resulting from this species has recently expanded southward. Current pest management practices are inadequate and uncertainty regarding geographic origin, as well as limited data on population structure and dynamics across North America impede progress towards more informed management. We examined the genetic divergence between samples collected in North America and northeastern Asia, the assumed native range of C. cinctus using two mitochondrial regions (COI and 16S). Subsequently, we characterized the structure of genetic diversity in the main wheat producing areas in North America using a combination of mtDNA marker and micro-satellites in samples collected both in wheat fields and in grasses in wildlands. The strong genetic divergence observed between North American samples and Asian congeners, in particular the synonimized C. hyalinatus, did not support the hypothesis of a recent Ameri-can colonization by C. cinctus. Furthermore, the relatively high genetic diversity both with mtDNA and microsatellite markers offered additional evidence in favor of the native Ameri-can origin of this pest. The genetic diversity of North American populations is structured into three genetic clusters and these are highly correlated with geography. Regarding the recent southern outbreaks in North America, the results tend to exclude the hypothesis of recent movement of damaging wheat stem sawfly populations from the northern area. The shift in host plant use by local populations appears to be the most likely scenario. Finally, the significance of these findings is discussed in the context of pest management. International audience
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2016Full-Text: http://europepmc.org/articles/PMC5154603Data sources: PubMed Centraladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0168370&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 36 citations 36 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2016Full-Text: http://europepmc.org/articles/PMC5154603Data sources: PubMed Centraladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0168370&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2015 Netherlands, United Kingdom, Italy, France, Italy, Netherlands, Netherlands, United StatesPublisher:American Astronomical Society ALMA Partnership; E. B. Fomalont; C. Vlahakis; S. Corder; A. Remijan; D. Barkats; R. Lucas; T. R. Hunter; C. L. Brogan; Y. Asaki; S. Matsushita; W. R. F. Dent; R. E. Hills; N. Phillips; A. M. S. Richards; P. Cox; R. Amestica; D. Broguiere; W. Cotton; A. S. Hales; R. Hiriart; A. Hirota; J. A. Hodge; C. M. V. Impellizzeri; J. Kern; R. Kneissl; E. Liuzzo; N. Marcelino; R. Marson; A. Mignano; K. Nakanishi; B. Nikolic; J. E. Perez; L. M. Pérez; I. Toledo; R. Aladro; B. Butler; J. Cortes; P. Cortes; V. Dhawan; J. Di Francesco; D. Espada; F. Galarza; D. Garcia-Appadoo; L. Guzman-Ramirez; E. M. Humphreys; T. Jung; S. Kameno; R. A. Laing; S. Leon; J. Mangum; G. Marconi; H. Nagai; L.-A. Nyman; M. Radiszcz; J. A. Rodón; T. Sawada; S. Takahashi; R. P. J. Tilanus; T. van Kempen; B. Vila Vilaro; L. C. Watson; T. Wiklind; F. Gueth; K. Tatematsu; A. Wootten; A. Castro-Carrizo; E. Chapillon; G. Dumas; I. de Gregorio-Monsalvo; H. Francke; J. Gallardo; J. Garcia; S. Gonzalez; J. E. Hibbard; T. Hill; T. Kaminski; A. Karim; M. Krips; Y. Kurono; C. Lopez; S. Martin; L. Maud; F. Morales; V. Pietu; K. Plarre; G. Schieven; L. Testi; L. Videla; E. Villard; N. Whyborn; M. A. Zwaan; F. Alves; P. Andreani; A. Avison; M. Barta; F. Bedosti; G. J. Bendo; F. Bertoldi; M. Bethermin; A. Biggs; J. Boissier; J. Brand; S. Burkutean; V. Casasola; J. Conway; L. Cortese; B. Dabrowski; T. A. Davis; M. Diaz Trigo; F. Fontani; R. Franco-Hernandez; G. Fuller; R. Galvan Madrid; A. Giannetti; A. Ginsburg; S. F. Graves; E. Hatziminaoglou; M. Hogerheijde; P. Jachym; I. Jimenez Serra; M. Karlicky; P. Klaasen; M. Kraus; D. Kunneriath; C. Lagos; S. Longmore; S. Leurini; M. Maercker; B. Magnelli; I. Marti Vidal; M. Massardi; A. Maury; S. Muehle; S. Muller; T. Muxlow; E. O’Gorman; R. Paladino; D. Petry; J. Pineda; S. Randall; J. S. Richer; A. Rossetti; A. Rushton; K. Rygl; A. Sanchez Monge; R. Schaaf; P. Schilke; T. Stanke; M. Schmalzl; F. Stoehr; S. Urban; E. van Kampen; W. Vlemmings; K. Wang; W. Wild; Y. Yang; S. Iguchi; T. Hasegawa; M. Saito; J. Inatani; N. Mizuno; S. Asayama; G. Kosugi; K.-I. Morita; K. Chiba; S. Kawashima; S. K. Okumura; N. Ohashi; R. Ogasawara; S. Sakamoto; T. Noguchi; Y.-D. Huang; S.-Y. Liu; F. Kemper; P. M. Koch; M.-T. Chen; Y. Chikada; M. Hiramatsu; D. Iono; M. Shimojo; S. Komugi; J. Kim; A.-R. Lyo; E. Muller; C. Herrera; R. E. Miura; J. Ueda; J. Chibueze; Y.-N. Su; A. Trejo-Cruz; K.-S. Wang; H. Kiuchi; N. Ukita; M. Sugimoto; R. Kawabe; M. Hayashi; S. Miyama; P. T. P. Ho; N. Kaifu;Accepted: 2015-04-10 資料番号: SA1150145000 著者人数: 248名
CORE (RIOXX-UK Aggre... arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2015 . Peer-reviewedLicense: IOP Copyright PoliciesOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2015Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/2041-8205/808/1/l1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 65 citations 65 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!visibility 48visibility views 48 download downloads 47 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2015 . Peer-reviewedLicense: IOP Copyright PoliciesOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2015Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/2041-8205/808/1/l1&type=result"></script>'); --> </script>
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description Publicationkeyboard_double_arrow_right Article 2018 FrancePublisher:Public Library of Science (PLoS) Funded by:ANR | CRB-AnimANR| CRB-AnimYi-Chen Chen; Wei-Che Chang; Shau-Ping Lin; Masataka Minami; Christian Jean; Hisato Hayashi; Sylvie Rival-Gervier; Tatsuro Kanaki; Shinn-Chih Wu; Bertrand Pain;Scalable production of avian cell lines exhibits a valuable potential on therapeutic application by producing recombinant proteins and as the substrate for virus growth due to the special glycosylation occurs in avian species. Chicken primordial germ cells (cPGCs), a germinal pluripotent avian cell type, present the ability of self-renewal, an anchorage-independent cell growth and the ability to be genetically modified. This cell type could be an interesting bioreactor system for industrial purposes. This study sought to establish an expandable culture system with defined components for three-dimensional (3D) culture of cPGCs. cPGCs were cultured in medium supplemented with the functional polymer FP003. Viscoelasticity was low in this medium but cPGCs did not sediment in culture and efficiencies of space and nutrient utilization were thus enhanced and consequently their expansion was improved. The total number of cPGCs increased by 17-fold after 1 week of culture in 3D-FAot medium, an aseric defined medium containing FP003 polymer, FGF2 and Activin A as growth factors and Ovotransferrin as protein. Moreover, cPGC cell lines stably expressed the germline-specific reporter VASA:tdTOMATO, as well as other markers of cPGCs, for more than 1 month upon culture in 3D-FAot medium, indicating that the characteristics of these cells are maintained. In summary, this novel 3D culture system can be used to efficiently expand cPGCs in suspension without mechanical stirring, which is available for long-term culture and no loss of cellular properties was found. This system provides a platform for large-scale culture of cPGCs.
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6150485Data sources: PubMed CentralMémoires en Sciences de l'Information et de la CommunicationArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01906546/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0200515&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 11 citations 11 popularity Top 10% influence Average impulse Average Powered by BIP!more_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6150485Data sources: PubMed CentralMémoires en Sciences de l'Information et de la CommunicationArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01906546/documentadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0200515&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2007 United States, FrancePublisher:American Geophysical Union (AGU) Martine Simoes; Jean Philippe Avouac; Olivier Beyssac; Bruno Goffé; Kenneth A. Farley; Yue-Gau Chen;doi: 10.1029/2006jb004824
The Taiwan mountain belt is classically viewed as a case example of a critical wedge growing essentially by frontal accretion and therefore submitted to distributed shortening. However, a number of observations call for a significant contribution of underplating to the growth of the orogenic wedge. We propose here a new thermokinematic model of the Taiwan mountain belt reconciling existing kinematic, thermometric and thermochronological constraints. In this model, shortening across the orogen is absorbed by slip on the most frontal faults of the foothills. Crustal thickening and exhumation are sustained by underplating beneath the easternmost portion of the wedge (Tananao Complex, TC), where the uplift rate is estimated to 6.3 mm a1, and beneath the westernmost internal region of the orogen (Hsueshan Range units, HR), where the uplift rate is estimated to 4.2 mm a1. Our model suggests that the TC units experienced a synchronous evolution along strike despite the southward propagation of the collision. It also indicates that they have reached a steady state in terms of cooling ages but not in terms of peak metamorphic temperatures. Exhumation of the HR units increases northward but has not yet reached an exhumational steady state. Presently, frontal accretion accounts for less than 10% of the incoming flux of material into the orogen, although there is indication that it was contributing substantially more (80%) before 4 Ma. The incoming flux of material accreted beneath the TC significantly increased 1.5 Ma ago. Our results also suggest that the flux of material accreted to the orogen corresponds to the top 7 km of the upper crust of the underthrust Chinese margin. This indicates that a significant amount (76%) of the underthrust material has been subducted into the mantle, probably because of the increase in density associated with metamorphism. We also show that the density distribution resulting from metamorphism within the orogenic wedge explains well the topography and the gravity field. By combining available geological data on the thermal and kinematic evolution of the wedge, our study sheds new light onto mountain building processes in Taiwan and allows for reappraising the initial structural architecture of the passive margin. International audience
HAL-Rennes 1; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2007 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-Rennes 1; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2007add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2006jb004824&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess Routesbronze 93 citations 93 popularity Top 10% influence Top 10% impulse Top 10% Powered by BIP!visibility 1visibility views 1 Powered bymore_vert HAL-Rennes 1; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2007 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-Rennes 1; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2007add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1029/2006jb004824&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article , Other literature type 2018 FrancePublisher:Public Library of Science (PLoS) Authors: Callet, Thérèse; Dupont-Nivet, Mathilde; Cluzeaud, Marianne; Jaffrezic, Florence; +8 AuthorsCallet, Thérèse; Dupont-Nivet, Mathilde; Cluzeaud, Marianne; Jaffrezic, Florence; Laloë, Denis; Kerneis, Thierry; Labbé, Laurent; Quillet, Edwige; Geurden, Inge; Mazurais, David; Skiba-Cassy, Sandrine; Médale, Françoise;To meet the growing demand of fish feed for aquaculture, an increasing proportion of marine ingredients are being replaced by blends of plant products. However, the total replacement of marine ingredients in salmonid diets impairs fish performance. This is particularly true during the early fry stage and this stage is therefore considered of particular importance. In rainbow trout (RBT), the existence of a genetic variability to survive and grow with plant-based diets devoid of marine ingredients has now been proved, but the mechanisms behind are little studied especially at early stage. To investigate these, we analysed the whole transcriptome of three isogenic lines of RBT fry, which have similar growth when fed a marine resources-based diet (M diet) but which highly differ in their responses to a plant-based diet (V diet). Analysis of transcriptomes profiles revealed 1740, 1834 and 246 probes differentially expressed among the three genotypes when fed the V diet. The use of these lines led to the discovery of potential molecular markers linked to plant-based diet utilisation, some of them belonging to new pathways, never described before. An important number of genes was related to immunity, but further investigations are needed to better understand the difference between the genotypes in their immune status response to V diet exposure. Finally, differences in expression of genes related to feed intake and sensory perception among genotypes suggested that the mechanisms underlying the differences in growth on plant-based diet are closely linked to diet acceptance. Research on plants components affecting feed intake should be thus further explored. Unités expérimentales PEIMA et NuMeA-Donzacq International audience
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6067751Data sources: PubMed CentralArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01857986/documentArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of Ifremeradd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0201462&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 13 citations 13 popularity Top 10% influence Average impulse Top 10% Powered by BIP!visibility 10visibility views 10 download downloads 1 Powered bymore_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2018Full-Text: http://europepmc.org/articles/PMC6067751Data sources: PubMed CentralArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of IfremerMémoires en Sciences de l'Information et de la Communication; HAL-IRDArticle . 2018License: CC BYFull-Text: https://hal.science/hal-01857986/documentArchiMer - Institutional Archive of IfremerOther literature type . 2018Data sources: ArchiMer - Institutional Archive of Ifremeradd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0201462&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2010 FrancePublisher:American Geophysical Union (AGU) Authors: Sebastien Boutareaud; Anne-Marie Boullier; Muriel Andreani; Dan-Gabriel Calugaru; +3 AuthorsSebastien Boutareaud; Anne-Marie Boullier; Muriel Andreani; Dan-Gabriel Calugaru; Pierre Beck; Sheng-Rong Song; Toshihiko Shimamoto;doi: 10.1029/2008jb006254
Spherical aggregates named clay-clast aggregates (CCAs) have been reported from recent investigations on retrieved clay-bearing fault gouges from shallow depth seismogenic faults and rotary shear experiments conducted on clay-bearing gouge at seismic slip rates. The formation of CCAs appears to be related to the shearing of a smectite-rich granular material that expands and becomes fluidized. We have conducted additional high-velocity rotary shear experiments and low-velocity double-shear experiments. We demonstrate that a critical temperature depending on dynamic pressure-temperature conditions is needed for the formation of CCAs. This temperature corresponds to the phase transition of pore water from liquid to vapor or to critical, which induced gouge pore fluid expansion and therefore a thermal pressurization of the fault. A detailed examination by energy dispersive X-ray spectrometry (EDX-SEM) element mapping, SEM, and transmission electron microscopy (TEM) shows strong similar characteristics of experimental and natural CCAs with a concentric well-organized fabric of the cortex and reveals that their development may result from the combination of electrostatic and capillary forces in a critical reactive medium during the dynamic slip weakening. Accordingly, the occurrence of CCAs in natural clay-rich fault gouges constitutes new unequivocal textural evidence for shallow depth thermal pressurization and consequently for past seismic faulting. International audience
HAL-ENS-LYON; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2010 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-ENS-LYON; Hal-DiderotArticle . 2010HAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2010add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.euAccess Routesbronze 104 citations 104 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!more_vert HAL-ENS-LYON; Mémoir... arrow_drop_down Journal of Geophysical Research AtmospheresArticle . 2010 . Peer-reviewedLicense: Wiley Online Library User AgreementData sources: CrossrefHAL-ENS-LYON; Hal-DiderotArticle . 2010HAL - UPEC / UPEM; HAL-Pasteur; HAL-InsermArticle . 2010add ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2019 France, Netherlands, Netherlands, Netherlands, United Kingdom, Netherlands, Italy, Italy, United States, Netherlands, Finland, Japan, Spain, NetherlandsPublisher:American Astronomical Society Funded by:NSF | Center for Cosmological P..., NSERC, NSF | Graduate Research Fellows... +15 projectsNSF| Center for Cosmological Physics ,NSERC ,NSF| Graduate Research Fellowship Program (GRFP) ,EC| BLACKHOLECAM ,NSF| Physics Frontier Center at the Kavli Institute for Cosmological Physics: Pushing Cosmology to the Edge ,NSF| The Arizona Radio Observatory: Surveying the ISM through Millimeter and Sub-millimeter Spectroscopy ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,NSF| Cosmological Research with the 10-meter South Pole Telescope ,NSF| PSCIC Full Proposal: The iPlant Collaborative: A Cyberinfrastructure-Centered Community for a New Plant Biology ,NWO| From micro- to mega-scales: understanding how black holes shape the local Universe ,AKA| Physics of Black Hole-Powered Jets ,NSF| The iPlant Collaborative: Cyberinfrastructure for the Life Sciences ,EC| AENEAS ,NSF| CyVerse: Cyberinfrastructure for the Life Sciences ,NSF| Collaborative Research: Building an Event Horizon Telescope: (Sub)millimeter VLBI from the South Pole Telescope ,NSF| MRI: Development of an ALMA Beamformer for Ultra High Resolution VLBI and High Frequency Phased Array Science ,EC| RadioNet ,AKA| Physics of Black Hole-Powered JetsKazunori Akiyama; Antxon Alberdi; Walter Alef; Keiichi Asada; Rebecca Azulay; Anne Kathrin Baczko; David Ball; Mislav Baloković; John E. Barrett; Dan Bintley; Lindy Blackburn; W. Boland; Katherine L. Bouman; Geoffrey C. Bower; Michael Bremer; Christiaan D. Brinkerink; Roger Brissenden; Silke Britzen; Avery E. Broderick; Thomas Bronzwaer; Do-Young Byun; Andrew Chael; Chi-kwan Chan; Shami Chatterjee; Koushik Chatterjee; Ming-Tang Chen; Yi Chen; Ilje Cho; Pierre Christian; John Conway; James M. Cordes; Geoffrey B. Crew; Yuzhu Cui; Jordy Davelaar; Mariafelicia De Laurentis; Roger Deane; Jessica Dempsey; Gregory Desvignes; Jason Dexter; Sheperd S. Doeleman; R. P. Eatough; Heino Falcke; Vincent L. Fish; Ed Fomalont; Raquel Fraga-Encinas; Per Friberg; José L. Gómez; Peter Galison; Charles F. Gammie; Roberto Garcia; Olivier Gentaz; Boris Georgiev; Ciriaco Goddi; Roman Gold; Minfeng Gu; Mark Gurwell; Kazuhiro Hada; Michael H. Hecht; Ronald Hesper; Luis C. Ho; Paul T. P. Ho; Mareki Honma; Chih-Wei Locutus Huang; Lei Huang; David H. Hughes; Shiro Ikeda; Makoto Inoue; Sara Issaoun; David J. James; Buell T. Jannuzi; Michael Janssen; Britton Jeter; Wu Jiang; Michael D. Johnson; Svetlana G. Jorstad; Taehyun Jung; Mansour Karami; Ramesh Karuppusamy; Tomohisa Kawashima; Garrett K. Keating; Mark Kettenis; Jae-Young Kim; Junhan Kim; Motoki Kino; Jun Yi Koay; Patrick M. Koch; Shoko Koyama; Michael Kramer; Carsten Kramer; Thomas P. Krichbaum; C. Y. Kuo; Tod R. Lauer; Sang-Sung Lee; Yan-Rong Li; Zhiyuan Li; Michael Lindqvist; Kuo Liu; Elisabetta Liuzzo; Andrei P. Lobanov; Laurent Loinard; Colin J. Lonsdale; Ru-Sen Lu; Nicholas R. MacDonald; Jirong Mao; Sera Markoff; Daniel P. Marrone; Alan P. Marscher; Satoki Matsushita; Lynn D. Matthews; Lia Medeiros; Karl M. Menten; Yosuke Mizuno; Izumi Mizuno; James M. Moran; Kotaro Moriyama; Monika Moscibrodzka; Cornelia Müller; Hiroshi Nagai; Neil M. Nagar; Masanori Nakamura; Ramesh Narayan; Gopal Narayanan; Iniyan Natarajan; Roberto Neri; Chunchong Ni; Aristeidis Noutsos; Hector Olivares; Gisela N. Ortiz-León; Feryal Özel; Daniel C. M. Palumbo; Nimesh A. Patel; Ue-Li Pen; Dominic W. Pesce; Richard L. Plambeck; Aleksandar Popstefanija; Oliver Porth; Ben Prather; Jorge A. Preciado-López; Dimitrios Psaltis; Hung Yi Pu; Venkatessh Ramakrishnan; Ramprasad Rao; Mark G. Rawlings; Alexander W. Raymond; Luciano Rezzolla; Bart Ripperda; Freek Roelofs; Alan E. E. Rogers; Eduardo Ros; Mel Rose; Arash Roshanineshat; Helge Rottmann; Alan L. Roy; Chet Ruszczyk; Benjamin R. Ryan; Kazi L.J. Rygl; David Sánchez-Arguelles; Mahito Sasada; Tuomas Savolainen; F. Peter Schloerb; Karl Friedrich Schuster; Lijing Shao; Zhiqiang Shen; Des Small; Bong Won Sohn; Jason SooHoo; Fumie Tazaki; Paul Tiede; Remo P. J. Tilanus; Michael Titus; Kenji Toma; Pablo Torne; Tyler Trent; Sascha Trippe; Ilse van Bemmel; Huib Jan van Langevelde; Daniel R. van Rossum; Jan Wagner; John Wardle; Jonathan Weintroub; Norbert Wex; Robert Wharton; Maciek Wielgus; George N. Wong; Qingwen Wu; André Young; Ken H. Young; Ziri Younsi; Feng Yuan; Ye-Fei Yuan; J. Anton Zensus; Guang-Yao Zhao; Shan Shan Zhao; Ziyan Zhu; Roger J. Cappallo; Joseph R. Farah; Thomas W. Folkers; Zheng Meyer-Zhao; Daniel Michalik; A. Nadolski; Hiroaki Nishioka; Nicolas Pradel; Rurik A. Primiani; Kamal Souccar; Paul Yamaguchi;Academy of Sciences (CAS, grants QYZDJ-SSW-SLH057, QYZDJ-SSW-SYS008); the Leverhulme Trust Early Career Research Fellowship; the Max-Planck-Gesellschaft (MPG); the Max Planck Partner Group of the MPG and the CAS; the MEXT/JSPS KAKENHI (grants 18KK0090, JP18K13594, JP18K03656, JP18H03721, 18K03709, 18H01245, 25120007); the MIT International Science and Technology Initiatives (MISTI) Funds; the Ministry of Science and Technology (MOST) of Taiwan (105-2112-M-001-025-MY3, 106-2112-M001-011, 106-2119-M-001-027, 107-2119-M-001-017, 107- 2119-M-001-020, and 107-2119-M-110-005); the National Aeronautics and Space Administration (NASA, Fermi Guest Investigator grant 80NSSC17K0649); the National Institute of Natural Sciences (NINS) of Japan; the National Key Research and Development Program of China (grant 2016YFA0400704, 2016YFA0400702); the National Science Foundation (NSF, grants AST-0096454, AST-0352953, AST-0521233, AST0705062, AST-0905844, AST-0922984, AST-1126433, AST1140030, DGE-1144085, AST-1207704, AST-1207730, AST1207752, MRI-1228509, OPP-1248097, AST-1310896, AST1312651, AST-1337663, AST-1440254, AST-1555365, AST1715061, AST-1615796, AST-1614868, AST-1716327, OISE1743747, AST-1816420); the Natural Science Foundation of China (grants 11573051, 11633006, 11650110427, 10625314, 11721303, 11725312, 11873028, 11873073, U1531245, 11473010); the Natural Sciences and Engineering Research Council of Canada (NSERC, including a Discovery Grant and the NSERC Alexander Graham Bell Canada Graduate Scholarships-Doctoral Program); the National Youth Thousand Talents Program of China; the National Research Foundation of Korea (grant 2015-R1D1A1A01056807, the Global PhD Fellowship Grant: NRF-2015H1A2A1033752, and the Korea Research Fellowship Program: NRF-2015H1D3A1066561); the Netherlands Organization for Scientific Research (NWO) VICI award (grant 639.043.513) and Spinoza Prize (SPI 78-409); the New Scientific Frontiers with Precision The authors of this Letter thank the following organizations and programs: the Academy of Finland (projects 274477, 284495, 312496); the Advanced European Network of E-infrastructures for Astronomy with the SKA (AENEAS) project, supported by the European Commission Framework Programme Horizon 2020 Research and Innovation action under grant agreement 731016; the Alexander von Humboldt Stiftung; the Black Hole Initiative at Harvard University, through a grant (60477) from the John Templeton Foundation; the China Scholarship Council; Comisión Nacional de Investigación Científica y Tecnológica (CONICYT, Chile, via PIA ACT172033, Fondecyt 1171506, BASAL AFB170002, ALMA-conicyt 31140007); Consejo Nacional de Ciencia y Tecnología (CONACYT, Mexico, projects 104497, 275201, 279006, 281692); the Delaney Family via the Delaney Family John A. Wheeler Chair at Perimeter Institute; Dirección General de Asuntos del Personal Académico-Universidad Nacional 9 The Astrophysical Journal Letters, 875:L1 (17pp), 2019 April 10 The EHT Collaboration et al. Autónoma de México (DGAPA-UNAM, project IN112417); the European Research Council (ERC) Synergy Grant “BlackHoleCam: Imaging the Event Horizon of Black Holes” (grant 610058); the Generalitat Valenciana postdoctoral grant APOSTD/2018/177; the Gordon and Betty Moore Foundation (grants GBMF-3561, GBMF-5278); the Istituto Nazionale di Fisica Nucleare (INFN) sezione di Napoli, iniziative specifiche TEONGRAV; the International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne; the Jansky Fellowship program of the National Radio Astronomy Observatory (NRAO); the Japanese Government (Monbukagakusho: MEXT) Scholarship; the Japan Society for the Promotion of Science (JSPS) Grant-in-Aid for JSPS Research Fellowship (JP17J08829); JSPS Overseas Research Fellowships; the Key Research Program of Frontier Sciences, Chinese Radio Interferometry Fellowship awarded by the South African Radio Astronomy Observatory (SARAO), which is a facility of the National Research Foundation (NRF), an agency of the Department of Science and Technology (DST) of South Africa; the Onsala Space Observatory (OSO) national infrastructure, for the provisioning of its facilities/observational support (OSO receives funding through the Swedish Research Council under grant 2017-00648); the Perimeter Institute for Theoretical Physics (research at Perimeter Institute is supported by the Government of Canada through the Department of Innovation, Science and Economic Development Canada and by the Province of Ontario through the Ministry of Economic Development, Job Creation and Trade); the Russian Science Foundation (grant 17-12-01029); the Spanish Ministerio de Economía y Competitividad (grants AYA2015-63939-C2-1-P, AYA2016-80889-P); the State Agency for Research of the Spanish MCIU through the “Center of Excellence Severo Ochoa” award for the Instituto de Astrofísica de Andalucía (SEV-2017-0709); the Toray Science Foundation; the US Department of Energy (USDOE) through the Los Alamos National Laboratory (operated by Triad National Security, LLC, for the National Nuclear Security Administration of the USDOE (Contract 89233218CNA000001)); the Italian Ministero dell’Istruzione Università e Ricerca through the grant Progetti Premiali 2012-iALMA (CUP C52I13000140001); the European Unionʼs Horizon 2020 research and innovation programme under grant agreement No 730562 RadioNet; ALMA North America Development Fund; Chandra TM6-17006X We present the calibration and reduction of Event Horizon Telescope (EHT) 1.3 mm radio wavelength observations of the supermassive black hole candidate at the center of the radio galaxy M87 and the quasar 3C 279, taken during the 2017 April 5–11 observing campaign. These global very long baseline interferometric observations include for the first time the highly sensitive Atacama Large Millimeter/submillimeter Array (ALMA); reaching an angular resolution of 25 μas, with characteristic sensitivity limits of ~1 mJy on baselines to ALMA and ~10 mJy on other baselines. The observations present challenges for existing data processing tools, arising from the rapid atmospheric phase fluctuations, wide recording bandwidth, and highly heterogeneous array. In response, we developed three independent pipelines for phase calibration and fringe detection, each tailored to the specific needs of the EHT. The final data products include calibrated total intensity amplitude and phase information. They are validated through a series of quality assurance tests that show consistency across pipelines and set limits on baseline systematic errors of 2% in amplitude and 1° in phase. The M87 data reveal the presence of two nulls in correlated flux density at ~3.4 and ~8.3 Gλ and temporal evolution in closure quantities, indicating intrinsic variability of compact structure on a timescale of days, or several light-crossing times for a few billion solar-mass black hole. These measurements provide the first opportunity to image horizon-scale structure in M87.© 2019. The American Astronomical Society Peer reviewed
NARCIS arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019The Astrophysical Journal LettersArticle . 2019Radboud Repository; The Astrophysical Journal LettersArticle . 2019Aaltodoc Publication ArchiveArticle . 2019 . Peer-reviewedData sources: Aaltodoc Publication ArchiveOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019 . Peer-reviewedThe Astrophysical Journal; The Astrophysical Journal LettersArticle . 2019 . Peer-reviewedLicense: CC BYarXiv.org e-Print ArchiveOther literature type . Preprint . 2019Data sources: arXiv.org e-Print ArchiveHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.3847/2041-8213/ab0c57&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 504 citations 504 popularity Top 0.1% influence Top 1% impulse Top 0.01% Powered by BIP!visibility 30visibility views 30 download downloads 32 Powered bymore_vert NARCIS arrow_drop_down NARCIS; Radboud RepositoryArticle . 2019The Astrophysical Journal LettersArticle . 2019Radboud Repository; The Astrophysical Journal LettersArticle . 2019Aaltodoc Publication ArchiveArticle . 2019 . Peer-reviewedData sources: Aaltodoc Publication ArchiveOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2019Data sources: OA@INAF - Istituto Nazionale di AstrofisicaRecolector de Ciencia Abierta, RECOLECTA; DIGITAL.CSICArticle . 2019 . Peer-reviewedThe Astrophysical Journal; The Astrophysical Journal LettersArticle . 2019 . Peer-reviewedLicense: CC BYarXiv.org e-Print ArchiveOther literature type . Preprint . 2019Data sources: arXiv.org e-Print ArchiveHAL - UPEC / UPEM; HAL-Pasteur; HAL-Inserm; Hal-DiderotArticle . 2019https://doi.org/10.48550/arxiv...Article . 2019License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2018 FrancePublisher:IOP Publishing Funded by:EC | TESTDE, EC | COGS, EC | COSMICDAWN +3 projectsEC| TESTDE ,EC| COGS ,EC| COSMICDAWN ,NSF| Sustained-Petascale In Action: Blue Waters Enabling Transformative Science And Engineering ,NSF| Leadership Class Scientific and Engineering Computing: Breaking Through the Limits ,NSF| Collaborative Research: The Dark Energy Survey Data Management OperationsEric Morganson; Robert A. Gruendl; Felipe Menanteau; M. Carrasco Kind; Y.-C. Chen; G. Daues; Alex Drlica-Wagner; Douglas N. Friedel; M. Gower; M. W. G. Johnson; M. D. Johnson; Richard Kessler; F. Paz-Chinchón; Don Petravick; C. Pond; Brian Yanny; S. Allam; Robert Armstrong; Wayne A. Barkhouse; Keith Bechtol; A. Benoit-Lévy; Gary Bernstein; E. Bertin; E. Buckley-Geer; R. Covarrubias; Shantanu Desai; H. T. Diehl; Daniel A. Goldstein; Daniel Gruen; T. S. Li; Huan Lin; J. P. Marriner; Joseph J. Mohr; Eric H. Neilsen; Chow-Choong Ngeow; K. Paech; Eli S. Rykoff; M. Sako; I. Sevilla-Noarbe; Erin Sheldon; Flavia Sobreira; Douglas L. Tucker; W. C. Wester;International audience; The Dark Energy Survey (DES) is a five-year optical imaging campaign with the goal of understanding the origin of cosmic acceleration. DES performs a 5000 square degree survey of the southern sky in five optical bands (g,r,i,z,Y) to a depth of ~24th magnitude. Contemporaneously, DES performs a deep, time-domain survey in four optical bands (g,r,i,z) over 27 square degrees. DES exposures are processed nightly with an evolving data reduction pipeline and evaluated for image quality to determine if they need to be retaken. Difference imaging and transient source detection are also performed in the time domain component nightly. On a bi-annual basis, DES exposures are reprocessed with a refined pipeline and coadded to maximize imaging depth. Here we describe the DES image processing pipeline in support of DES science, as a reference for users of archival DES data, and as a guide for future astronomical surveys.
arXiv.org e-Print Ar... arrow_drop_down arXiv.org e-Print ArchiveOther literature type . Preprint . 2018Data sources: arXiv.org e-Print ArchivePublications of the Astronomical Society of the PacificArticle . 2018 . Peer-reviewedLicense: IOP Copyright PoliciesData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1538-3873/aab4ef&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen bronze 166 citations 166 popularity Top 1% influence Top 10% impulse Top 1% Powered by BIP!more_vert arXiv.org e-Print Ar... arrow_drop_down arXiv.org e-Print ArchiveOther literature type . Preprint . 2018Data sources: arXiv.org e-Print ArchivePublications of the Astronomical Society of the PacificArticle . 2018 . Peer-reviewedLicense: IOP Copyright PoliciesData sources: Crossrefhttps://doi.org/10.48550/arxiv...Article . 2018License: arXiv Non-Exclusive DistributionData sources: Dataciteadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/1538-3873/aab4ef&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2016 FrancePublisher:Public Library of Science (PLoS) Vincent Lesieur; Jean-François Martin; David K. Weaver; Kim A. Hoelmer; David R. Smith; Wendell L. Morrill; N. Kadiri; Frank B. Peairs; Darren M. Cockrell; Terri L. Randolph; Debra K. Waters; Marie-Claude Bon;The wheat stem sawfly, Cephus cinctus Norton (Hymenoptera: Cephidae), is a key pest of wheat in the northern Great Plains of North America, and damage resulting from this species has recently expanded southward. Current pest management practices are inadequate and uncertainty regarding geographic origin, as well as limited data on population structure and dynamics across North America impede progress towards more informed management. We examined the genetic divergence between samples collected in North America and northeastern Asia, the assumed native range of C. cinctus using two mitochondrial regions (COI and 16S). Subsequently, we characterized the structure of genetic diversity in the main wheat producing areas in North America using a combination of mtDNA marker and micro-satellites in samples collected both in wheat fields and in grasses in wildlands. The strong genetic divergence observed between North American samples and Asian congeners, in particular the synonimized C. hyalinatus, did not support the hypothesis of a recent Ameri-can colonization by C. cinctus. Furthermore, the relatively high genetic diversity both with mtDNA and microsatellite markers offered additional evidence in favor of the native Ameri-can origin of this pest. The genetic diversity of North American populations is structured into three genetic clusters and these are highly correlated with geography. Regarding the recent southern outbreaks in North America, the results tend to exclude the hypothesis of recent movement of damaging wheat stem sawfly populations from the northern area. The shift in host plant use by local populations appears to be the most likely scenario. Finally, the significance of these findings is discussed in the context of pest management. International audience
Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2016Full-Text: http://europepmc.org/articles/PMC5154603Data sources: PubMed Centraladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1371/journal.pone.0168370&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 36 citations 36 popularity Top 10% influence Average impulse Top 10% Powered by BIP!more_vert Europe PubMed Centra... arrow_drop_down Europe PubMed CentralArticle . 2016Full-Text: http://europepmc.org/articles/PMC5154603Data sources: PubMed Centraladd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
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For further information contact us at helpdesk@openaire.eudescription Publicationkeyboard_double_arrow_right Article 2015 Netherlands, United Kingdom, Italy, France, Italy, Netherlands, Netherlands, United StatesPublisher:American Astronomical Society ALMA Partnership; E. B. Fomalont; C. Vlahakis; S. Corder; A. Remijan; D. Barkats; R. Lucas; T. R. Hunter; C. L. Brogan; Y. Asaki; S. Matsushita; W. R. F. Dent; R. E. Hills; N. Phillips; A. M. S. Richards; P. Cox; R. Amestica; D. Broguiere; W. Cotton; A. S. Hales; R. Hiriart; A. Hirota; J. A. Hodge; C. M. V. Impellizzeri; J. Kern; R. Kneissl; E. Liuzzo; N. Marcelino; R. Marson; A. Mignano; K. Nakanishi; B. Nikolic; J. E. Perez; L. M. Pérez; I. Toledo; R. Aladro; B. Butler; J. Cortes; P. Cortes; V. Dhawan; J. Di Francesco; D. Espada; F. Galarza; D. Garcia-Appadoo; L. Guzman-Ramirez; E. M. Humphreys; T. Jung; S. Kameno; R. A. Laing; S. Leon; J. Mangum; G. Marconi; H. Nagai; L.-A. Nyman; M. Radiszcz; J. A. Rodón; T. Sawada; S. Takahashi; R. P. J. Tilanus; T. van Kempen; B. Vila Vilaro; L. C. Watson; T. Wiklind; F. Gueth; K. Tatematsu; A. Wootten; A. Castro-Carrizo; E. Chapillon; G. Dumas; I. de Gregorio-Monsalvo; H. Francke; J. Gallardo; J. Garcia; S. Gonzalez; J. E. Hibbard; T. Hill; T. Kaminski; A. Karim; M. Krips; Y. Kurono; C. Lopez; S. Martin; L. Maud; F. Morales; V. Pietu; K. Plarre; G. Schieven; L. Testi; L. Videla; E. Villard; N. Whyborn; M. A. Zwaan; F. Alves; P. Andreani; A. Avison; M. Barta; F. Bedosti; G. J. Bendo; F. Bertoldi; M. Bethermin; A. Biggs; J. Boissier; J. Brand; S. Burkutean; V. Casasola; J. Conway; L. Cortese; B. Dabrowski; T. A. Davis; M. Diaz Trigo; F. Fontani; R. Franco-Hernandez; G. Fuller; R. Galvan Madrid; A. Giannetti; A. Ginsburg; S. F. Graves; E. Hatziminaoglou; M. Hogerheijde; P. Jachym; I. Jimenez Serra; M. Karlicky; P. Klaasen; M. Kraus; D. Kunneriath; C. Lagos; S. Longmore; S. Leurini; M. Maercker; B. Magnelli; I. Marti Vidal; M. Massardi; A. Maury; S. Muehle; S. Muller; T. Muxlow; E. O’Gorman; R. Paladino; D. Petry; J. Pineda; S. Randall; J. S. Richer; A. Rossetti; A. Rushton; K. Rygl; A. Sanchez Monge; R. Schaaf; P. Schilke; T. Stanke; M. Schmalzl; F. Stoehr; S. Urban; E. van Kampen; W. Vlemmings; K. Wang; W. Wild; Y. Yang; S. Iguchi; T. Hasegawa; M. Saito; J. Inatani; N. Mizuno; S. Asayama; G. Kosugi; K.-I. Morita; K. Chiba; S. Kawashima; S. K. Okumura; N. Ohashi; R. Ogasawara; S. Sakamoto; T. Noguchi; Y.-D. Huang; S.-Y. Liu; F. Kemper; P. M. Koch; M.-T. Chen; Y. Chikada; M. Hiramatsu; D. Iono; M. Shimojo; S. Komugi; J. Kim; A.-R. Lyo; E. Muller; C. Herrera; R. E. Miura; J. Ueda; J. Chibueze; Y.-N. Su; A. Trejo-Cruz; K.-S. Wang; H. Kiuchi; N. Ukita; M. Sugimoto; R. Kawabe; M. Hayashi; S. Miyama; P. T. P. Ho; N. Kaifu;Accepted: 2015-04-10 資料番号: SA1150145000 著者人数: 248名
CORE (RIOXX-UK Aggre... arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2015 . Peer-reviewedLicense: IOP Copyright PoliciesOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2015Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/2041-8205/808/1/l1&type=result"></script>'); --> </script>
For further information contact us at helpdesk@openaire.euAccess RoutesGreen gold 65 citations 65 popularity Top 10% influence Top 10% impulse Top 1% Powered by BIP!visibility 48visibility views 48 download downloads 47 Powered bymore_vert CORE (RIOXX-UK Aggre... arrow_drop_down NARCIS; The Astrophysical Journal LettersArticle . 2015 . Peer-reviewedLicense: IOP Copyright PoliciesOA@INAF - Istituto Nazionale di AstrofisicaArticle . 2015Data sources: OA@INAF - Istituto Nazionale di Astrofisicaadd ClaimPlease grant OpenAIRE to access and update your ORCID works.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.This Research product is the result of merged Research products in OpenAIRE.
You have already added works in your ORCID record related to the merged Research product.All Research productsarrow_drop_down <script type="text/javascript"> <!-- document.write('<div id="oa_widget"></div>'); document.write('<script type="text/javascript" src="https://www.openaire.eu/index.php?option=com_openaire&view=widget&format=raw&projectId=10.1088/2041-8205/808/1/l1&type=result"></script>'); --> </script>
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