adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019A&A...632A..36C (acknowledgments)
We thank the anonymous referee for the useful comments and suggestions that improved the manuscript. G.B.C, G.R. and K.I.C. acknowledge funding from the European Research Council through the award of the Consolidator Grant ID 681627-BUILDUP. C.G. acknowledges support by VILLUM FONDEN Young Investigator programme grant 10123. A.M. acknowledges funding from the INAF PRIN-SKA 2017 programme 1.05.01.88.04. K.U. acknowledges support from the Ministry of Science and Technology of Taiwan (grant MOST 106-2628-M-001-003-MY3) and from Academia Sinica (grant AS-IA-107-M01). R.D. gratefully acknowledges support from the Chilean Centro de Excelencia en Astrofísica y Tecnologías Afines (CATA) BASAL grant AFB-170002 This research made use of Astropy, ( http://www.astropy.org ) a community-developed core Python package for Astronomy ( Astropy Collaboration 2013 , 2018 ). This work made use of the CHE cluster, managed and funded by ICRA/CBPF/MCTI, with financial support from FINEP (grant 01.07.0515.00 from CT-INFRA – 01/2006) and FAPERJ (grants E-26/171.206/2006 and E-26/110.516/2012). This work made use of data taken under the ESO programme IDs 186.A-0798, 095.A-0525, 096.A-0105, 096.A-0650, 097.A-0909 and 098.A-0590.
Paper: 2017MNRAS.467..586M (acknowledgments)
Acknowledgments We thank the anonymous referee for a helpful report that allowed us to improve the manuscript. We thank Arwa Dabbech, Chiara Ferrari, Ivan Marti-Vidal, Stephen Wilkins and Ilana Feain for useful discussions. DM acknowledges support from the Science and Technology Facilities Council (grant number ST/M503836/1). MTS acknowledges support from a Royal Society Leverhulme Trust Senior Research Fellowship. PPP is supported by an Ernest Rutherford Fellowship. JS was supported in part by ERC Project No. 267117 (DARK) hosted by Universit Pierre et Marie Curie (UPMC) Paris 6. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research made use of aplpy , an open-source plotting package for python hosted at http://aplpy.github.com . This research made use of astropy , a community-developed core python package for Astronomy (Astropy Collaboration 2013 ).
Paper: 2016ApJ...828...24P (acknowledgments)
We thank the anonymous referee for their careful reading and constructive comments that improved the presentation of our work. 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 and the VizieR catalog access tool, CDS, Strasbourg, France. D.C.L. acknowledges support from NSF grants AST-1009571 and AST-1210311, under which part of this research was carried out. This research was also supported by NSF grants AST-1210599 (UA) and AST-1210372 (U. Denver). Some observations reported here were obtained at the MMT Observatory, a joint facility of the University of Arizona and the Smithsonian Institution.
Paper: 2020A&A...633A..56M (acknowledgments)
C. A. M. is supported by an Irish Research Council Government of Ireland Postgraduate Scholarship. E. P. C. is supported by the European Commission Horizon 2020 INFRADEV-1-2017 LOFAR4SW project, no. 777442. We would like to acknowledge NOAA’s National Centers for Environmental Information SUVI team for providing data on the 2017 September 2 event, particular thanks to Dan Seaton for preparing the data. We are grateful to the GOES, Wind and LASCO teams for open access to their data. I-LOFAR received funding from Science Foundation Ireland (SFI) grant no. 15/RI/3204. ORFÉES is part of the FEDOME project, partly funded by the French Ministry of Defense. We would like to thank Pietro Zucca for his assistance with the Zucca et al. (2014a) model.
Paper: 2019ApJ...870..133E (acknowledgments)
We wish to thank our colleagues in the CANDELS, 3D-HST, and CLEAR collaborations for their intense work to make these data sets usable. The authors thank the anonymous referee for their constructive report, which improved the quality and clarity of this paper. We also thank them (and others) for productive conversations, comments, suggestions, and information, including Charlie Conroy, Romeel Davé, Sandy Faber, Kristian Finlator, Rob Kennicutt, Marcin Sawicki, Corentin Schreiber, and Sarah Wellons. V.E.C. acknowledges generous support from the Hagler Institute for Advanced Study at Texas AM University. This work benefited from generous support from George P. and Cynthia Woods Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University. This work is based on data obtained from the Hubble Space Telescope through program number GO 14227. Support for program number GO 14227 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, Incorporated, under NASA contract NAS5-26555.
Paper: 2018ApJ...869...13J (acknowledgments)
Data from observations are courtesy of NASA SDO /AIA and the HMI science teams. The computational work was carried out on TianHe-1 (A) at the National Supercomputer Center in Tianjin, China. This work is supported by the National Natural Science Foundation of China (NSFC 41822404, 41731067, 41574170, 41531073), the Fundamental Research Funds for the Central Universities (grant No. HIT.BRETIV.201901), and Shenzhen Technology Project JCYJ20170307150645407. C.J. and Q.H. also acknowledge NSF grant AGS-1650854 and NASA grant 80NSSC17K0016 for partial support. R.L. acknowledges support by NSFC 41474151, 41774150, and 41761134088. P.V. acknowledges support by an INSPIRE grant of the AORC scheme under the Department of Science and Technology of India. We are very grateful to the anonymous referee for his meaningful comments and suggestions.
Paper: 2017MNRAS.465.2489T (acknowledgments)
Acknowledgments We thank Igor Soszynski for providing calibrated OGLE light curves of stars in our field. This work made use of python routines based on gatspy and astroML methods. This project was supported by DGAPA-UNAM grant through project IN106615. DMB acknowledges NPRP grant X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation). This work makes use of observations from the LCOGT network. This work has made a large use of the SIMBAD and ADS services.
Paper: 2016MNRAS.455.3848J (acknowledgments)
This paper arose, in part, out of discussions early on with Don VandenBerg, to whom the authors are grateful. SJ is a fellow of the Alexander von Humboldt Foundation. FH acknowledges funding through a Discovery Grant from NSERC. MP acknowledges support from the ‘Lendület-2014’ Programme of the Hungarian Academy of Sciences (Hungary) and from SNF (Switzerland). MP is also thankful for support from EuroGENESIS. MGB's research is supported by the US Department of Energy, Office of Nuclear Physics. BP is supported by the NSF under grants PHY 11- 25915, AST 11-09174, and ACI 13-39581.
Paper: 2015ApJ...804...75N (acknowledgments)
The authors are grateful to Makoto Sakuda and Tomonori Totani for valuable comments. We would also like to thank Yusuke Koshio for providing us the data of upper limits from Super-Kamiokande. In this work, numerical computations were partially performed on the supercomputers at Research Center for Nuclear Physics (RCNP) in Osaka University. This work was partially supported by Grants-in-Aids for the Scientific Research (No. 24105008, No. 26104006, No. 26105515, and No. 26870615) from MEXT in Japan.
Paper: 2018MNRAS.473..457R (acknowledgments)
Acknowledgements The author is grateful to the referee, Lothar Frommhold, for his valuable remarks which contributed to improving the quality of this work, and to Burkhard Militzer for useful comments and to share numerical data used in Fig. 9 . Valuable comments from A. Dewaele and C. Iglesias are also acknowledged. This research was supported by the Consejo Nacional de Investigaciones Científicas y Técnicas (CONICET, Argentina) through grant no. PIP 114-201101-00208 and the Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina) through Grant No. PICT 2016-1128.
Paper: 2016ApJ...832..192H (acknowledgments)
We would like to thank Jonathan Gair, James Guillochon, and Alberto Sesana for useful discussions and suggestions. C.J.H. acknowledges support from CIERA though a visiting pre-doctoral fellowship and a travel grant from the RAS. F.A. was supported by a CIERA postdoctoral fellowship and from a NASA Fermi Grant NNX15AU69G. We acknowledge the use of computing resources at CIERA funded by NSF PHY-1126812.
Paper: 2018MNRAS.481.2273C (acknowledgments)
ACKNOWLEDGEMENTS JC thanks the Science and Technology Facilities Council and the Royal Astronomical Society for their financial support. DA thanks the Royal Society, and the International Space Science Institute ( ISSI ) for its support. ND is supported by a Vidi grant from the Dutch Organisation for Scientific Research (NWO). TB acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0 between Istituto Nazionale di Astrofisica (INAF) and the Agenzia Spaziale Italiana (ASI). The authors acknowledge the use of astropy (Astropy Collaboration et al. 2013 ), numpy (Jones et al. 2001 ), and matplotlib (Hunter 2007 ) libraries for python . We also acknowledge the use of public data from the RXTE (Bradt et al. 1993 ) archive, as well as FTOOLS (Blackburn 1995 ) for data manipulation. Results provided by the ASM/ RXTE teams at MIT and at the RXTE Science Operations Facility and Guest Observer Facility at NASA’s Goddard Space Flight Centre.
Paper: 2017ApJ...841...39Y (acknowledgments)
Work by M.Y., K.W., S.D.R., and N.J.T. was supported by NASA grant NNX10AH28G and further work by M.Y. and S.D.R. was supported by NSF grant 1055910. This work was performed in part at the Jet Propulsion Laboratory, California Institute of Technology. N.J.T. was supported by grant 13-OSS13-0114 from the NASA Origins of Solar Systems program. M.Y. was supported by a Continuing Fellowship from the University of Texas at Austin. We acknowledge helpful input from L. Cleeves, E. Bergin, E.F. van Dishoeck, K. Öberg, J. Huang, M. Ansdell, and A. Kraus. We are grateful to Feng Long et al. ( 2017 ) for sharing their paper in advance of publication, and Huang et al. for sharing processed ALMA data for our model comparison. Software: RADMC ( http://www.ita.uni-heidelberg.de/dullemond/software/radmc-3d/ ), LIME (Brinch Hogerheijde 2010 ).
Paper: 2020ApJ...889...71B (acknowledgments)
This research has made use of data obtained with NuSTAR , a project led by the California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by NASA. We thank the NuSTAR Operations, Software and Calibration teams for support with the execution and analysis of these observations. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (USA). Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award Number GO6-17080X issued by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060. This research has made use of software provided by the Chandra X-ray Center (CXC) in the application package ciao . We also acknowledge the use of public data from the Swift data archive. D.J.W. acknowledges support from an STFC Ernest Rutherford Fellowship. Facilities: Chandra (ACIS) , NuSTAR , Swift (XRT).
Paper: 2015MNRAS.449.3137G (acknowledgments)
The authors would like to thank the anonymous referee for their very constructive comments. LG thanks R. Valiante for the invaluable support during the gamete refactoring and re-engineering. SS acknowledges support from the Netherlands Organization for Scientific Research (NWO), VENI grant 639.041.233. RS, AM and SS wish to thank the Osservatorio Astrofisico di Arcetri where the project was originally conceived and developed in successive meetings. The authors acknowledge Andrea Ferrara and Benedetta Ciardi for their very constructive comments. We also thank the 4C Institute at the Scuola Normale Superiore of Pisa for the computational resources necessary to develop and test gamesh . We also acknowledge PRACE 9 for awarding us access to the CEA HPC facility CURIE@GENCI 10 under the Type B project: High Performance Release of the gamesh Pipeline. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement no. 306476.
Paper: 2020MNRAS.491.1355D (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for the useful comments that improved the quality of the work. This project has received funding from the European Unions Horizon 2020 research and innovation programme under grant agreement No.607254; this publication reflects only the authors view, and the European Union is not responsible for any use that may be made of the information contained therein. SD acknowledges support from the Science and Technology Facilities Council (grant number ST/M503836/1). SO acknowledges support from the Science and Technology Facilities Council (grant number ST/L000652/1). We would like to thank M. P. Viero for his very useful help with the simstack code. The Herschel spacecraft was designed, built, tested, and launched under a contract to ESA managed by the Herschel or Planck Project team by an industrial consortium under the overall responsibility of the prime contractor Thales Alenia Space (Cannes), and including Astrium (Friedrichshafen) responsible for the payload module and for system testing at spacecraft level, Thales Alenia Space (Turin) responsible for the service module, and Astrium (Toulouse) responsible for the telescope, with in excess of a hundred subcontractors SPIRE has been developed by a consortium of institutes led by Cardiff University (UK) and including University of Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, University of Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, University of Sussex (UK); and Caltech, JPL, NHSC, University of Colorado (USA). This development has been supported by national funding agencies CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC, UKSA (UK); and NASA (USA).
Paper: 2016A&A...587A..40P (acknowledgments)
We thank the referee for comments that help us to improve the manuscript. We acknowledge the 2011 PRIN-INAF grant for financial support. We acknowledge the financial support of the UnivEarthS Labex program at Sorbonne Paris Cité (ANR-10-LABX-0023 and ANR-11-IDEX-0005-02). G.G. thanks the Observatoire de Paris (Meudon) for support and hospitality during the completion of this work. We thank S. Campana and G. Tagliaferri for contributing to useful discussions.
Paper: 2017A&A...599A..51P (acknowledgments)
The Planck Collaboration acknowledges the support of: ESA; CNES, and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, J.A., and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/planck-collaboration . The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement No. 267934.
Paper: 2017MNRAS.467.3279R (acknowledgments)
Acknowledgments This research was supported by projects GOA/2015-014 (2014-2018 KU Leuven) and the Interuniversity Attraction Poles Programme by the Belgian Science Policy Office (IAP P7/08 CHARM) The computational resources and services used in this work were provided by the VSC (Flemish Supercomputer Center), funded by the Research Foundation Flanders (FWO) and the Flemish Government department EWI. BR likes to thank Lorenzo Sironi, Fabio Bacchini, Norbert Magyar, Jannis Teunissen, Kirit Makwana, Matthieu Leroy and Dimitris Millas for fruitful discussions and comments.
Paper: 2015MNRAS.450.3811M (acknowledgments)
DM would like to thank Philip Massey, Scott Adams, Michael Fausnaugh, Rubab Khan, Ben Shappee and Obright Lorain for helpful discussions that contributed greatly to this paper. We also wish to thank the anonymous referee, who provided numerous useful comments and aided the betterment of this manuscript. Based on observations made with the NASA GALEX . 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 NNX13AC07G and by other grants and contracts. Some/all 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.
Paper: 2018A&A...613L..10O (acknowledgments)
Acknowledgements The authors thank the referee for their very useful comments. This work has been financially supported by the Programme National Hautes Energies (PNHE), project 994584. LO and AN thank Integrated Activities in the High Energy Astrophysics Domain project for support that enabled this work. L.O. acknowledges support from the DLR grant 50 OR 1612. TB was supported by the FNP grant TEAM/2016-3/19. LO and TB thank Kavli Institute for Theoretical Physics, University of California, where this project have been initiated, for their support. This research has made use of the SIMBAD database, the VizieR catalogue access tool, operated at CDS, Strasbourg, France, and the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. The scientific results reported in this article are based to a significant degree on the data obtained from the Chandra and XMM-Newton Data Archives.
Paper: 2016MNRAS.458.2928C (acknowledgments)
EC acknowledges the support of the Royal Astronomical Society via a RAS Research Fellowship. EC would like to thank Ajinkya Patil, Cathryn Trott, Jonathan Pritchard, Geraint Harker and Harish Vedantham for useful discussions. FBA acknowledges the support of the Royal Society via a University Research Fellowship. VJ would like to thank the Netherlands Foundation for Scientific Research (NWO) for financial support through VENI grant 639.041.336. The work involving oskar was performed using the Darwin Supercomputer of the University of Cambridge High Performance Computing Service ( http://www.hpc.cam.ac.uk/ ), provided by Dell Inc. using Strategic Research Infrastructure Funding from the Higher Education Funding Council for England and funding from the Science and Technology Facilities Council.
Paper: 2015MNRAS.452.3106M (acknowledgments)
J-M M acknowledges financial support from the Spanish Ministerio de Economía y Competitividad (grants AYA2013-40979-P, and AYA2013-48226-C3-2-P) and from the local Autonomous Government (Generalitat Valenciana, grant Prometeo-II/2014/069). The author also acknowledges fruitful discussions with Professors J. A. Miralles and M. Perucho, and the anonymous referee for comments and criticism that helped to improve this manuscript.
Paper: 2019MNRAS.489.3870S (acknowledgments)
ACKNOWLEDGEMENTS We are grateful to the anonymous referee for his/her thoughtful and constructive comments which enabled us to improve the first edition of this paper. This work has been supported financially by Research Institute for Astronomy and Astrophysics of Maragha (RIAAM) under research project No. 1/6275-1.
Paper: 2015A&A...578A..45P (acknowledgments)
C. S. Peri and P.B. are supported by the ANPCyT PICT-2012/00878. P.B. also acknowledges support from CONICET PIP 0078 and UNLP G11/115 projects. This publication makes uses 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. We thank the SIMBAD database, operated at CDS, Strasbourg, France, and 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. We also thank the HubbleSite, which is produced by the Space Telescope Science Institute (STScI). STScI is operated by the Association of Universities for Research in Astronomy, Inc. (AURA) for NASA, under contract with the Goddard Space Flight Center, Greenbelt, MD. The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency (ESA). We thank 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). Finally, we appreciate the suggestions of A. Noriega-Crespo, and insightful discussions with M. V. del Valle and L. J. Pellizza. We thank the anonymous AA referee for comments and suggestions that improved the article.
Paper: 2016A&A...595A.102B (acknowledgments)
OSIRIS was built by a consortium of the Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany, CISAS-University of Padova, Italy, the Laboratoire d’Astrophysique de Marseille, France, the Instituto de Astrofísica de Andalucia, CSIC, Granada, Spain, the Research and Scientific Support Department of the European Space Agency, Noordwijk, The Netherlands, the Instituto Nacional de Técnica Aeroespacial, Madrid, Spain, the Universidad Politéchnica de Madrid, Spain, the Department of Physics and Astronomy of Uppsala University, Sweden, and the Institut für Datentechnik und Kommunikationsnetze der Technischen Universität Braunschweig, Germany. VIRTIS was built by a consortium from Italy, France, and Germany, under the scientific responsibility of IAPS, Istituto di Astrofisica e Planetologia Spaziali of INAF, Rome, which lead also the scientific operations. The VIRTIS instrument development for ESA has been funded and managed by ASI (Italy), with contributions from Observatoire de Meudon (France) financed by CNES and from DLR (Germany). The VIRTIS instrument industrial prime contractor was former Officine Galileo, now Finmeccanica in Campi Bisenzio, Florence, Italy. The support of the national funding agencies of Germany (DLR), France (CNES), Italy (ASI), Spain (MEC), Sweden (SNSB), and the ESA Technical Directorate is gratefully acknowledged.