adsabs/WIESP2022-NER huggingface dataset:
Paper: 2016A&A...591A..42S (acknowledgments)
This work was partly supported by Campus France, by the Scientific Council of Paris Observatory, by IMCCE, and by IPSA. This work was supported by the Russian Foundation for Basic Research, project No. 16-52-150005-CNRS-a.
Paper: 2019ApJ...874...51K (acknowledgments)
M.M. wishes to acknowledge support from NASA under contract NAS8-03060. This research has made use of data obtained from the Chandra Data Archive and software provided by the Chandra X-ray Center (CXC). T.K. was supported in part by NASA grant 14-ATP14-0022 through the Astrophysics Theory Program.
Paper: 2015MNRAS.453.2644A (acknowledgments)
This paper is partially based on observations made with SOPHIE on the 1.93 m telescope at the Observatoire de Haute-Provence (CNRS), France. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. All of the data presented in this paper were obtained from the MAST. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. The team at LAM acknowledge support by CNES grants 98761 (SCCB), 426808 (CD) and 251091 (JMA). JMA and XB acknowledge funding from the European Research Council under the ERC Grant Agreement no. 337591-ExTrA. XB acknowledge the support of the French Agence Nationale de la Recherche (ANR), under the program ANR-12-BS05-0012 Exo-atmos. RFD acknowledge funding from the European Union Seventh Framework Programme (FP7/2007-2013) under Grant agreement no. 313014 (ETAEARTH), and the financial support of the SNSF in the frame of the National Centre for Competence in Research ‘PlanetS’. We thank S. Udry for discussions on the dynamics of this system, L. Kreidberg for her Mandel Agol code, and T. Fenouillet for his assistance with the LAM cluster.
Paper: 2017MNRAS.468.1038W (acknowledgments)
Acknowledgments We are grateful to the referee, Raffaele Gratton, whose comments greatly improved the paper. Support for this work (proposal number GO-10775) was provided by NASA through a grant from the Space Telescope Science Institute that is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. This material is based upon work supported by the National Aeronautics and Space Administration under Grant NNX11AF34G issued through the Office of Space Science and through the University of Central Floridas NASA Florida Space Grant Consortium. DSs work was supported by NSF grants DMS 1208791. DvD was partially supported by a Wolfson Research Merit Award (WM110023) provided by the British Royal Society and by Marie-Curie Career Integration (FP7-PEOPLE-2012-CIG-321865) and Marie-Skodowska-Curie RISE (H2020-MSCA-RISE-2015-691164) Grants both provided by the European Commission.
Paper: 2017ApJ...837..128W (acknowledgments)
We thank the anonymous referee for his/her constructive comments. This work is supported by the National Basic Research Program (“973” Program) of China under grant no. 2014CB845800 and the National Natural Science Foundation of China (grant no. U1331202, 11533033, U1331101, 11573014, 11422325, and 11373022). D.X. acknowledges support from the One-Hundred-Talent Program of the National Astronomical Observatories, Chinese Academy of Sciences.
Paper: 2016ApJ...820...23G (acknowledgments)
This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of the NASA/ IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work was partly supported by Kepler grants NNX12AC89G and NNX11AG95G. D.K. is supported by a DOE office of nuclear physics early career award.
Paper: 2017ApJ...834..192L (acknowledgments)
The authors are much indebted to Ke-Jun Li for his constructive proposals and helpful suggestions. This work is supported by the National Natural Science Foundation of China (11573065, 11633008, 11273057, 11603071, and 11603069), the Specialized Research Fund for State Key Laboratories, and the Chinese Academy of Sciences. The authors declare that they have no conflicts of interest.
Paper: 2019ApJ...883..173P (acknowledgments)
We are thankful to the helpful comments about star formation rate estimation and the implications of MIR neon emission lines from an anonymous referee on this paper. This work is supported by the National Natural Science Foundation of China (NSFC-11573024, 11903029, 11473025, 11421303) and the National Basic Research Program of China (2013CB834905). W.L. acknowledges supports from the Natural Science Foundation of China grant (NSFC-11703079) and the 'Light of West China' Program of Chinese Academy of Sciences (CAS). P.J. is supported by the National Natural Science Foundation of China (NSFC-11973037), and H.W. is supported by the Natural Science Foundation of China (NSFC-11890693). We acknowledge the use of the Hale 200-inch Telescope at Palomar Observatory through the Telescope Access Program (TAP), as well as the archival data from the SDSS, 2MASS, and WISE surveys. TAP is funded by the Strategic Priority Research Program, the Emergence of Cosmological Structures (XDB09000000), National Astronomical Observatories, Chinese Academy of Sciences, and the Special Fund for Astronomy from the Ministry of Finance. Observations obtained with the Hale Telescope at Palomar Observatory were obtained as part of an agreement between the National Astronomical Observatories, Chinese Academy of Sciences, and the California Institute of Technology. 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 website is http://www.sdss3.org/ .
Paper: 2018ApJ...859..153S (acknowledgments)
We thank the referee for a constructive report. This paper includes data collected by the K2 mission, funded by the NASA Science Mission directorate. The work was supported in part by NSERC grants to R.J. A.S. received funding from the UK Science and Technology Facilities Council (ST/R000824/1). S.A. gratefully acknowledges support from the Leverhulme Trust (RPG-2012-661) and the UK Science and Technology Facilities Council (ST/K00106X/1,ST/N000919/1). D.P.’s work was supported by NASA grant NNX17AI61G. Facility: Kepler / K2 . Software: astropy (Astropy Collaboration et al. 2013 ), numpy (Van Der Walt et al. 2011 ), scipy (Jones et al. 2001 ), emcee (Foreman-Mackey et al. 2013 ), K2SC (Aigrain et al. 2016 ), PyAstronomy ( https://github.com/sczesla/PyAstronomy ).
Paper: 2016MNRAS.462.3854L (acknowledgments)
We thank Dave Campbell, Will Cowley and Peder Norberg for their contributions to this work. We thank Claudia Maraston for supplying versions of her stellar population model for different IMFs. We thank Rychard Bouwens, Ignacio Ferreras and Ian Smail for comments on the paper. Finally, we thank the referee Bruno Henriques for a detailed and constructive report that helped improve the paper. This work was supported by the Science and Technology Facilities Council grants ST/F001166/1 and ST/L00075X/1, and by European Research Council grant GA 267291 (Cosmiway). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1, and STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure. CMB acknowledges receipt of a Research Fellowship from the Leverhulme Trust. Galaxy catalogues calculated using the model described in this paper will be made available on a relational data base accessible from http://virgodb.dur.ac.uk/ .
Paper: 2019MNRAS.490.5904C (acknowledgments)
ACKNOWLEDGEMENTS This research is co-financed by Greece and the European Union (European Social Fund–ESF) through the Operational Programme ‘Human Resources Development, Education and Lifelong Learning’ in the context of the project ‘Strengthening Human Resources Research Potential via Doctorate Research’ (MIS-5000432), implemented by the State Scholarships Foundation (IKY). We acknowledge Davide de Martin James Long (ESA/Hubble) for use of the HST image of A2218, as well as Prof. Gustavo Yepes for providing access to the Cosmological N -body Simulation data used in this work. We also wish to thank Dr. Angel-Ruiz Camuñas for his help in using the photutils package. This research made use of photutils , an astropy package for detection and photometry of astronomical sources. Finally, we would like to thank the anonymous referee for suggestions that improved significantly the work presented in our manuscript.
Paper: 2015ApJ...798...21B (acknowledgments)
D. V. Bisikalo and V. I. Shematovich were partially supported by the Russian Academy of Sciences (Program-22), and by the Russian Foundation for Basic Research (Project 14-02-00838). B. Hubert, D. Hutsemékers, and E. Jehin are supported by the Belgian FRS-FNRS. This work was supported by the FRFC grant no. 2.4541.11. A. Decock acknowledges the support of the Belgian National Science Foundation F.R.I.A., Fonds pour la formation à la Recherchedansl'Industrie et l'Agriculture. The authors thank the reviewer for very helpful comments.
Paper: 2020MNRAS.491.1243P (acknowledgments)
ACKNOWLEDGEMENTS This work has been partially supported by UNAM-PAPIIT IN-107518. RP thanks Carl Knight and Anal Wnsche for nicely providing information about the observations of WASP-19b published in the ETD. RP and EJ acknowledge DGAPA for their postdoctoral fellowships and Drs. L. Hebb, C. Hellier, J. Tregloan-Reed, D. Dragomir, J. Bean, E. Sedaghati, and N. Espinoza for kindly providing the new transits presented in their studies. RP and EJ are also grateful to the operators of the 1.54-m telescope at EABA, Cecilia Quiones and Luis Tapia, for their support during the observing runs. All the authors thank the anonymous referee for useful comments and suggestions. We would also like to thank the Pierre Auger Collaboration for the use of its facilities. The operation of the robotic telescope FRAM is supported by the grant of the Ministry of Education of the Czech Republic LM2015038. The data calibration and analysis related to FRAM telescope is supported by the Ministry of Education of the Czech Republic MSMT-CRLTT18004 and MSMT/EU funds CZ.02.1.01/0.0/0.0/16_013/0001402. This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France and NASAs Astrophysics Data System Bibliographic Services (Wenger et al. 2000 ). This work is partially based on observations obtained with the 1.54-m telescope at Estacin Astrofsica de Bosque Alegre dependent on the National University of Crdoba, Argentina. Based on data acquired at Complejo Astronmico El Leoncito, operated under agreement between the Consejo Nacional de Investigaciones Cientficas y Tcnicas de la Repblica Argentina and the National Universities of La Plata, Crdoba and San Juan (Programme ID: JS-2019A-06, PI: E. Jofr).
Paper: 2015A&A...582A..71H (acknowledgments)
X.H. thanks Myriam Benisty and Gilles Duvert for their work on the reduction package amdlib, the AMBER data reduction package of the Jean-Marie Mariotti Center 2 . For quick-look analysis, this work has made use of LITPro ( Tallon-Bosc et al. 2008 ). CNRS is acknowledged for having supported this work with allocation of 14 h in Guaranteed Time Observations. Support for this work was provided by NASA through grant number HST-GO-12610.001-A from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555.
Paper: 2016MNRAS.458.2012V (acknowledgments)
We thank two anonymous referees for helpful comments and suggestions that improved this work. RVV thanks the STFC for support. ACF and JA acknowledge ERC Advanced Grant FEEDBACK. CSR is grateful for financial support from the Simons Foundation (through a Simons Fellowship in Theoretical Physics), a Sackler Fellowship (hosted by the Institute of Astronomy, Cambridge), and NASA under grant NNX14AF86G. CSR thanks the Institute of Astronomy at the University of Cambridge for their hospitality during an extended visit while this work was being performed. We thank Dom Walton for useful discussions on this work.
Paper: 2017ApJ...839....8T (acknowledgments)
We thank the anonymous referee for significantly improving this paper by pointing out uncertainties that had been missed. This work is supported by the International Partnership Program of the Chinese Academy of Sciences No.114A11KYSB20160008, the National Natural Science Foundation of China No. 11373038, and the National Key Basic Research Program of China (973 Program) 2015CB857100, the China Ministry of Science. D.L. acknowledges support from the “CAS Interdisciplinary Innovation Team” program. This work was carried out in part at the Jet Propulsion Laboratory, which is operated for NASA by the California Institute of Technology. M.K. acknowledges the support of Special Funding for Advanced Users, budgeted and administrated by Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS). N.M.M.G. acknowledges the support of the Australian Research Council through grant FT150100024. The Arecibo Observatory is operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968), and in alliance with Ana G Méndez-Universidad Metropolitana, and the Universities Space Research Association. CO data were observed with the Delingha 13.7 m telescope of the Qinghai Station of Purple Mountain Observatory. We appreciate all the staff members of the Delingha observatory and Zhichen Pan for their help during the observations.
Paper: 2016A&A...593A..67H (acknowledgments)
S.H. was supported by the German Research Foundation (DFG, grant We 1312/37-1), T.R. by the German Aerospace Center (DLR, grant 05 OR 1402). The TMAD service ( http://astro-uni-tuebingen.de/~TMAD ) used to compile atomic data for this paper was constructed as part of the activities of the German Astrophysical Virtual Observatory. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 093.D-0426. 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/ . This research made use of the SIMBAD database, operated at CDS, Strasbourg, France, and of NASA’s Astrophysics Data System.
Paper: 2017ApJ...846..151H (acknowledgments)
This work is based on observations with the NASA/ESA Hubble Space Telescope , which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. T.H. and S.B. were supported by grant HST GO 13862. V.W. acknowledges the support of the European Research Council via the award of a starting gant (SEDMorph: P.I. V. Wild). This project also made use of archival SDSS data. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max Planck-Institute for Astronomy (MPIA), the Max Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. T.H. thanks the Kavli Institute for Theoretical Physics, the Simons Foundation, and the Aspen Center for Physics for supporting informal workshops on galactic winds, feedback, and the circum-galactic medium during 2014, 2015, and 2016. These provided important input for this paper. Conversations at these workshops with Romeel Davé Crystal Martin, Norm Murray, Ralph Pudritz, Eliot Quataert, Brant Robertson, Chuck Steidel, Todd Thompson, and Ellen Zweibel were especially helpful. He also thanks Greg Bryan, Mark Voit, and Brian O‘Shea for interesting discussions of the possible importance of wind-driven precipitation. Facility: Sloan (COS) .
Paper: 2018MNRAS.476.5268M (acknowledgments)
ACKNOWLEDGEMENTS We gratefully acknowledge support from Australian Research Council (DMcN), and the Deutsche Forschungsgemeinschaft, the Land Niedersachsen (J-UG). The quantum chemical calculations performed in this work were supported by computational resources on the NCI Australia National Facility through the National Computational Merit Allocation Scheme.
Paper: 2016MNRAS.457..362B (acknowledgments)
The realization of this work was supported by the Hungarian OTKA NN grants 103244 and 114560.
Paper: 2017A&A...601A.110M (acknowledgments)
We thank the referee for a timely and constructive report that helped improve this paper. We would like to thank David Phillips and the members of the HARPS-N solar telescope team for sharing the data with us before their publication. The research leading to these results received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement number 313014 (ETAEARTH). A.C.C. acknowledges support from STFC grant ST/M001296/1.
Paper: 2019MNRAS.489.5030F (acknowledgments)
ACKNOWLEDGEMENTS The authors wish to thank Michelle Cluver, Jeffrey Newman, and Steven Bamford for helpful discussions, along with the anonymous referee for providing useful comments that improved the quality of this manuscript. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. 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.
Paper: 2018ApJ...855....5M (acknowledgments)
S.G.M. would like to thank Ian McCarthy and Ishiyama Tomoaki for access to and help with simulation data. A.S.G.R. acknowledges support of a UWA postdoctoral research fellowship, as well as an Australian Research Council (ARC) Discovery Project (DP) grant, DP140100395. The Centre for All-Sky Astrophysics (CAASTRO) is an Australian Research Council Centre of Excellence, funded by grant CE11E0090. This research has made use of NASA’s Astrophysics Data System.
Paper: 2015ApJ...805....4Z (acknowledgments)
The authors thank the referee for valuable suggestions and comments to improve the quality of this article. We gratefully acknowledge Y. N. Su, P. F. Chen, J. Zhang, B. Kliem, R. Liu, S. Gibson, H. Gilbert, M. D. Ding, and H. N. Wang for inspiring and constructive discussions. SDO is a mission of NASA's Living With a Star Program. AIA and HMI data are courtesy of the NASA/ SDO science teams. STEREO /SECCHI data are provided by a consortium of US, UK, Germany, Belgium, and France. QMZ is supported by Youth Fund of JiangSu BK20141043, by 973 program under grant 2011CB811402, and by NSFC 11303101, 11333009, 11173062, 11473071, and 11221063. H. Ji is supported by the Strategic Priority Research Program—The Emergence of Cosmological Structures of the Chinese Academy of Sciences, grant No. XDB09000000. Y.G. is supported by NSFC 11203014. Li Feng is supported by the NFSC grant 11473070, 11233008, and by grant BK2012889. Li Feng also thanks the Youth Innovation Promotion Association, CAS, for the financial support.
Paper: 2016MNRAS.459.1340S (acknowledgments)
We thank N. Schartel for the possibility to perform the ToO observation in the Director Discretionary Time, and the XMM–Newton team for the support for the observation. We gratefully acknowledge the Sardinia Regional Government for the financial support (P. O. R. Sardegna F.S.E. Operational Programme of the Autonomous Region of Sardinia, European Social Fund 2007-2013 – Axis IV Human Resources, Objective l.3, Line of Activity l.3.1). This work was partially supported by the Regione Autonoma della Sardegna through POR–FSE Sardegna 2007–13, L.R. 7/2007, Progetti di Ricerca di Base e Orientata, project no. CRP-60529. We also acknowledge financial contribution from the agreement ASI-INAF I/037/12/0. The High-Energy Astrophysics Group of Palermo acknowledges support from the Fondo Finalizzato alla Ricerca (FFR) 2012/13, project no. 2012- ATE-0390, founded by the University of Palermo.