adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019MNRAS.487.5062M (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for helpful comments and suggestions that have improved this manuscript. We thank Kathryn Disher for her helpful discussion. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship Program under Grant No. DGE1255832. Any opinions, findings, and conclusions or recommendations expressed in this material are those of the author and do not necessarily reflect the views of the National Science Foundation. This research has made use of the National Aeronautics and Space Administration Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program.
Paper: 2017A&A...608A..95M (acknowledgments)
T.M., M.V.d.S., and S.v.E. are supported by a grant from the Fondation ULB. This work has been partly funded by an Action de recherche concertée (ARC) from the Direction générale de l’Enseignement non obligatoire et de la Recherche scientifique – Direction de la recherche scientifique – Communauté française de Belgique. T.M. is supported by the FNRS-F.R.S. as temporary post-doctoral researcher under grant No. 2.4513.11. This work was supported by the Fonds de la Recherche Scientifique FNRS under grant No. T.0198.13. C.A. acknowledges to the Spanish grant AYA2015-63588-P within the European Founds for Regional Development (FEDER). M.T.C. acknowledges the financial support from the Spanish Ministerio de Economía y Competitividad, through grant AYA2013-40611-P. R.S. acknowledges support from the Polish Ministry of Science and Higher Education. This work was partly supported by the European Union FP7 programme through ERC grant number 320360 and by the Leverhulme Trust through grant RPG-2012-541. We acknowledge the support from INAF and Ministero dell’Istruzione, dell’Università e della Ricerca (MIUR) in the form of the grant “Premiale VLT 2012”. The results presented here benefit from discussions held during the Gaia -ESO workshops and conferences supported by the ESF (European Science Foundation) through the GREAT Research Network Programme. This research has made use of the Washington Double Star Catalogue maintained at the US Naval Observatory. This research has made use of the WEBDA database, operated at the Department of Theoretical Physics and Astrophysics of the Masaryk University. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of Python, in particular the Python module pyfits.py which is a product of the Space Telescope Science Institute, which is operated by AURA for NASA. This research has made used of the Digitized Sky Surveys which were produced at the Space Telescope Science Institute under US Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. 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. The authors thank the referee for his comments which helped to improve the manuscript.
Paper: 2016MNRAS.456.1666A (acknowledgments)
The authors acknowledge the anonymous referees for their valuable suggestions that have helped to improve this paper. The authors are also grateful to Takahiro Sumi for providing the MOA-II survey data. SA gratefully acknowledges the support from the Thai Government Scholarship and the University of Manchester President's Doctoral Scholar Award.
Paper: 2017MNRAS.468.3450C (acknowledgments)
Acknowledgments We thank an anonymous referee for comments that improved this paper. The Australia Telescope Compact Array (ATCA) is part of the Australia Telescope National Facility that is funded by the Australian Government for operation as a National Facility managed by CSIRO. This paper includes archived data obtained through the Australia Telescope Online Archive ( http://atoa.atnf.csiro.au ). This research has made use of the SIMBAD data base (Wenger et al. 2000 ), operated at CDS, Strasbourg, France. This research has made use of the VizieR catalogue (Ochsenbein, Bauer Marcout 2000 ) access tool, CDS, Strasbourg, France.
Paper: 2019A&A...631A..80B (acknowledgments)
Acknowledgements All calculations are run on MPCDF clusters Draco and Cobra. We thank Anish Amarsi for kindly providing us with the H collision rates computed using the Kaulakys recipe. This study is supported by SFB 881 of the DFG (subprojects A05, A10) and by the Research Council of Norway through its Centres of Excellence scheme, project number 262622. S.A.Y. and A.K.B. gratefully acknowledge support from the Ministry for Education and Science (Russian Federation), projects No. 3.5042.2017/6.7, 3.1738.2017/4.6. J.L. has received support through a grant from the Knut och och Alice Wallenberg foundation (2016.0019). Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant agreement no.: DNRF106). B.P. is partially supported by the CNES, Centre National d’Etudes Spatiales.
Paper: 2015ApJ...806..258M (acknowledgments)
This material is based upon work supported by the National Science Foundation (NSF) under grant AST-1211146 to C.W.M. We also gratefully acknowledge support by Chandra X-Ray Center award 1170050. C.S.K. is supported by NSF grant AST-1009756, and F.C. and G.M. are supported by the Swiss National Science Foundation (SNSF). This research made extensive use of the USNA high performance computing cluster. We thank the reviewer for valuable comments which improved the manuscript. Facilities: CTIO:2MASS (ANDICAM) , HST ( NICMOS , ACS ), Euler1.2 m , CXO (ACIS)
Paper: 2019MNRAS.487.1675A (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for their useful comments, and we are grateful to Stefania Marassi and Luca Graziani for their suggestions. MCA and MM acknowledge financial support from the Austrian National Science Foundation through FWF standalone grant P31154-N27 ‘Unraveling merging neutron stars and black hole–neutron star binaries with population synthesis simulations’. MM acknowledges financial support by the European Research Council for the ERC Consolidator grant DEMOBLACK, under contract no. 770017. MS acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie-Sklodowska-Curie grant agreement No. 794393. We acknowledge the Virgo Consortium for making their simulation data available. The eagle simulations were performed using the DiRAC-2 facility at Durham, managed by the ICC, and the PRACE facility Curie based in France at TGCC, CEA, Bruyères-le-Châtel.
Paper: 2018A&A...610A...4G (acknowledgments)
We thank S. Guilloteau and S. Bardeau for their help on the GILDAS software and J. M. Winters for helpful comments. This paper makes use of data from the following instruments: The Submillimeter Array (SMA project number 2011B-S052, 2012B-S004, and 2012B-S101), IRAM single dish telescope and interferometer (projects t020, v018), ALMA (ADS/JAO.ALMA#2013.1.01215.S). The work was partly supported by the CNRS program “Physique et Chimie du Milieu Interstellaire” (PCMI). M.G. also acknowledges support for travel by the SMA. We thank Spanish MICINN for funding support through grants AYA2006-14876, AYA2009-07304 and the CONSOLIDER program “ASTROMOL” CSD2009-00038, and the European Research Counil for funding support through the European Union’s Seventh Framework Program (FP/2007-2013)/ ERC Grant Agreement No. 610256 NANOCOSMOS.
Paper: 2019ApJ...879...86G (acknowledgments)
This work is funded by the NSFC of China (grant Nos. 11333006 and 11521303).
Paper: 2016A&A...596A...2B (acknowledgments)
The 1.5-m GREGOR solar telescope was built by a German consortium under the leadership of the Kiepenheuer-Institut für Sonnenphysik in Freiburg with the Leibniz-Institut für Astrophysik Potsdam, the Institut für Astrophysik Göttingen, and the Max-Planck-Institut für Sonnensystemforschung in Göttingen as partners, and with contributions by the Instituto de Astrofísica de Canarias and the Astronomical Institute of the Academy of Sciences of the Czech Republic. We are very grateful to the engineering, operating and technical staff at the GREGOR Telescope: Andreas Fischer, Olivier Grassin, Roberto Simoes, Clements Halbgewachs, Thomas Kentischer, Thomas Sonner, Peter Caligari, Michael Wiessschädel, Frank Heidecke, Stefan Semeraro, and Oliver Wiloth. We are also indebted to Franz Kneer and an anonymous referee for their comments on the paper. A.A.R. acknowledges financial support by the Spanish Ministry of Economy and Competitiveness through project AYA2014-60476-P and the Ramón y Cajal fellowships. This research has made use of NASA’s Astrophysics Data System.
Paper: 2019A&A...621A..59S (acknowledgments)
We thank Silvan Hunziker, Janis Hagelberg, and Jonas Kühn for valuable discussions, Dimitri Mawet for sharing the transmission profile of the AGPM coronagraph, and the referee for providing constructive comments that helped to improve the quality of this paper. TS acknowledges the support from the ETH Zurich Postdoctoral Fellowship Program. SPQ thanks the Swiss National Science Foundation (SNSF) for financial support under grant number 200021_169131. Part of this work was carried out within the framework of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation. SPQ acknowledges the financial support of the SNSF.
Paper: 2018MNRAS.476..470L (acknowledgments)
Acknowledgements We acknowledge the data from the Kepler Discovery mission, whose funding is provided by NASA's Science Mission Directorate. This work has also made use of data from the European Space Agency (ESA) mission Gaia , 1 processed by the Gaia Data Processing and Analysis Consortium (DPAC 2 ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. S.B. and Y.L. acknowledges the Joint Research Fund in Astronomy (U1631236) under cooperative agreement between the National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences (CAS), NSFC 11273007 and 10933002, and the Fundamental Research Funds for the Central Universities. EC has received fundings from the European Union's Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement no. 664931.
Paper: 2017A&A...607A..82M (acknowledgments)
We thank an anonymous referee for a prompt and positive report. We thank the Observatoire de Haute Provence for assistance with the T-193 telescope and the SOPHIE instrument. We warmly thank John Hillier for making the code CMFGEN available to the community and for constant help with it. L.M. acknowledges support from the Fonds National de la Recherche Scientifique (F.R.S.-F.N.R.S.) and through the ARC grant for Concerted Research Actions, financed by the French Community of Belgium (Wallonia-Brussels Federation).
Paper: 2020MNRAS.491..264G (acknowledgments)
ACKNOWLEDGEMENTS We thank our colleagues, including but not limited to Alexandre Correia, Zhengwei Liu, and Rosanne Di Stefano for valuable discussion in the course of this work. This work was jointly supported by the Natural Science Foundation of China (Grant No. 11521303), and the Science and Technology Innovation Talent Programme of Yunnan Province (Grant No. 2017HC018).
Paper: 2016MNRAS.462..689O (acknowledgments)
The authors thank Drs H. Hidaka and Y. Osamura for valuable discussion about reaction mechanisms. This study was supported in part by a Grant-in-Aid for Scientific Research from the Ministry of Education, Culture, Sports, Science and Technology of Japan and the Japan Society for the Promotion of Science ( JSPS; KAKENHI Grant Number JP26108501 ).
Paper: 2016ApJ...825...31P (acknowledgments)
The authors thank the referee for their careful reading of the paper. CP acknowledges support of Australian Research Council (ARC) Future Fellowship FT130100041 and Discovery Project DP130100117. ASGR acknowledges support of a University of Western Australia Research Fellowship. Both CP and ASGR acknowledge support of an ARC Discovery Project DP140100198. CP thanks Alexander Hobbs and Justin Read for making this version of GADGET-SPHS available. The research presented in this paper is undertaken as part of the Survey Simulation Pipeline (SSimPL; http://ssimpl.org/ ). This work was supported by resources provided by the Pawsey Supercomputing Centre with funding from the Australian Government and the Government of Western Australia.
Paper: 2019MNRAS.487.4238M (acknowledgments)
ACKNOWLEDGEMENTS 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. These observations are associated with programme #12310,#11522. The authors gratefully thank Dr. R. Bouwens and Dr. E. Wisnioski for sharing their catalogues. The authors are also thankful to the anonymous referee for comments and suggestions that helped improve the manuscript. AA, GÖ, and MH acknowledge the support of the Swedish Research Council (Vetenskapsrådet) and the Swedish National Space Agency (SNSA). MH acknowledges the continued support as a Fellow of the Knut and Alice Wallenberg Foundation.
Paper: 2020MNRAS.491.2346T (acknowledgments)
ACKNOWLEDGEMENTS The authors are grateful to the anonymous referee for very helpful suggestions. Numerical calculations have been made possible through a CINECA-ISCRA project and a CINECA-INFN agreement, providing access to resources on MARCONI at CINECA. We acknowledge financial support from the Accordo Attuativo ASI-INAF no. 2017-14-H.0 Progetto: on the escape of cosmic rays and their impact on the background plasma and from the INFN Teongrav collaboration. MB acknowledges support from the European Research Council (ERC starting grant no. 7153 68 MagBURST).
Paper: 2016ApJ...816...76L (acknowledgments)
This work was supported by the National Basic Research Program of China (973 program, grant No. 2012CB821800), the talent team of science and technology innovation in Guizhou Province (Grant No. (2015) 4015) and the National Natural Science Foundation of China (grant Nos 11373011, 11303069, 11225314, 11103021, 11565010, and 11165006). We would like to thank Dr. Dipanjan Mitra for sharing the 317 MHz pulse profile data observed with the GMRT and Dr. Ramesh Karuppusamy for sharing the 116.75–173.75 MHz pulse profile data observed with the Westerbork Synthesis Radio Telescope (WSRT). We would also like to thank the Kunming 40 m Radio Telescope and EPN teams for providing their pulse profiles. In particular, we would like to greatly thank Prof. Richard de Grijs for his kind help in carefully improving the language. We sincerely thank the anonymous referee for insightful suggestions and valuable comments.
Paper: 2020ApJ...889..128R (acknowledgments)
We thank IIT Indore for providing computing facilities necessary for the data analysis. We thank both the VLA and GMRT staff who made these radio observations possible. GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. R.R. is supported through ECR/2017/001296 grant awarded to A.D. by DST-SERB, India. M.R. would like to thank DST-India for INSPIRE fellowship program for financial support (IF160343). This research was supported in part by NASA ADAP grant NNX15AE17G. D.R. was supported by a NASA Postdoctoral Program Senior Fellowship at the NASA Ames Research Center, administered by the Universities Space Research Association under contract with NASA. Facilities: VLA , GMRT , CXO . Software: CASA (McMullin et al. 2007 ), SPAM (Intema et al. 2009 , 2017 ), XSPEC (Arnaud 1996 ), PyBDSF (Mohan Rafferty 2015 ), ClusterPyXT (Alden et al. 2019 ), CIAO (Fruscione et al. 2006 ), PROFFIT (Eckert et al. 2011 ).
Paper: 2017ApJ...849...54L (acknowledgments)
The authors would like to thank the anonymous referee for helpful comments and suggestions that improved the manuscript. This work is supported in part by NSF grant AST-1412768, NASA ATP grant NNX11AE07G, NASA Chandra grants GO213004B and GO7-18121X, NASA ASTRO-H (Hitomi) Science Support grant NNX16AD55G, the Research Corporation, and by the facilities and staff of the Yale Center for Research Computing. M.G. is supported by NASA through Einstein Postdoctoral Fellowship Award Number PF5-160137 issued by the Chandra X-ray Observatory Center, which is operated by the SAO for and on behalf of NASA under contract NAS8-03060. HPC resources were in part provided by the NASA/Ames HEC Program (SMD-16-7251). FLASH code was in part developed by the DOE NNSA-ASC OASCR Flash center at the University of Chicago. Part of the analysis were performed using the publicly-available yt package (Turk et al. 2011 ).
Paper: 2018A&A...613A..70S (acknowledgments)
Acknowledgements The CoRoT space mission, launched on December 27 2006, has been developed and was operated by CNES, with the contribution of Austria, Belgium, Brazil, ESA, Germany, and Spain. T.S. warmly thanks Cyril Georgy and Sylvia Ekström for discussions on the evolutionary tracks and Sébastien Salmon for the discussions on the instability trips. We are also very grateful to the referee, Dr. D. Baade, whose critical reading of the manuscript helped to improve the presentation of our results.
Paper: 2015ApJ...798...94W (acknowledgments)
This work was supported by NASA ADAP grant NNX09AC73G, Hubble Space Telescope grant HST-GO-13032, the IRD program at The Aerospace Corporation, and the University of Cincinnati Honors Program. We would like to thank Dr. Sascha Quanz, Dr. Munetake Momose, and the Astronomical Society of the Pacific Conference Series for permission to reproduce the images from their original publications. We would also like to thank the anonymous journal referee whose comments greatly improved this article.
Paper: 2017MNRAS.464...94N (acknowledgments)
We, in particular FN, NB, VKP and IP, gratefully acknowledge financial support for this project provided by NASA through grant HST -GO-14069 from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS526555. NB gratefully acknowledges financial support from the Royal Society (University Research Fellowship) and the European Research Council ( ERC-CoG-646928 , Multi-Pop). DG gratefully acknowledges support from the Chilean BASAL Centro de Excelencia en Astrofísica y Tecnologías Afines (CATA) grant PFB-06/2007 . MJC gratefully acknowledges support from the Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (subproject A8) of the German Research Foundation (DFG) . We are grateful to Jay Anderson for sharing with us his ePSF software. We thank the anonymous referee for useful comments and suggestions. Based on observations made with the NASA/ESA HST , 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).
Paper: 2019MNRAS.483.4086B (acknowledgments)
ACKNOWLEDGEMENTS MBK and AF acknowledge support from NSF grant AST-1517226. MBK was also partially supported by NASA grants NNX17AG29G and HST -AR-13888, HST -AR-13896, HST -AR-14282, HST -AR-14554, HST -GO-12914, and HST -GO-14191 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS5-26555. KNA is supported by NSF Theoretical Physics Grant No. PHY-1620638. DK was supported by NSF grant AST-1715101 and the Cottrell Scholar Award from the Research Corporation for Science Advancement. Support for SGK was provided by NASA through Einstein Postdoctoral Fellowship grant number PF5-160136 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060. CAFG was supported by NSF through grants AST-1412836, AST-1517491, AST-1715216, and CAREER award AST-1652522, by NASA through grant NNX15AB22G, and by a Cottrell Scholar Award from the Research Corporation for Science Advancement.
Paper: 2020ApJ...891...68C (acknowledgments)
We thank the anonymous referee for their comments and suggestions that helped to improve the paper. This work was supported by CONACyT (Consejo Nacional de Ciencia y Tecnología) research grant 280789 (México). R.A.A.-A. acknowledges support from the CONACyT program for PhD studies. Data from the Steward Observatory spectropolarimetric monitoring project were used. This program is supported by Fermi Guest Investigator grants NNX08AW56G, NNX09AU10G, NNX12AO93G, and NNX15AU81G http://james.as.arizona.edu/psmith/Fermi/ . The optical and near-infrared photometry are partly based on data collected by the WEBT collaboration and stored in the WEBT archive at the Osservatorio Astrofisico di Torino—INAF ( http://www.oato.inaf.it/blazars/webt/ ); for questions regarding their availability, please contact the WEBT President Massimo Villata ( massimo.villata@inaf.it ). the 1 mm flux density light-curve data from the Submillimeter Array were provided by Mark A. Gurwell. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. The authors thank A. Porras, E. Recillas, and G. Escobedo for their help with the observations as part of the Blazar NIR Monitoring Program at OAGH. Software: IRAF (Tody 1986 , 1993 ), FTOOLS (Blackburn 1995 ), XSPEC (Arnaud 1996 ), Fermitools (v 1.0.20).
Paper: 2015MNRAS.453..893S (acknowledgments)
It is a pleasure to thank Luca Amendola, Matthias Bartelmann, Alan Heavens, Tom Kitching and Björn Malte Schäfer for support and helpful discussions. This work has received financial support through the RTG Particle Physics beyond the Standard Model (DFG fund 1904), and the transregional collaborative research centre TR 33 ‘ The Dark Universe ’ of the German Science Foundation.
Paper: 2015ApJ...814...50D (acknowledgments)
The authors thank the anonymous referee for helpful comments that significantly improved the paper. The authors also thank Phil Uttley for useful and constructive comments. 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. G.P. acknowledges support via the Bundesministerium für Wirtschaft und Technologie/Deutsches Zentrum für Luft und Raumfahrt (BMWI/DLR, FKZ 50 OR 1408) and the Max Planck Society. T.M.-D. acknowledges support by the Spanish Ministerio de Economía y competitividad (MINECO) under grant AYA2013-42627. Facilities: XMM (EPIC pn) , RXTE (PCA).
Paper: 2016A&A...592A.139D (acknowledgments)
We thank the useful comments for the anonymous referee who helped in substantially improving the manuscript. We also thank René Heller for the helpful discussion. V.D. has been supported by the Hungarian OTKA Grant K104607, the Hungarian National Research, Development and Innovation Office (NKFIH) grant K-115709, the Lendület-2009 Young Researchers Program of the Hungarian Academy of Sciences, the TÉT-14FR-1-2015-0012 project, and the ESA PECS Contract No. 4000110889/14/NL/NDe. Á.K. has been supported by the Astrophysical and Geochemical Laboratory and the COST TD 1308 project. P.A. has been supported by the LP2012-31 project.
Paper: 2018MNRAS.477.4063M (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank the anonymous referee for very useful comments that contributed to the clarity and overall improvement of the paper.