adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019A&A...623A.112D (acknowledgments)
An anonymous referee made challenging yet stimulating comments which resulted in substantial improvements in the paper. This work presents results from the European Space Agency (ESA) space mission Gaia . Gaia data are being processed by the Gaia Data Processing and Analysis Consortium (DPAC). Funding for the DPAC is provided by national institutions, in particular the institutions participating in the Gaia MultiLateral Agreement (MLA). The Gaia mission website is https://www.cosmos.esa.int/gaia . The Gaia archive website is https://archives.esac.esa.int/gaia . This research makes use of the SIMBAD database and the Vizier catalog service, operated at CDS, Strasbourg, France. We also make heavy use of R: A language and environment for statistical computing. R Foundation for Statistical Computing, Vienna, Austria ( http://www.R-project.org/ ).
Paper: 2015ApJ...799...48B (acknowledgments)
We thank the referee for valuable comments that prompted improvements in the manuscript. We thank Markus Böttcher, Dominique Sluse, Tommaso Treu, and Jabran Zahid for the valuable comments on the manuscript. A.B. is supported by the Department of Energy Office of Science, NASA, and the Smithsonian Astrophysical Observatory with financial support from the NCN grant DEC-2011/01/M/ST9/01891. M.J.G. is supported by the Smithsonian Institution.
Paper: 2017MNRAS.465..123B (acknowledgments)
The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The SAMI was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the SDSS, the GAMA Survey and the VST ATLAS Survey. The SAMI Galaxy Survey is funded by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The SAMI Galaxy Survey website is http://sami-survey.org/ . GAMA is a joint European-Australasian project based around a spectroscopic campaign using the AAT. The GAMA input catalogue is based on data taken from the SDSS and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE , Herschel -ATLAS, GMRT ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/ . SMC acknowledges the support of an Australian Research Council Future Fellowship (FT100100457). LC acknowledges financial support from the Australian Research Council (DP130100664). SB acknowledges the funding support from the Australian Research Council through a Future Fellowship (FT140101166). MSO acknowledges the funding support from the Australian Research Council through a Future Fellowship Fellowship (FT140100255).
Paper: 2017A&A...601L...4K (acknowledgments)
The authors would like to thank S. Cabrit for stimulating discussions, G. Sandell for help with scheduling the observations, and the referee for valuable comments that helped improving the clarity of the paper. Submillimeter astronomy in Copenhagen is supported by the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 646908) through ERC Consolidator Grant “S4F”. Research at the Centre for Star and Planet Formation is funded by the Danish National Research Foundation. J.C.M. acknowledges support from the European Research Council under the European Community’s Horizon 2020 framework program (20142020) via the ERC Consolidator grant “From Cloud to Star Formation (CSF)” (project number 648505). A.K. acknowledges support from the Polish National Science Center grants 2013/11/N/ST9/00400 and 2016/21/D/ST9/01098. Based on observations made with the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50 OK 0901 to the University of Stuttgart.
Paper: 2015ApJ...807..158F (acknowledgments)
The SDO/AIA images are available courtesy of NASA/SDO and the AIA science teams. This work made extensive use of the AIA archive at MEDOC, http://medoc-sdo.ias.u-psud.fr .
Paper: 2019MNRAS.489.1291S (acknowledgments)
ACKNOWLEDGEMENTS This work was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. We gratefully thank the staff of the Palomar Observatory and Frank Loya for their assistance, and the referee for many questions that led to an improved paper.
Paper: 2017A&A...601A..67C (acknowledgments)
This work is based on data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. This collaboration was partially supported by funding from the Laboratoire Lagrange 2015 BQR. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in AAS, 143, 23. This work was supported in part by NASA grants NNX13AE91G and NNX16AB97G. Computational time at the Texas Advanced Computing Center was provided through XSEDE allocation TG-AST090107. D.S. and R.A.G. acknowledge the financial support from the CNES GOLF grants. D.S. acknowledges the Observatoire de la Côte d’Azur for support during his stays. Some of these computations have been done on the “Mesocentre SIGAMM” machine, hosted by the Observatoire de la Côte d’Azur. The authors wish to thank Sylvain Korzennik for his very careful reading of the paper and valuable suggestions for improving the presentation and the scientific arguments.
Paper: 2015A&A...577A..72V (acknowledgments)
We thank the anonymous referee for the valuable comments. This work has been supported by PRIN-MIUR 2010-2011 (Chemical and dynamical evolution of the Milky Way and Local Group galaxies, PI F. Matteucci) and PRIN-INAF 2012 (The M4 Core Project with Hubble Space Telescope, PI L. Bedin).
Paper: 2016ApJ...818...28S (acknowledgments)
We thank William Gray, Christopher Matzner, Prateek Sharma, and Robert Thacker for helpful discussions and the anonymous referee for comments. S.S. and E.S. were supported by the National Science Foundation grant AST11-03608 and NASA theory grants NNX09AD106 and NNX15AK82G. E.S. gratefully acknowledges the Simons Foundation for funding the workshop Galactic Winds: Beyond Phenomenology which helped to inspire this work. He also gratefully acknowledges Joanne Cohn, Eliot Quataert, and the UC Berkeley Theoretical Astronomy Center, and Uroš Seljak and the Lawrence Berkeley National Lab Cosmology group for hosting him during the period when much of this work was carried out. Part of this research was carried out during the visit of E.S. and E.C.O. at the KITP in UC Santa Barbara, which is supported by the National Science Foundation under grant PHY-1125915. The work of E.C.O. on this project was supported by the National Science Foundation under grant AST-1312006. The authors thank the Texas Advanced Computing Center (TACC) at The University of Texas at Austin (URL: http://www.tacc.utexas.edu ) and the Extreme Science and Engineering Discovery Environment (XSEDE) for providing HPC resources via grant TG-AST140004 that have contributed to the results reported within this paper. The FLASH code is developed in part by the DOE-supported Alliances Center for Astrophysical Thermonuclear Flashes (ASC) at the University of Chicago.
Paper: 2019MNRAS.490.2219N (acknowledgments)
ACKNOWLEDGEMENTS This paper includes data gathered with the 6.5-m Magellan Telescope located at Las Campanas Observatory, Chile. We thank David W. Hogg (NYU) and Hans-Walter Rix (MPIA) for useful discussions. ARC is supported through an Australian Research Council Discovery Project under grant DP160100637. AIK acknowledges financial support from the Australian Research Council (DP170100521). AYQH was supported by the GROWTH project funded by the National Science Foundation under PIRE Grant No 1545949, and a National Science Foundation Graduate Research Fellowship under Grant No. DGE-1144469. APJ is supported by NASA through Hubble Fellowship grant HST-HF2-51393.001 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. This research has made use of NASA’s Astrophysics Data System. The Guoshoujing Telescope (LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. This work has made use of data from the European Space Agency (ESA) mission Gaia ( https://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, https://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement.
Paper: 2017MNRAS.467.2787H (acknowledgments)
Acknowledgments The authors have benefited from many inspiring discussions with Hlne Curtois, Noam Libeskind and Brent Tully. We also like to thank the anonymous referee for their constructive report that helped to increase the quality of this work. The hospitality of the Technion Israel Institute of Technology enjoyed by WAH, MF and MB at the early stages of this project is warmly acknowledged. WAH acknowledges support from European Research Council (grant number 646702 CosTesGrav). WAH and MB were also supported by the Polish National Science Center under contract #UMO-2012/07/D/ST9/02785. This research was supported by the I-CORE Program of the Planning and Budgeting Committee, THE ISRAEL SCIENCE FOUNDATION (grant Nos. 1829/12 and 203/09) and the Asher Space Research Institute. MF acknowledges support through the Grant Spin(e) ANR-13-BS05-0005 of the French National Research Agency.
Paper: 2016MNRAS.460..240K (acknowledgments)
We thank Maxim Makukov, Chingis Omarov, Emmanuil Y. Vilkoviskij and Ari Laor for valuable comments, discussion, support and supervision. We also thank the anonymous referee for useful comments and suggestions. This work has benefitted very much from funding of exchange and collaboration between Germany and Kazakhstan by Volkswagen Foundation under the project ‘STARDISK – Simulating Dense Star-Gas Systems in Galactic Nuclei using special hardware’ (I/81 396). GRAPE and GPU hardware at Fesenkov Astrophysical Institute in Kazakhstan used for this work have been supported by the STARDISK project too. We acknowledge support from the Strategic Priority Research Program ‘The Emergence of Cosmological Structure’ of the Chinese Academy of Sciences (No. XDB09000000) (Pilot B programme). We acknowledge support by Chinese Academy of Sciences through the Silk Road Project at NAOC, through the Chinese Academy of Sciences Visiting Professorship for Senior International Scientists, Grant Number 2009S1-5 (RS), and through the ‘Qianren’ special foreign experts programme of China. RS has also been partially supported by NSFC (National Natural Science Foundation of China), grant no. 11073025. GK acknowledges a Chinese Academy of Sciences Young International Postdoctoral Fellowship Grant No. 2011Y2JB09. YM acknowledges support from the China Postdoctoral Science Foundation through grant no. 2015T80011 and from excellence initiative at the University of Heidelberg, through mobility measures for international research collaborations project no. 7.1.47, and the European Research Council under the European Union's Horizon 2020 Programme, ERC-2014-STG grant GalNUC 638435. PB acknowledges the special support by the NASU under the Main Astronomical Observatory GRID/GPU computing cluster project. The special GPU accelerated supercomputer laohu at the Center of Information and Computing at National Astronomical Observatories, Chinese Academy of Sciences, funded by Ministry of Finance of People's Republic of China under the grant ZDYZ2008-2, has been used for some of the largest simulations. We also used smaller GPU clusters titan , hydra and kepler , funded under the grants I/80041-043 and I/84678/84680 of the Volkswagen Foundation and grants 823.219-439/30 and /36 of the Ministry of Science, Research and the Arts of Baden-Württemberg, Germany.
Paper: 2015ApJ...807...44P (acknowledgments)
We thank the anonymous referee for a meticulous and thoughful set of comments. B.P. thanks NSERC for an undergraduate summer fellowship, and Nikhil Mahajan for assistance. Y.W. acknowledges NSERC funding, as well as conversations with Yoram Lithwick, Doug Lin (who pointed out that Johannes Kepler did ponder the planet packing problem), and Scott Tremaine.
Paper: 2019ApJ...873....7Z (acknowledgments)
We thank the anonymous referee for valuable comments and suggestions. This work was partially supported by the National Natural Science Foundation of China (grant Nos. 11673060, 11763005, and 11873043), the Key Research Program of the Chinese Academy of Sciences (grant No. KJZD-EW-M06), the Strategic Priority Research Program “The Emergence of Cosmological Structure” of the Chinese Academy of Sciences (grant No. XDB09000000), and the Natural Science Foundation of Yunnan Province (grant Nos. 2016FB003 and 2017FD072). Additional support was provided by the Specialized Research Fund for Shandong Provincial Key Laboratory (grant No. KLWH201804), by the Key Laboratory of Particle Astrophysics of Yunnan Province (grant No. 2015DG035) and by the Research Foundation for Scientific Elitists of the Department of Education of Guizhou Province (grant No. QJHKYZ[2018]068).
Paper: 2018MNRAS.480.1466S (acknowledgments)
ACKNOWLEDGEMENTS We thank an anonymous referee for a careful reading of the manuscript. We benefitted from numerous sisyphean conversations about the grey area between explosions and winds with Stan Owocki, Dave Arnett, Eliot Quataert, and Chris Matzner, and informative conversations about binary L2 mass-loss and mergers with Ondrej Pejcha, Stephen Justham, Kaitlin Kratter, and Philipp Podsiadlowski. We have also discussed binary evolution, on occasion, with Selma de Mink. NS’s research on Eta Carinae’s light echoes and eruptive transients was supported by National Science Foundation (NSF) grants AST-1312221 and AST-1515559. Partial support for this work was provided by NASA grants AR-12618, AR-14586, and GO-13390 from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. Support for JLP is provided in part by FONDECYT through the grant 1151445 and by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. DJJ gratefully acknowledges support from the NSF through award AST-1440254. This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile. This project used data obtained with the Dark Energy Camera (DECam), which was constructed by the Dark Energy Survey (DES) collaborating institutions. Funding for DES, including DECam, has been provided by the U.S. DoE, NSF, MECD (Spain), STFC (UK), HEFCE (England), NCSA, KICP, FINEP, FAPERJ, CNPq (Brazil), the GRF-sponsored cluster of excellence ‘Origin and Structure of the Universe’ and the DES collaborating institutions. This work makes use of observations from the LCO network. Based, in part, on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil) (Program GS-2014B-Q-24).
Paper: 2015ApJ...810...52M (acknowledgments)
We thank the anonymous referee for helpful comments which improved the quality of this paper. This research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. This research has also made use of the NASA/IPAC Extragalactic Database (NED) which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Paper: 2017ApJ...846..140M (acknowledgments)
We thank the anonymous referees for many useful comments and suggestions. This work is supported by National Natural Science Foundation of China under Grant No. 11175147,11547311.
Paper: 2015MNRAS.454.1778J (acknowledgments)
This work is based on the data from NASA's GALEX spacecraft. GALEX is operated for NASA by the California Institute of Technology under NASA contract NAS5-98034. We acknowledge the NASA's Astrophysics Data System and NASA's SkyView facility ( http://skyview.gsfc.nasa.gov ) located at NASA Goddard Space Flight Center. Jyothy is grateful to Sri Mata Amritanandamayi Devi, the Chancellor of Amrita University for her spiritual guidance. Jyothy would like to thank Mr Sathyanarayanan for his help. We thank the referee for a prompt response and for pointing out inconsistencies in the first draft.
Paper: 2016MNRAS.463.4490C (acknowledgments)
We thank the referee for useful discussion that helped in improving the content of this paper. Funding for the SDSS-IV has been provided by the Alfred P. Sloan Foundation, the US Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org . SDSS-IV is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofísica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatory of China, New Mexico State University, New York University, University of Notre Dame, Observatário Nacional/MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University. YYZ acknowledges support by the German BMWI through the Verbundforschung under grant 50 OR 1506. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ .
Paper: 2019ApJ...874...54M (acknowledgments)
We are grateful to Scott Adams and Kevin Croxall for helpful discussions about the analysis of MODS prism data. We also appreciate helpful comments from the referee. Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award No. G04-15134X issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060. The work of P.M. is partially supported by the National Science Foundation under grant 1615553 and by the Department of Energy under grant DE-SC0015525.
Paper: 2018A&A...610A...7M (acknowledgments)
This work was supported by grant No. 2014/13/D/ST9/ 01818 from the National Science Centre, Poland. The research leading to these results has received funding from the European Union’s Horizon 2020 Research and Innovation Programme, under Grant Agreement No. 687378. V.K. was supported by the grant from the Slovak Research and Development Agency with number APVV-15-0458. The Joan Oró Telescope (TJO) of the Montsec Astronomical Observatory (OAdM) is owned by the Catalan Government and is operated by the Institute for Space Studies of Catalonia (IEEC). The 0.82 m IAC80 Telescope is operated on the island of Tenerife by the Instituto de Astrofisica de Canarias in the Spanish Observatorio del Teide. Based on observations obtained with the SARA Observatory 1.0 m Jacobus Kapteyn Telescope at ORM, and 0.6 m telescope at CTIO, which are owned and operated by the Southeastern Association for Research in Astronomy ( http://saraobservatory.org ).
Paper: 2016A&A...589A.127J (acknowledgments)
We thank Dr. O. Pirali and S. Gruet for helpful discussions and advices in the far-infrared analysis using the Loomis-Wood program. I.K. and A.J. are indebted to Dr. V.V. Ilyushin for helpful discussions and careful reading of the manuscript. A.J. and I.K. thank the Groupe de Recherche International GDRI HighRes (especially Dr. A. Perrin) and the Programme Chimie Milieu Interstellaire PCMI for travel funding. V. V. thanks the Fonds der Chemischen Industrie (FCI) for a Ph.D. fellowship.
Paper: 2019ApJ...876...39G (acknowledgments)
R.A.G.L., L.L., and G.B. acknowledge the financial support of DGAPA, UNAM (respectively, projects IN108518, IN112417, and IG100319), and CONACyT, Mexico. We sincerely thank the anonymous referee for the very constructive and insightful comments. This work is based on observations made with the NASA/ESA Hubble Space Telescope and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA), and the Canadian Astronomy Data Centre (CADC/NRC/CSA). Facilities: GTC:OSIRIS , HST , CFHT , Westerbork Synthesis Radio Telescope . Software: SExtractor (Bertin Arnouts 1996 ), IRAF, rvsao (Kurtz Mink 1998 ), sm (Lupton Monger 1991 ), der_snr, Kapteyn (Terlouw Vogelaar 2015 ).
Paper: 2015A&A...579A.122A (acknowledgments)
We thank Achim Weiss for the GARSTEC models used in this work, Zazralt Magic for the grid of model photospheres, and the anonymous referee for critical comments that improved the introduction section and the overall presentation of the text.