adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015ApJ...806..122Z (acknowledgments)
We thank the anonymous referee for a careful reading of the manuscript. H.J.Z. gratefully acknowledges the generous support of the Clay Postdoctoral Fellowship. I.D. is supported by the Harvard College Observatory Menzel Fellowship and the Natural Sciences and Engineering Research Council of Canada Postdoctoral Fellowship (NSERC PDF-421224-2012). I.C. acknowledges support from the Russian Science Foundation project #14-22-00041. This research has made use of NASA’s Astrophysics Data System Bibliographic Services. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III web site is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. Based on observations made with the NASA/ESA Hubble Space Telescope , obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555.
Paper: 2019ApJ...885....6J (acknowledgments)
We thank an anonymous referee for insightful comments that have improved the content and presentation of this paper. D.W.J. and D.Z. acknowledge financial support from NASA LTSA award NNG05GE82G and GALEX grant NNX11AI47G. G.D.L. acknowledges financial support from the European Research Council under European Community’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement No. 202781. P.J. acknowledges support by the Swiss National Science Foundation (SNSF).
Paper: 2020MNRAS.491..576J (acknowledgments)
ACKNOWLEDGEMENTS The author is grateful to Paul Bryans and an anonymous referee for useful comments. NCAR is sponsored by the National Science Foundation.
Paper: 2018A&A...609A..77S (acknowledgments)
We thank the referee for valuable comments and suggestions. N.S. acknowledges financial support from the pole PAGE of the Université Grenoble Alpes. G.L., G.D. and M.F. are grateful to the participants of the KITP 2017 program on Confronting MHD Theories of Accretion Disks with Observations for the many useful conversations pertaining to this work (and thus this research was supported in part by the National Science Foundation under Grant No. NSF PHY-1125915). This work was granted access to the HPC resources of IDRIS under the allocation A0020402231 made by GENCI (Grand Equipement National de Calcul Intensif). Some of the computations presented in this paper were performed using the Froggy platform of the CIMENT infrastructure ( https://ciment.ujf-grenoble.fr ), which is supported by the Rhône-Alpes region (GRANT CPER07_13 CIRA), the OSUG@2020 labex (reference ANR10 LABX56) and the Equip@Meso project (reference ANR-10-EQPX-29-01) of the programme Investissements d’Avenir supervised by the Agence Nationale pour la Recherche.
Paper: 2015ApJ...802...51H (acknowledgments)
RH thanks Avi Shporer for providing the program to compute ingress and egress shapes, Tiffany Kataria for making available preliminary 3D atmospheric circulation simulations, Edwin Kite for discussion on the molten lava planet, Feng Tian for discussion on the atmospheric escape of rocky planets, and Wesley Traub and Yuk L. Yung for helpful discussions. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. Support for RH’s work was provided in part by NASA through Hubble Fellowship grant #51332 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. Part of the research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. NKL’s work was performed in part under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute.
Paper: 2015ApJ...815...11V (acknowledgments)
This work was supported by the Romanian Ministry of National Education under the contracts 1EU-10 (in the Programme of Complementary Research in Fusion) and PN 09 39 01 01.
Paper: 2015MNRAS.451.4253R (acknowledgments)
Work is supported by grant of Russian Science Foundation 14-12-01287.
Paper: 2018A&A...609A..44T (acknowledgments)
The authors acknowlede insightful comments from Moti Milgrom, Paola Di Matteo, Francoise Combes, Edouard Bernard, Gary Mamon, and an anonymous referee. F.R. acknowledges support from the European Research Council through grant ERC-StG-335936.
Paper: 2019ApJ...872..100D (acknowledgments)
We wish to thank T. Fouchet, E. Jaupart, G. Laibe, and D. Stevenson for helpful discussions. G.C. acknowledges the warm hospitality of the OWL Institute at the University of Santa Cruz, where part of this work was accomplished. This work was supported by the Programme National de Planétologie (PNP) of CNRS-INSU cofunded by CNES.
Paper: 2018MNRAS.473...38S (acknowledgments)
Acknowledgements The authors contributed in the following way to this paper. DS undertook the calibration and completion of all simulations; the development of all analysis codes, including the ANN; the production of all figures and the first draft of the paper. II supervised the project and helped with the interpretation of results and feedback on the first draft. KD provided guidance throughout and significant feedback on the first draft. DS would like to thank Joakim Rosdahl for valuable technical feedback, Scott J. Clay for advice and feedback on the first draft, Peter A. Thomas, Paul R. Shapiro, and Benoît Fournier for useful discussions and feedback. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the Science and Technology Facilities Council (STFC) DiRAC High-performance computing (HPC) Facility ( www.dirac.ac.uk ). The DiRAC system is funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1, STFC DiRAC Operations grant ST/K003267/1, and Durham University. DiRAC is part of the National E-Infrastructure. We acknowledge PRACE for awarding us computational time under project PRACE4LOFAR grant 2014102339 and ‘Multi-scale simulations of Cosmic Reionization’ grants 2014102281, 2015122822, and 2016153528 to resource Curie based in France at CEA and to resource Marenostrum based in Spain at BSC. This work was supported by the Science and Technology Facilities Council (grant numbers ST/F002858/1 and ST/I000976/1) and the Southeast Physics Network (SEPNet). Some of the analysis was done on the Apollo cluster at The University of Sussex. We made extensive use of the pymses (Guillet, Chapon Labadens 2013 ) and pynbody (Pontzen et al. 2013 ) python modules when developing our own analysis pipeline.
Paper: 2018A&A...619A.111N (acknowledgments)
The authors are grateful to the referee for comments and suggestions that greatly improved the manuscript. This work was supported by the Programme National “Physique et Chimie du Milieu Interstellaire” (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES and the DIM ACAV a funding programme of the Region Ile de France. T.N is granted by the LabEx MICHEM.
Paper: 2015ApJ...799...92J (acknowledgments)
We thank the anonymous referee for careful review and valuable suggestions, the SMT staff for their help during the observations, Ran Wang for her help with the observation, and U. Lisenfeld for kindly making the H i data available to us. X.J. acknowledges support for this work from the Strategic Priority Research Program “The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (CAS), grant XDB09000000. This work is supported under the National Natural Science Foundation of China (grants 11273015 and 11133001), the National Basic Research Program (973 program No. 2013CB834905), and Specialized Research Fund for the Doctoral Program of Higher Education (20100091110009). Z.-Y.Z acknowledges support from the European Research Council (ERC) in the form of an Advanced Grant, cosmicism . This publication makes use of data products from the Wide-field Infrared Survey Explorer , which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. The Arecibo Observatory is part of the National Astronomy and Ionosphere Center which is operated by Cornell University under a cooperative agreement with the National Science Foundation. Based on observations made with the NASA Galaxy Evolution Explorer ( GALEX ). GALEX is operated for NASA by the California Institute of Technology under NASA contract NAS5-98034. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. The SDSS-III Web site is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University.
Paper: 2016MNRAS.460.4063A (acknowledgments)
This work was supported by the ERC under the Advanced Investigator Project 267219 and the University of Jordan. JT and SNY thank the support of the COST action MOLIM (CM1405). We thank the Royal Society for supporting a visit by OVN to London.
Paper: 2017ApJ...837...11B (acknowledgments)
We thank the anonymous referee for a careful review and suggestions that improved the manuscript. This research was partially supported by a Jet Propulsion Lab/NASA grant to the University of Minnesota (RSA 1541900/NNN12AA01C). Support for HST Programs GO-11696, 12283, 12568, 12902, 13517, 13352, and 14178 was provided by NASA through grants from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. T.G. is grateful to the LABEX Lyon Institute of Origins (ANR-10-LABX-0066) of the Université de Lyon for its financial support within the program “Investissements d’Avenir” (ANR-11-IDEX-0007) of the French government operated by the National Research Agency (ANR). This research has made use of NASA’s Astrophysics Data System Bibliographic Services.
Paper: 2019MNRAS.484.2009B (acknowledgments)
ACKNOWLEDGEMENTS We thank Gianfranco Bertone and Denis Erkal for useful discussions and comments. We thank the anonymous referee whose comments have greatly improved this manuscript. NB acknowledges the support of the D-ITP consortium, a programme of the Netherlands Organization for Scientific Research (NWO) that is funded by the Dutch Ministry of Education, Culture and Science (OCW). JB acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC), funding reference number RGPIN-2015-05235, and from an Alfred P. Sloan Fellowship.
Paper: 2016MNRAS.461.2847B (acknowledgments)
We thank an anonymous referee for helpful comments that considerably improved the manuscript. GB thanks Judd Bowman, Andrea Ferrara, Adrian Liu and Aaron Ewall-Wice for useful inputs and comments on this work and Jordan Mirocha for help with ares . The LEDA experiment is supported by NSF grants AST/1106059 and PHY/0835713. JZ gratefully acknowledges a South Africa National Research Foundation Square Kilometre Array Research Fellowship. This research was supported by the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence ‘Origin and Structure of the Universe’. With the support of the Ministry of Foreign Affairs and International Cooperation, Directorate General for the Country Promotion (Bilateral Grant Agreement ZA14GR02 – Mapping the Universe on the Pathway to SKA).
Paper: 2015ApJ...808..117N (acknowledgments)
We thank the referee for his/her constructive comments. This research has been partly co-financed by the European Union (European Social Fund—ESF) and Greek national funds through the Operational Program “Education and Lifelong Learning” of the National Strategic Reference Framework (NSRF)—Research Funding Program: “Thales. Investing in knowledge society through the European Social Fund.” S.P. acknowledges support from an FP7 Marie Curie Grant (FP7-PEOPLE-2010-RG/268288). A.V. was also supported by internal JHU/APL funds.
Paper: 2019ApJ...879...74C (acknowledgments)
We sincerely thank the anonymous referee for valuable comments and suggestions that significantly improved the scientific content and presentation of the manuscript. We also thank Jun Zhang for constructive suggestions, as well as Junchao Hong and Haidong Li for helpful discussions. SDO is a mission of NASA’s Living With a Star Program. H.C.C, J.Y.Y, and Y.D.D are supported by the Natural Science Foundation of China (NSFC) under grants 11633008, 11703084, and 11873088, and also by the CAS program QYZDJ-SSW-SLH012. K.F.J is supported by NSFC under grants 11773072 and 11873027.
Paper: 2017A&A...597A.114B (acknowledgments)
M. Beuret thanks Arnaud Siebert for providing the shape of the spiral arms from Englmaier et al. (2011) . 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 research has also made use of NASA’s Astrophysics Data System Bibliographic Services. Davide Elia’s and Eugenio Schisano’s research activity is supported by the VIALACTEA project, a Collaborative project under Framework Programme 7 of the European Union funded under Contract #607380, that is hereby acknowledged.
Paper: 2015MNRAS.448..119F (acknowledgments)
The authors are grateful to the anonymous referee for the important suggestions/corrections on this paper. Part of this work was supported by CAPES/Cofecub Project 712/2011. BF thanks CNPq Project 142849/2010-3. JGH acknowledges partial support from FAPESP Proc. No. 2010/50930-6. This publication makes use of data products from the 2MASS, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. This publication makes use of data products from the WISE , which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration.
Paper: 2019MNRAS.483..964B (acknowledgments)
ACKNOWLEDGEMENTS The Dunlap Institute is funded through an endowment established by the David Dunlap family and the University of Toronto. BMG acknowledges the support of the Natural Sciences and Engineering Research Council of Canada (NSERC) through grant RGPIN-2015-05948, and of the Canada Research Chairs program. Partial support for LR comes from NSF grant 17-14205 to the University of Minnesota. XS is supported by the National Natural Science Foundation of China under grant No. 11763008.
Paper: 2019MNRAS.490.1803R (acknowledgments)
ACKNOWLEDGEMENTS ADR, LAA, GO, GRL, and SOK acknowledge financial support from CNPq and PRONEX-FAPERGS/CNPq (Brazil). TK acknowledges financial support from Capes (Brazil). DS is supported by the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., on behalf of the international Gemini partnership of Argentina, Brazil, Canada, Chile, the Republic of Korea, and the United States of America. IP acknowledges funding by the Deutsche Forschungsgemeinschaft under grant GE2506/12-1. Based on observations obtained at Observatório do Pico dos Dias/LNA, at the Southern Astrophysical Research (SOAR) telescope, which is a joint project of the Ministério da Ciência, Tecnologia, Inovação e Comunicaçẽs (MCTIC) do Brasil, the US National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU) and processed using the Gemini iraf package, 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, Inovação e Comunicaçẽs (Brasil). This work has used 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. This research has also made use of the TOPCAT ( http://www.starlink.ac.uk/topcat/ ) software (Taylor 2005 ), The Montreal White Dwarf Database (Dufour et al. 2017 , http://www.montrealwhitedwarfdatabase.org/home.html ), and NASA Astrophysics Data System. We thank P. Bergeron for sharing the atmosphere models for DA white dwarf for Gaia filters. The observational data are available upon request to alejandra.romero@ufrgs.br .
Paper: 2016MNRAS.456..739X (acknowledgments)
The authors would like to thank Stefan Hilbert, Sherry Suyu, Malte Tewes, James Nightingale and an anonymous referee for very useful comments. DDX thanks the HITS fellowship. DS acknowledges support from a Back to Belgium grant from the Belgian Federal Science Policy (BELSPO) and partial funding from the Deutsche Forschungsgemeinschaft, reference SL172/1-1. PS and VS acknowledge support by the DFG through Transregio 33, ‘The Dark Universe’. VS also acknowledges support by the European Research Council under ERC-StG EXAGAL-308037. LH acknowledges support from NASA grant NNX12AC67G and NSF grant AST-1312095. DDX and VS gratefully acknowledge the support of the Klaus Tschira Foundation.
Paper: 2016ApJ...818...46M (acknowledgments)
A.W.M. was supported through Hubble Fellowship grant 51364 awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. This research was supported by NASA grant NNX11AC33G to E.G. E.G. was also supported by an International Visitor grant from the Swiss National Science Foundation. We thank Bandit for his useful discussions and encouragement during the writing of this manuscript. This work used the Immersion Grating Infrared Spectrograph (IGRINS), which was developed under a collaboration between the University of Texas at Austin and the Korea Astronomy and Space Science Institute (KASI) with the financial support of the US National Science Foundation under grant ASTR1229522, of the University of Texas at Austin, and of the Korean GMT Project of KASI. The IGRINS pipeline package PLP was developed by Dr. Jae-Joon Lee at Korea Astronomy and Space Science Institute and Professor Soojong Pak's team at Kyung Hee University. SNIFS on the UH 2.2 m telescope is part of the Nearby Supernova Factory project, a scientific collaboration among the Centre de Recherche Astronomique de Lyon, Institut de Physique Nucléaire de Lyon, Laboratoire de Physique Nucléaire et des Hautes Energies, Lawrence Berkeley National Laboratory, Yale University, University of Bonn, Max Planck Institute for Astrophysics, Tsinghua Center for Astrophysics, and the Centre de Physique des Particules de Marseille. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. This research was made possible through the use of the AAVSO Photometric All-Sky Survey (APASS), funded by the Robert Martin Ayers Sciences Fund. The authors acknowledge the Texas Advanced Computing Center (TACC) at The University of Texas at Austin for providing grid resources that have contributed to the research results reported within this paper. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Facilities: IRTF (SpeX) , UH:2.2 m (SNIFS) , kepler , Keck:II (NIRC2) , Smith (IGRINS) .
Paper: 2018A&A...616A.186F (acknowledgments)
We would like to thank the referee for the very helpful comments that helped to improve the manuscript. We thank M. Kühnel and M. Nowak for the useful discussions. DJW and MJM acknowledge support from STFC Ernest Rutherford fellowships. This research has made use of data obtained with NuSTAR , a project led by Caltech, funded by NASA and managed by NASA/JPL, and has utilized the nustardas software package, jointly developed by ASDC (Italy) and Caltech (USA). This research has also made use of data obtained with XMM-Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States. This work has made use of data supplied by the UK Swift Science Data Centre at the University of Leicester, and also of the XRT Data Analysis Software (XRTDAS) developed under the responsibility of the ASI Science Data Center (ASDC), Italy. This research has made use of a collection of ISIS functions (ISISscripts) provided by ECAP/Remeis observatory and MIT ( http://www.sternwarte.uni-erlangen.de/isis/ ).
Paper: 2015ApJ...799...49H (acknowledgments)
This work is supported by the NSF Astronomy and Astrophysics Division (grant No.1311958 to G.V.). We thank Dr. J. Brucato of the Astrophysical Observatory of Arcetri (Italy) for providing the sample used in these experiments and Zhirou Zhang, Jianming Shi, and Tyler Hopkins for technical help. R.T.G. acknowledges the support of the NASA Astrophysics Theory Program (grant No. NNX11AC38G).