adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019ApJ...885..154K (acknowledgments)
This research has received funding by the Sêr Cymru II, part-funded by the European Regional Development Fund through the Welsh Government. H.M. is partly funded by an STFC consolidated grant to Aberystwyth University. The Swedish 1 m Solar Telescope is operated on the island of La Palma by the Institute for Solar Physics of Stockholm University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. The Institute for Solar Physics is supported by a grant for research infrastructures of national importance from the Swedish Research Council (registration number 2017-00625). The work of D.K. was supported by Georgian Shota Rustaveli National Science Foundation project FR17_323. J.K. acknowledges the project VEGA 2/0004/16. This work was also supported by the project ITMS No. 26220120029, based on the operational Research and Development Program financed from the European Regional Development Fund. The authors acknowledge support from the grant 19-17102S of the Czech Funding Agency. P.H. was supported also by the grant 19-09489S. S.J. acknowledges the financial support from the Slovenian Research Agency No. P1-0188. The data were acquired within Spanish SST time allocation. This research has made use of NASA’s Astrophysics Data System. The authors wish to thank the anonymous referee who provided constructive remarks that greatly improved the quality of this paper. Facilities: SST (CRISP , CHROMIS).
Paper: 2017MNRAS.469.1655K (acknowledgments)
Acknowledgments BK, SK and LT acknowledge Shota Rustaveli National Science Foundation and Ilia State University for the fundamental research grant FR/377/6-290/14. KM and DD acknowledge the funding by the German BMBF (Verbundforschung Astro- und Astroteilchenphysik) and HAP (Helmholtz Alliance for Astro-particle Physics). PR acknowledges the contract ASI-INAF I/004/11/0. We acknowledge the helpful service of heasarc , and the use of public data from the Swift and Fermi archives. This research has made use of the xrtdas software, developed under the responsibility of the ASDC, Italy, and the data from the OVRO 40-m monitoring programme that is supported in part by NASA grants NNX08AW31G and NNX11A043G, and NSF grants AST-0808050 and AST-1109911. In our study, the data from the Steward Observatory spectropolarimetric monitoring project supported by Fermi Guest Investigator grants NNX08AW56G, NNX09AU10G, NNX12AO93G and NNX15AU81G were used. We thank the FACT Collaboration for making their analysis results publicly available, and appreciate their long-term monitoring initiative that provides precious input for MWL studies. We thank the anonymous referee for his/her very useful comments and suggestions that helped to improve the quality of the paper.
Paper: 2017MNRAS.472L.109A (acknowledgments)
Acknowledgements DAA acknowledges support by a CIERA Postdoctoral Fellowship. CAFG was supported by NSF grants AST-1412836 and AST-1517491, NASA grant NNX15AB22G, STScI grant HST-AR-14562.001 and CXO grant TM7-18007X. EQ was supported by NASA ATP grant 12-ATP-120183, a Simons Investigator award from the Simons Foundation, and the David and Lucile Packard Foundation. Support for PFH was provided by an Alfred P. Sloan Research Fellowship, NASA ATP Grant NNX14AH35G, and NSF grant AST-1411920 and CAREER award #1455342. RF acknowledges support from the Swiss National Science Foundation (grant no. 157591). PT acknowledges support from NASA through Hubble Fellowship grant HST-HF-51384.001-A awarded by STScI. AW was supported by a Caltech-Carnegie Fellowship, the Moore Center for Theoretical Cosmology and Physics at Caltech and NASA grant HST-GO-14734 from STScI. DK was supported by NSF Grant AST1412153 and a Cottrell Scholar Award from the Research Corporation for Science Advancement. The simulations were run using XSEDE, supported by NSF grant ACI-1053575, and Northwestern Universitys compute cluster Quest.
Paper: 2018ApJ...865...34C (acknowledgments)
We thank the referee for a very helpful report. C.-Y.C. is grateful for the support from Virginia Institute of Theoretical Astronomy (VITA) at the University of Virginia through the VITA Postdoctoral Prize Fellowship, and the support partly from NSF grant AST-1815784. The work of E.C.O. was supported by grant 510940 from the Simons Foundation.
Paper: 2015MNRAS.449.1605Z (acknowledgments)
We are grateful to the anonymous referee for the valuable comments and advices. In this study, we used the SDSS DR9 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 US 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 website is http://www.sdss.org/ . We acknowledge the use of the HyperLeda data base. This work was supported by Russian Foundation for Basic Research (projects nos. 12-02-00685 and 14-22-03006-ofi-m). IYK is also grateful to Dmitry Zimin's non-profit Dynasty Foundation. 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. The observations at the 6-meter BTA telescope were carried out with the financial support of the Ministry of Education and Science of the Russian Federation (agreement No. 14.619.21.0004, project ID RFMEFI61914X0004).
Paper: 2018MNRAS.477.3279S (acknowledgments)
ACKNOWLEDGEMENTS The authors thank Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Science and Technology Facilities Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência e Tecnologia (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), for the observational data in the projects GS-2009A-Q-5 and GS-2010A-Q-26. This work is based in part on data products produced in big surveys, so we also thank the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii and the Sloan Digital Sky Survey IV funding by the Alfred P. Sloan Foundation, the U.S. Department of Energy Office of Science, and the Participating Institutions. ACS thanks the financial support provided by CAPES. LSJ thanks support from CNPq and FAPESP (00800-4/2012). RMO thanks the financial support provided by CAPES and CNPq (142219/2013-4). ESC acknowledges support from CNPq and FAPESP (2014/13723-3). GLN also thanks support from CNPq.
Paper: 2017ApJ...845...48S (acknowledgments)
The authors acknowledge the staff members of the Qinghai Radio Observing Station at Delingha for their support of the observations. We thank the anonymous referee for valuable comments and suggestions that helped to improve this paper. This work is supported in part by National Key RD Program of China (2017YFA0402700). Y.S. acknowledges support from NSFC grants 11233001 and 11233007. X.Z. acknowledges support from NSFC grant 11403104 and Jiangsu Provincial Natural Science Foundation grant BK20141044. Y.C. acknowledges support from 973 Program grant 2015CB857100 and NSFC grant 11633007. Y.G. acknowledges support from NSFC grant 11127903. Facility: PMO 13.7m . Software: GILDAS/CLASS (Pety 2005 ).
Paper: 2018ApJ...858...20V (acknowledgments)
Work on this project by K.T.V. and A.C.S. was supported by AST-1350389. J.S. acknowledges support from NSF grant AST-1514763 and the Packard Foundation. A.J.R. was supported by National Science Foundation grant AST-1515084 and as a Research Corporation for Science Advancement Cottrell Scholar. I.C.’s research is supported by the Telescope Data Center, Smithsonian Astrophysical Observatory. I.C. also acknowledges support by the Russian Science Foundation grant 17-72-20119 and by the ESO Visiting Scientist programme. Based on observations made with the NASA/ESA Hubble Space Telescope , 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). Facilities: HST , VLT/SINFONI .
Paper: 2015ApJ...803..105P (acknowledgments)
This work was supported by a U.S. Department of Energy Early Career grant. We thank Dan Matthews, David Schlegel, Arjun Dey, and Eduardo Rozo for helpful discussions. Funding for the DEEP2 survey has been provided by NSF grants AST-0071048, AST-0071198, AST-0507428, and AST-0507483. (Some of) the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The DEEP2 team and Keck Observatory acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community and appreciate the opportunity to conduct observations from this mountain. 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 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. CFHT LS is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the Canada–France–Hawaii Telescope (CFHT), which is operated by the National Research Council (NRC) of Canada, the Institut National des Science de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at Terapix available at the Canadian Astronomy Data Centre as part of the Canada–France–Hawaii Telescope Legacy Survey, a collaborative project of NRC and CNRS. We gratefully acknowledge the contributions of the entire COSMOS collaboration, consisting of more than 100 scientists. The HST COSMOS program was supported through NASA grant HST -GO-09822.
Paper: 2019MNRAS.490..135L (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the National Research Foundation of Korea (NRF) grant no. 2017R1A3A3001362, funded by the Korea government (MSIP). MH acknowledges the support from Global PhD Fellowship Program through the National Research Foundation of Korea (NRF) funded by the Ministry of Education (NRF-2013H1A2A1033110). This paper includes data gathered with the 6.5 m Magellan Telescopes located at Las Campanas Observatory, Chile, and the United Kingdom Infrared Telescope (UKIRT) which is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology Center; operations are enabled through the cooperation of the Joint Astronomy Centre of the Science and Technology Facilities Council of the UK.
Paper: 2015MNRAS.451.3581P (acknowledgments)
I am grateful to the referee for helpful comments and suggestions. This work has been supported by the French National Research Agency (ANR) through the grant no. ANR-13-JS05-0003-01 (project EMPERE).
Paper: 2016ApJ...817...56T (acknowledgments)
The authors thank Joshua Moloney for helpful discussions and assistance with emission line identification. Support for program number HST -GO-13302.01 was provided by NASA through a grant from the Space Telescope Science Institute. EMT acknowledges support from NASA Earth and Space Science Fellowship grant NNX14-AO18H. Facilities: HST (COS, STIS) .
Paper: 2018MNRAS.476.4279Y (acknowledgments)
Acknowledgements We would are deeply grateful to our colleagues who have provided us with valuable guidance. Special thanks to Dr Julia Bryant (CAASTRO) and Prof Matthia Jäger (Institut für Photonische Technologien) for productive discussions.
Paper: 2018MNRAS.481.1624M (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for insightful comments and suggestions that improved not only the original manuscript, but the algorithm itself as well. This publication was made possible by NPRP grant ♯ X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation). The statements made herein are solely the responsibility of the author.
Paper: 2019MNRAS.482L..19C (acknowledgments)
ACKNOWLEDGEMENTS TRC acknowledges support from the Associateship Scheme of ICTP, Trieste. PD acknowledges support from the European Research Council’s starting grant DELPHI (717001) and from the European Commission’s and University of Groningen’s CO-FUND Rosalind Franklin program. PD thanks R. Bouwens, N. Gnedin, P. Oesch, and Z. Haiman for illuminating discussions.
Paper: 2020A&A...634A..89D (acknowledgments)
This research has made use of data and/or software provided by 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. This work made use of data supplied by the UK Swift Science Data Centre at the University of Leicester. Authors thank the Russian Science Foundation (grant 19-12-00423), National Natural Science Foundation of China (NSFC U1838201), German Academic Exchange Service (DAAD, project 57405000, VD), and the Academy of Finland travel grants 324550 (ST) and 316932 (AL) for support.
Paper: 2015MNRAS.448.3215Z (acknowledgments)
We acknowledge the use of data from the Fermi Science Support Center (FSSC) at NASA's Goddard Space Flight Center. JNZ thanks Dr Yizhong Fan for help in improving the presentation. This work is supported in part by 973 Programme of China under grant 2013CB837000, the National Natural Science Foundation of China under grants 11273064 and 11443004, the Strategic Priority Research Programme ‘The Emergence of Cosmological Structures’ of the Chinese Academy of Sciences (Grant No. XDB09000000) and by the China Postdoctoral Science Foundation under grant 2014M551680.
Paper: 2019A&A...630A..95O (acknowledgments)
LSO and RW received support from a NWO TOP Grant, module 1, awarded to RW. DP is partially supported by the Mexican Conacyt (CB-2014-01, #240512). This work was supported in part by the National Science Foundation under Grant No. PHY-1430152 (JINA Center for the Evolution of the Elements).
Paper: 2016A&A...586A..39R (acknowledgments)
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. A. Recio-Blanco, P. de Laverny and V. Hill acknowledge the Programme National de Cosmologie et Galaxies (PNCG) of CNRS/INSU, France, for financial support.
Paper: 2020A&A...635A..34K (acknowledgments)
Acknowledgements SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including: Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory(Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); and Caltech, JPL, NHSC, Univ. 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). PACS has been developed by a consortium of institutes led by MPE (Germany) and including UVIE (Austria); KUL, CSL, IMEC (Belgium); CEA, OAMP (France); MPIA (Germany); IFSI, OAP/AOT, OAA/CAISMI, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI (Italy), and CICT/MCT (Spain). V.K. would like to thank Richard Allison, and Richard Parker for their help and discussions on mass segregation with the MST method. This work has received support from the European Research Council under the European Union’s Seventh Framework Programme (ERC Advanced Grant Agreements no. 291294 – ORISTARS – and no. 267934 – MISTIC) and from the French National Research Agency (Grant no. ANR–11–BS56–0010 – STARFICH). D.A. acknowledges support by FCT/MCTES through national funds (PIDDAC) by the grant UID/FIS/04434/2019. N.S. and S.B. acknowledge support by the French ANR and the German DFG through the project GENESIS (ANR–16–CE92–0035–01/DFG1591/2–1). G.J.W. gratefully acknowledges support from The Leverhulme Trust. We also acknowledgesupport from the French national programs of CNRS/INSU on stellar and ISM physics (PNPS and PCMI). This research hasmade use of the SIMBAD database, operated at CDS, Strasbourg (France), and of the NASA/IPAC Extragalactic Database (NED), operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Paper: 2017MNRAS.470..512K (acknowledgments)
Acknowledgments This work is based on observations with INTEGRAL , an ESA project with instruments and the science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland, Spain), and Poland, and with the participation of Russia and the USA. This research has made use of: data obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC) provided by NASAs Goddard Space Flight Center; the SIMBAD database operated at CDS, Strasbourg, France; the NASA/IPAC Extragalactic Database (NED) operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration; the Palermo BAT Catalogue and data base operated at INAFIASF Palermo. The data were obtained from the European 8 and Russian 9 INTEGRAL Science Data Centers. The authors are grateful to E. M. Churazov, who developed the INTEGRAL /IBIS data analysis methods and provided the software, and thank the Max Planck Institute for Astrophysics for computational support. This work was financially supported by Russian Science Foundation grant 14-22-00271.
Paper: 2019MNRAS.489.4520N (acknowledgments)
ACKNOWLEDGEMENTS AVN acknowledges the Russian Science Foundation (RSF) grant 16-12-10225. DB, YS, and FL were supported by the ‘Programme National Physique et Chimie du Milieu Interstellaire’ (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES. YS would like to thank support from the Computing Center of the ‘Institut National de Physique Nucléaire’ (IN2P3). We are grateful to Dr. Wan for providing the collisional rate coefficients for H 2 –H 2 collisions.
Paper: 2018A&A...619A.107S (acknowledgments)
Acknowledgements Comments from an anonymous referee are gratefully acknowledged. The authors thanks Sergio Dzib, Carlos Carrasco-González, Mark Reid, Riccardo Cesaroni, and Roberto Galván-Madrid for fruitful discussion in preparation. A.S. gratefully acknowledges financial support by the Deutsche Forschungsgemeinschaft (DFG) Priority Program 1573.
Paper: 2019MNRAS.487.5666S (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank the reviewer for the careful and thorough reading of this manuscript and for the thoughtful comments and constructive suggestions which help to improve the quality of this manuscript.
Paper: 2017MNRAS.470..350Y (acknowledgments)
Acknowledgments The authors thank Reed Essick, Tanja Hinderer and the referee for valuable comments. This work is supported in part by NASA ATP grant NNX14AB40G. HY is also supported in part by the National Science Foundation and the LIGO Laboratory. LIGO was constructed by the California Institute of Technology and Massachusetts Institute of Technology with funding from the National Science Foundation and operates under cooperative agreement PHY-0757058.
Paper: 2017MNRAS.472.1736R (acknowledgments)
Acknowledgements We thank our referee, Ulrike Heiter, for providing constructive feedback that improved the content and clarity of this manuscript. This work has made use of the VALD data base, operated at Uppsala University, the Institute of Astronomy RAS in Moscow and the University of Vienna. This research made use of Astropy, a community-developed core python package for Astronomy (Astropy Collaboration 2013 ). This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in AAS 143, 23. We acknowledge support from NSF-AST 1009314 (E.R., J.W.) and NASA Origins of Solar System program under NNX13AK17G (J.W.).
Paper: 2019A&A...626A..37K (acknowledgments)
Acknowledgements The IMEX model was developed under ESA funding (contract 4000106316/12/NL/AF - IMEX). H.K. and P.S. are grateful to the MPI für Sonnensystemforschung and the University of Stuttgart for their support. We are grateful to an anonymous referee whose comments substantially improved the presentation of our results.
Paper: 2018A&A...620A.133R (acknowledgments)
We thank the referee for his/her thorough report, in particular for pointing out the misinterpretation of broad-band colours. TR acknowledges support from CONICYT project Basal AFB-170002. He also acknowledges an ESO senior visitorship, during which the data reductions were performed, which was essential for this contribution. T.H.P. gratefully acknowledges support by FONDECYT Regular Project No. 1161817 and by CONICYT project Basal AFB-170002. Dominik Bomans is thanked for discussions on STARLIGHT and literature hints. We use QFitsView (version 3.2, developed by Thomas Ott and Alex Agudo Berbel at the Max Planck Institute for Extraterrestrial Physics, Garching) for extracting and averaging spectra.
Paper: 2016ApJ...826...68H (acknowledgments)
The authors thank Dr. J.J. Tobin for providing the CARMA N 2 H + (1–0) data for Figure 1 . We are grateful to Dr. A. Palau for providing the data points in Figure 13 . We thank Dr. T. Stanke for providing us with the JCMT CO (3–2) data for comparison. The authors acknowledge the staff at APEX, IRAM 30 m, SMA, and JVLA for assistance with operations. 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. T.H.H. and S.P.L. are thankful for the support of the Ministry of Science and Technology (MoST) of Taiwan through grants NSC 98-2112- M-007-007-MY3, NSC 101-2119-M-007-004, MoST 102-2119-M-007-004-MY3, and MoST 104-2119-M-007-021. T.H.H. appreciates the grant from MOST with the PhD exchange student award (MOST 103-2917-I-007-005) and also thanks the MPIfR for supporting him as a visiting astronomer in Bonn, Germany.
Paper: 2019A&A...624A..91K (acknowledgments)
This project was supported by the Polish National Center of Science under decision UMO-2016/20/S/ST9/00142.