adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017ApJ...834..125W (acknowledgments)
We gratefully acknowledge the developers of iSALE-2D, including Gareth Collins, Kai Wunnemann, Dirk Elbeshausen, Boris Ivanov and Jay Melosh. Numerical computations were carried out on the PC cluster at Center for Computational Astrophysics, National Astronomical Observatory of Japan. We thank the referee, H.J. Melosh for helpful suggestions and comments. S.W. thank Alexander N. Krot for helpful comments and discussions on chondrules and also thank Brandon C. Johnson and Kosuke Kurosawa for kindly comments on simulations. The part of this research was carried out at JPL/Caltech under a contract with NASA. Y.H. is supported by JPL/Caltech.
Paper: 2015ApJ...805...46T (acknowledgments)
This research was partially supported by the Italian Space Agency (ASI) under contracts I/013/12/0 and I/022/10/2 and by the European Commission’s Seventh Framework Program under the grant agreement STORM (project n° 313038). Data from Wind and Messenger were obtained from NASA-CDAWeb and NASA-PDS websites, respectively.
Paper: 2017ApJ...849..160H (acknowledgments)
We acknowledge the financial support of the UnivEarthS Labex program at Sorbonne-Paris-Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02) through project SolarGeoMag. We also acknowledge the support from the ERC PoC SolarPredict project, CNES Solar Orbiter and INSU/PNST grants, and Idex SPC through the DAMSE project. We are grateful to Roger Ulrich for giving us digital access to his surface meridional circulation measurements. We also thank SIDC for access to their sunspot series observations. Wilcox Solar Observatory data used in this study were obtained via the Web site http://wso.stanford.edu on 2017 September 29 03:15:25 PDT, courtesy of J.T. Hoeksema. A.S.B. thanks M. DeRosa and A. Title for useful discussions. Numerical computations were performed on the S-CAPAD platform, IPGP, France and on the DIM-ACAV funded Anais server at CEA/IRFU. IPGP contribution 3889.
Paper: 2017ApJ...845...81P (acknowledgments)
We thank the anonymous referee for useful comments. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award Number GO5-16133X issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics and Space Administration under contract NAS8-03060. R.J.W. is supported by a Clay Fellowship awarded by the Harvard-Smithsonian Center for Astrophysics. W.R.F., C.J., and F.A.-S. acknowledge support from the Smithsonian Institution. F.A.-S. acknowledges support from Chandra grant GO3-14131X. Basic research in radio astronomy at NRL by TEC is supported by 6.1 Base funding. M.N. acknowledges PRIN-INAF 2014 1.05.01.94.02. This research made use of APLpy, an open-source plotting package for Python (Robitaille Bressert 2012 ). This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration et al. 2013 ).
Paper: 2015A&A...574L...3K (acknowledgments)
Cs. K. has been supported by the PECS grant # 4000109997/13/NL/KML of the HSO ESA, the K-104607 grant of the Hungarian Research Fund (OTKA), and the LP2012-31 “Lendület” grant of the Hungarian Academy of Sciences. We are indebted to our referee for the useful comments.
Paper: 2017MNRAS.470.1971V (acknowledgments)
Acknowledgements This study is based on observations with XMMNewton , an ESA Science Mission with instruments and contributions directly funded by ESA Member states and the USA (NASA), and with Swift , a NASA mission with international participation. We would like to thank the anonymous referee for the useful comments and suggestions that helped improve the manuscript. The XMMNewton project is supported by the Bundesministerium fr Wirtschaft und Technologie/Deutsches Zentrum fr Luft- und Raumfahrt (BMWi/DLR, FKZ 50 OX 0001) and the Max-Planck Society. The OGLE project has received funding from the European Research Council under the European Communitys Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no. 246678 to AU. We thank the Swift team for accepting and carefully scheduling the target of opportunity observations, and we acknowledge the use of public data from the Swift data archive. GV acknowledges support from the BMWi/DLR grant FKZ 50 OR 1208. PM acknowledges support by the Centre National dtudes Spatiales (CNES). Last but not least, we wish to thank Dr. M. Petropoulou and Dr. F. Koliopanos for their useful comments.
Paper: 2017MNRAS.466.2922P (acknowledgments)
Acknowledgments The authors would like to thank Julian Krolik, Joe Silk, Meng Su and Ilias Cholis for useful discussions. We especially thank Glennys Farrar for valuable detailed comments on an earlier draft. This work was supported by NSF Grant No. 0244990, NASA NNX15AB18G, the John Templeton Foundation and the Simons Foundation.
Paper: 2019A&A...624A..94M (acknowledgments)
Acknowledgements This research was supported by the Italian Ministry of Education, University, and Research through the PREMIALEWOW 2013 research project under grant Ricerca di pianeti intorno a stelle di piccola massa. J.M. acknowledges support from the Ariel ASI-INAF agreement N. 2015-038-R.0. E.V. and C.E. acknowledge support from the On the rocks project funded by the Spanish Ministerio de Economía y Competitividad under grant AYA2014-55840-P. We sincerely appreciate the careful reading of the manuscript and the constructive comments of the anonymous referee.
Paper: 2016MNRAS.455..859S (acknowledgments)
We thank Chris Belczynski for providing tabulated data to map between ZAMS stellar masses and final compact remnant masses, and Tod Lauer for assistance in interpreting the Nuker data sets. We thank Iair Arcavi and Suvi Gezari for providing useful data on the peak luminosities of observed TDEs. We thank Brad Cenko, Jacqueline van Gorkum, Morgan MacLeod, Jeremiah Ostriker, Greg Snyder, Linda Strubbe, and Sjoert van Velzen for helpful conversations. Finally, we also thank the anonymous referee for many useful suggestions. BDM gratefully acknowledges support from the NSF grant AST-1410950 and the Alfred P. Sloan Foundation. This work was supported in part by the National Science Foundation under Grant No. PHYS-1066293 and the hospitality of the Aspen Center for Physics.
Paper: 2018A&A...616A.154G (acknowledgments)
I am grateful to the anonymous referee for the helpful comments that allowed me to improve the paper.
Paper: 2016ApJ...833..196M (acknowledgments)
We acknowledge A.J. Koning for development of the nuclear reaction code TALYS, his help in using the code, and his willingness to answer questions concerning nuclear physics. This work was supported by NASA grant NNH13AV36I and the Chief of Naval Research (CNR). B.K. acknowledges the Israeli Science Foundation for support. G.S. was supported by NSF/SHINE grant 1156092.
Paper: 2018ApJ...866..123M (acknowledgments)
Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award Number G04-15114X to S.M. 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. Support for the HST program number GO-13185 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. K.D.D. was supported by an NSF AAPF fellowship awarded under NSF grant AST-1302093 while she worked on this project. M.V. gratefully acknowledges support from the Danish Council for Independent Research via grant number DFF 4002-00275.
Paper: 2016MNRAS.456.2900A (acknowledgments)
We warmly thank Simon Goodwin, this papers referee, for his enlightened and useful comments that have helped to improve the content and presentation of this work. Likewise, we also wish to thank Richard Parker for his reading of the draft and the discussion held concerning specific points of the paper. We acknowledge support from the Spanish Ministry for Economy and Competitiveness and FEDER funds through grant AYA2013-40611-P.
Paper: 2016MNRAS.458.2371R (acknowledgments)
We thank Jeremiah P. Ostriker, Gurtina Besla, and Benedikt Diemer for useful comments and discussions. SG acknowledges support provided by NASA through Hubble Fellowship grant HST-HF2-51341.001-A awarded by the STScI, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. VS acknowledges support through the European Research Council through ERC-StG grant EXAGAL-308037. LH acknowledges support from NSF grant AST-1312095 and NASA grant NNX12AC67G. Simulations were run on the Harvard Odyssey and CfA/ITC clusters, the Ranger and Stampede supercomputers at the Texas Advanced Computing Center as part of XSEDE, the Kraken supercomputer at Oak Ridge National Laboratory as part of XSEDE, the CURIE supercomputer at CEA/France as part of PRACE project RA0844, and the SuperMUC computer at the Leibniz Computing Centre, Germany, as part of project pr85je.
Paper: 2016MNRAS.460.1086M (acknowledgments)
We thank Kassandra Anderson for useful discussions and Cristóbal Petrovich for comments on the manuscript. We also thank the referee Smadar Naoz for a constructive report. This work has been supported in part by NSF grant AST-1211061, and NASA grants NNX14AG94G and NNX14AP31G.
Paper: 2016A&A...591A..45P (acknowledgments)
This research has made use of the Exoplanet Orbit Database and the Exoplanet Data Explorer at exoplanets.org . The project has been supported by Swiss National Science Foundation grants 200021-138016, 200020-15710 and 200020-160119. A.A.V. acknowledges support from an Ambizione Fellowship of the Swiss National Science Foundation.
Paper: 2016A&A...592A.158H (acknowledgments)
We thank Joachim Puls for his advice and for the fastwind comparison models; Rolf Kudritzki for making the optical observations available to us; and Miguel Urbaneja for sharing his original CSPN model runs. We also thank the anonymous referees for helpful comments which improved the paper. This work was supported by the Deutsche Forschungsgemeinschaft (DFG) under grants Pa 477/4-1 and Pa 477/7-1.
Paper: 2015MNRAS.450.2692V (acknowledgments)
The authors acknowledge the anonymous referee for very useful comments and suggestions. JV acknowledges the support of ESO through a studentship. JV and MB acknowledge the support of the Fund for Scientific Research Flanders (FWO-Vlaanderen). The authors are grateful to CTIO for the hospitality and the dedicated assistance during the numerous observing runs.
Paper: 2016ApJ...832...31V (acknowledgments)
The authors thank R.G. Bhaskar and V. Wakelam for stimulating conversations. We also thank the anonymous referee for their valuable comments. This work was supported in part by the NSF Division of Astronomical Sciences Astronomy and Astrophysics Grants Program and by the NASA Astronomy and Physics Research and Analysis Program. X.U. is Senior Research Associate of the FRS-FNRS. S.V. was supported in part by the NSF Research Experience for Undergraduates program.
Paper: 2019MNRAS.488..706H (acknowledgments)
ACKNOWLEDGEMENTS Support for this work was provided by NASA through grant number JWST-ERS-01324 and HST-GO-15212 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. Support was also provided through NSF grant: COLLABORATIVE RESEARCH: The Final Frontier: Spectroscopic Probes of Galaxies at the Epoch of Reionization (AST 1815458, AST 1810822). The Cosmic Dawn Center is funded by the DNRF. MB acknowledges support by NSF through award NSF-AAG-1815458 and through NASA ADAP grant 80NSSC18K0945. The authors wish to thank Simon Birrer for helpful discussions during the development of the Bayesian inference analysis.
Paper: 2015MNRAS.452..368Y (acknowledgments)
The authors thank the anonymous referee for his/her constructive comments that greatly helped to improve the content of this manuscript. This work is financially supported by National Natural Science Foundation of China (grants no. 11273068, 11473073, 11403105), the Strategic Priority Research Program-The Emergence of Cosmological Structures of the Chinese Academy of Sciences (grant no. XDB09000000), the innovative and interdisciplinary program by CAS (grant no. KJZD-EW-Z001), the Natural Science Foundation of Jiangsu Province (grant no. BK20141509) and the Foundation of Minor Planets of Purple Mountain Observatory.
Paper: 2017A&A...607A..89B (acknowledgments)
We thank the anonymous referee for his/her very useful and constructive comments. We thank Y.-Y. Mao for providing the abundance matching code and for assistance. We thank Eric Jullo, Stéphane Arnouts, Olivier Ilbert, and Corentin Schreiber for their explanations. The Bolshoi-Planck simulation was performed by Anatoly Klypin within the Bolshoi project of the University of California High-Performance AstroComputing Center (UC-HiPACC) and was run on the Pleiades supercomputer at the NASA Ames Research Center. We acknowledge financial support from “Programme National de Cosmologie and Galaxies” (PNCG) funded by CNRS/INSU-IN2P3-INP, CEA and CNES, France. This work has been partially funded by the ANR under the contract ANR-15-CE31-0017. This work has been carried out thanks to the support of the OCEVU Labex (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the “Investissements d’Avenir” French government program managed by the ANR. H.W. acknowledges the support by the US National Science Foundation (NSF) grant AST1313037. Part of the research described in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Paper: 2017ApJ...850..123S (acknowledgments)
This research was supported by NSF grants AST-1515568 and AST-1140030. The Kitt Peak 12 m and the SMT are operated by the Arizona Radio Observatory (ARO), with partial support through the NSF University Radio Observatories (URO) program (AST-1140030).
Paper: 2020ApJ...889..123S (acknowledgments)
We are grateful to Andrej Dundovic for useful discussions as well as the comments of the unknown referee that helped to improve the original version of the paper. L.S., A.F., and B.E. acknowledge financial support from the MERCUR project An-2017-0009. Software: CRPropa3 (Alves Batista et al. 2016 ), NumPy (van der Walt et al. 2011 ), Matplotlib (Hunter 2007 ), SymPy (Meurer et al. 2017 ), Pandas (McKinney 2010 ).
Paper: 2019MNRAS.487.2296T (acknowledgments)
ACKNOWLEDGEMENTS Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 088.D-0096(A) and 095.D-0973(A). This research has used the SIMBAD data base, operated at CDS, Strasbourg, France, and of the NASA’s Astrophysics Data System. iraf is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation. Tom Marsh is thanked for developing and sharing his package molly . We thank the anonymous referee for constructive comments. MAPT and JC acknowledge support by the Spanish Ministry of Economy, Industry, and Competitiveness (MINECO) under grant AYA2017-83216-P. MAPT also acknowledges support via a Ramón y Cajal Fellowship (RYC-2015-17854). The work of SR was supported by the Netherlands Research School for Astronomy (NOVA). PGJ and ZKR acknowledge support from European Research Council Consolidator grant 647208. RIH and CBJ acknowledge support from NASA through Chandra Award Number AR3-14002X 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 LW has been supported by the Polish National Science Centre grant no.DEC-2011/03/B/ST9/02573. The OGLE project has received funding from the National Science Centre, Poland, grant MAESTRO 2014/14/A/ST9/00121 and 2015/18/M/ST9/00544 to Andrzej Udalski. COH is supported by NSERC Discovery grant RGPIN-2016-04602, and a Discovery Accelerator Supplement. SR is thankful to Hagai Perets for his insights on the triple scenario.
Paper: 2020A&A...634A..65D (acknowledgments)
This work is based on observations obtained with XMM-Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. This research has made use of data obtained with the NuSTAR mission, a project led by the California Institute of Technology (Caltech), managed by the Jet Propulsion Laboratory (JPL) and funded by NASA. BDM acknowledges support from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 798726, and grant agreement No. 665778 via the Polish National Science Center grant Polonez 2016/21/P/ST9/04025. TPA acknowledges support from Polish National Science Center grant Polonez 2016/21/P/ST9/04025 and Preludium 2016/21/N/ST9/0331. S. B. acknowledges financial support from ASI under grants ASI-INAF I/037/12/0 and n. 2017-14-H.O. AGM acknowledges partial support from Nardowe Centrum Nauki (NCN) award 2016/23/B/ST9/03123. JM is supported by STFC (UK) through the University of Strathclyde UK APAP network grant ST/R000743/1. D. J. W. acknowledges support from STFC in the form of an Ernest Rutherford fellowship. C. P. is supported by European Space Agency (ESA) Research Fellowship. POP thanks financial support from the CNES french agency and the CNRS/PNHE. AR was supported by Polish National Science Center grants No. 2015/17/B/ST9/03422 and 2015/18/M/ST9/00541. The authors thank the referee for their helpful comments.
Paper: 2017ApJ...842...81K (acknowledgments)
We thank the anonymous referee for the constructive comments and suggestions, which helped to improve the manuscript. GAMA is a joint European-Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalog is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel-ATLAS, GMRT, and ASKAP, providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA web site is http://www.gama-survey.org/ . The Radio Semi-Analytic Galaxy Evolution (Radio-SAGE) model used in this study is a publicly available for download at https://github.com/mojtabaraouf/sage . The Millennium Simulation was carried out by the Virgo Supercomputing Consortium at the Computing Centre of the Max Plank Society in Garching.
Paper: 2019ApJ...878..139T (acknowledgments)
Work by J.K. is supported in part by a research project hosted by Waseda Research Institute for Science and Engineering, also by Institute for Advanced Theoretical and Experimental Physics, Waseda university. We thank anonymous referees for carefully reading our manuscript and for giving useful comments. Software: HEASoft (v6.19), CIAO (v4.8).
Paper: 2020MNRAS.491.4310T (acknowledgments)
ACKNOWLEDGEMENTS This work has been funded by VIALACTEA, a Collaborative Project under Framework Programme 7 of the European Union (Contract n. 607380). ADC acknowledges support from the Science and Technology Facilities Council (under grant ST/N00706/1). This work is based on observations carried out under project number 133-15 with the IRAM 30-m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain).
Paper: 2018A&A...614A..34D (acknowledgments)
Acknowledgements We thank the anonymous referee for the useful comments that improved the manuscript. L.D. thanks Jun Yang for answering some questions about the library of X-ray pulsars in SMC. This paper is based on data from observationswith, XMM-Newton , Swift , and Chandra X-ray observatory. XMM-Newton is an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. Chandra data were obtained from the Chandra Data Archive. This paper is based on data from observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Spain, and Switzerland), Czech Republic, and Poland, and with the participation of Russia and the USA. This work is supported by the Bundesministerium für Wirtschaft und Technologie through the Deutsches Zentrum für Luft und Raumfahrt (grant FKZ 50 OG 1602). P.R. acknowledges contract ASI-INAF I/004/11/0.
Paper: 2019MNRAS.483.3910C (acknowledgments)
ACKNOWLEDGEMENTS We thank an anonymous referee for helpful comments. SC acknowledge NCRA-TIFR for providing financial support. We acknowledge the THINGS collaboration for providing the data for galaxy NGC 628.
Paper: 2016ApJ...831...65B (acknowledgments)
We thank the referee for a valuable report that greatly helped us to clarify the paper. This work was supported by NSF grants AST/110897 and AST/12117937.
Paper: 2016MNRAS.458..772Z (acknowledgments)
We thank the anonymous referee for helpful suggestions that improved the quality of the paper. LZ and YS acknowledge support for this work from the National Natural Science Foundation of China (grant 11373021), the Strategic Priority Research Program ‘The Emergence of Cosmological Structures’ of the Chinese Academy of Sciences (grant No. XDB09000000), and Excellent Youth Foundation of Jiangsu Scientific Committee (grant BK20150014). LZ also thanks for the support by the National Natural Science Foundation of China (Grant No. J1210039). AL is supported in part by NSF AST-1311804 and NASA NNX14AF68G. This research has made extensive 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 work is based (in part) on observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA.’ The Galaxy Evolution Explorer ( GALEX ) is a NASA Small Explorer, launched in 2003 April. We acknowledge NASA's support for construction, operation, and science analysis for the GALEX mission.
Paper: 2016A&A...593A..42T (acknowledgments)
This work is supported by Technology under State Key Development Program for Basic Research (973 program) No. 2012CB821802 and National Key Basic Research Program of China (973 Program) 2015CB857100, the China Ministry of Science, and the Guizhou Scientific Collaboration Program (#20130421). We are grateful to the anonymous referee for his/her constructive suggestions, which have greatly improved this paper. The authors would like to thank Pei Zuo for helping Delingha CO observations, John Dickey for discussing H i self-absorption, Xiaohu Li for discussing chemical evolutionary model. We thank the Pineda team for providing C and CO data. Part of CO data were observed with the Delingha 13.7 m telescope of the Qinghai Station of Purple Mountain Observatory. We appreciate the help of all the staff members of the observatory during the observations.