adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017ApJ...850...77K (acknowledgments)
H.B. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Consolidator Grant CSF-648505. J.M.D.K. gratefully acknowledges funding from the German Research Foundation (DFG) in the form of an Emmy Noether Research Group (grant number KR4801/1-1, PI Kruijssen), from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme via the ERC Starting Grant MUSTANG (grant agreement number 714907, PI Kruijssen), and from Sonderforschungsbereich SFB 881 “The Milky Way System” (subproject P1) of the DFG. E.R. is supported by a Discovery Grant from NSERC of Canada. T.P. acknowledges support from the Deutsche Forschungsgemeinschaft, DFG via the SPP (priority program) 1573 Physics of the ISM. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Software: CASA (McMullin et al. 2007 ), CLASS ( http://www.iram.fr/IRAMFR/GILDAS ), miriad (Sault et al. 1995 ), APLpy (Robitaille Bressert 2012 ). Facility: ATCA(CABB) .
Paper: 2018MNRAS.480.2743F (acknowledgments)
ACKNOWLEDGEMENTS This scientific work makes use of the Murchison Radio-astronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. Support for the operation of the Murchison Widefield Array is provided by the Australian Government (NCRIS), under a contract to Curtin University administered by Astronomy Australia Limited. We acknowledge the Pawsey Supercomputing Centre which is supported by the Western Australian and Australian Governments and the Centre of Excellence for All-sky Astrophysics (CAASTRO), which is an Australian Research Council Centre of Excellence, funded by grant CE110001020. Parts of this research were conducted with the support of Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. This research also made use of Montage. Montage is funded by the National Science Foundation under Grant Number ACI-1440620, and was previously funded by the National Aeronautics and Space Administration’s Earth Science Technology Office, Computation Technologies Project, under Cooperative Agreement Number NCC5-626 between NASA and the California Institute of Technology.
Paper: 2019ApJ...870...89P (acknowledgments)
This material is based upon work partially supported by the National Science Foundation under grant No. 1616538. The National Solar Observatory is operated by the Association of Universities for Research in Astronomy under a cooperative agreement with the National Science Foundation. The National Center for Atmospheric Research is sponsored by the National Science Foundation. This work utilized the RMACC Summit supercomputer, which is supported by the National Science Foundation (awards ACI-1532235 and ACI-1532236), the University of Colorado Boulder, and Colorado State University. The Summit supercomputer is a joint effort of the University of Colorado Boulder and Colorado State University. The authors are grateful for the International Space Science Institute in Bern for hosting the International Team 335 “Toward New Models of Solar Spectral Irradiance Based on 3D MHD Simulations,” which helped motivate this work. Software: MURaM (Vögler et al. 2005 ; Rempel et al. 2009 ), RH (Uitenbroek 2001 ; Pereira Uitenbroek 2015 ), Stagger (Nordlund Galsgaard 1995 ), Scipy ndimage (Jones et al. 2001 ).
Paper: 2019MNRAS.485.2010G (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank John Pritchard of ESO Operations Support for his assistance with the wavelength calibration of the spectra. Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 095.B-0133(A). This paper includes data gathered with the 6.5m Magellan Telescopes located at Las Campanas Observatory, Chile. This work makes use of PyAstronomy and emcee . DRW is supported by a fellowship from the Alfred P. Sloan Foundation. NFM acknowledges that this work has been published under the framework of the IdEx Unistra and benefits from a funding from the state managed by the French National Research Agency as part of the investments for the future programme. NFM also acknowledge support by the Programme National Cosmology et Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES.
Paper: 2019MNRAS.484..648P (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank Laurent Pueyo for his encouragement, and Suzanne Aigrain, Vinesh Maguire-Rajpaul, Jane Kaczmarek, Rocio Kiman, Daniella Bardalez Gagliuffi, David Hogg, Jim Davenport, and Brett Morris for their valuable comments. We are especially grateful for the thorough and insightful comments of the anonymous reviewer. This work was performed in part under contract with the Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute. This project was developed in part at the 2018 NYC Gaia Sprint, hosted by the Center for Computational Astrophysics of the Flatiron Institute in New York City. We have 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. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France; NASA’s Astrophysics Data System; and the ALMA Sensitivity Calculator in the ALMA Observing Tool by Mark Nicol. The Observing Tool is the software tool that will be used for the preparation of ALMA Observing Projects. The Tool is built by the Proposal and Observing Preparation System team within the ALMA Computing IPT. This research has made use of the following softwares: ipython (Pérez Granger 2007 ), scipy (Jones et al. 2001 ), matplotlib (Hunter 2007 ), astropy (Astropy Collaboration 2013 ), and numpy (Van Der Walt, Colbert Varoquaux 2011 ).
Paper: 2020MNRAS.492.1937P (acknowledgments)
ACKNOWLEDGEMENTS ENM acknowledges support by an SIIP-UNCuyo grant.
Paper: 2017MNRAS.472.2367C (acknowledgments)
Acknowledgements We acknowledge the substantial efforts of both the CFHT staff in implementing the Legacy Survey and of the CFHTLenS team in preparing catalogues of galaxy ellipticities and photometric redshifts. This work is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/IRFU, at the CanadaFranceHawaii Telescope (CFHT) that is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de lUnivers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency. CFHTLenS data processing was made possible thanks to significant computing support from the NSERC Research Tools and Instruments grant programme. MJH and MLB acknowledge support from NSERC.
Paper: 2020MNRAS.tmp..165D (acknowledgments)
ACKNOWLEDGEMENTS This work was partially supported by National Aeronautics and Space Administration (grant NNX13AN25G) and the National Science Foundation (grant 1616992).
Paper: 2019ApJ...883..143L (acknowledgments)
We thank the reviewer for the very comprehensive and insightful report that helped improve the quality of the paper. We also thank Freeman Dyson and Corey Powell for valuable comments regarding the paper. This work was supported in part by the Breakthrough Prize Foundation, Harvard University’s Faculty of Arts and Sciences, and the Institute for Theory and Computation (ITC) at Harvard University.
Paper: 2019MNRAS.484L..38M (acknowledgments)
ACKNOWLEDGEMENTS We are thankful to the anonymous referee for his/her valuable comments. This article is based on observations made in the Observatorios de Canarias del IAC with the William Herschel Telescope (WHT) operated on the island of La Palma by the Isaac Newton Group in the Observatorio del Roque de los Muchachos. This work is partly financed by the Spanish Ministry of Economics and Competitiveness through grants ESP2013-48391-C4-2-R and AYA2016-79425-C3-2-P.
Paper: 2015MNRAS.450.4184Z (acknowledgments)
Support for this work was provided by the NASA through Chandra award number AR4-15013X issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the NASA under contract NAS8-03060. SWA acknowledges support from the US Department of Energy under contract number DE-AC02-76SF00515. IZ and NW are partially supported from Suzaku grants NNX12AE05G and NNX13AI49G. PA acknowledges financial support from FONDECYT grant 1140304. EC and RS are partly supported by grant No. 14-22-00271 from the Russian Scientific Foundation.
Paper: 2018ApJ...857...38H (acknowledgments)
We thank the reviewer for providing helpful comments that improved this paper. A.M.H. is supported by the DOE NNSA Stewardship Science Fellowship. P.M.R. acknowledges support from the National Science Foundation under grant AST 14-13367. Portions of this work were completed at the Kavli Institute for Theoretical Physics, where it was supported in part by the National Science Foundation under grant NSF PHY-1125915. We thank Vicky Kalogera, Frank Timmes, Krzysztof Belczynski, Grzegorz Wicktorowicz, Pablo Marchant, Imre Bartos, Daniel Siegel, Konstantin Postnov, Aleksandr Tutukov, Brian Fields, and Lars Bildsten for helpful comments and fruitful discussions. We also thank Samaya Nissanke for reviewing this work as an LVC reviewer. The LIGO document number for this work is P1700155. Software: MESA (V8845; Paxton et al. 2011 , 2013 , 2015 ), Matplotlib (Hunter 2007 ), Numpy (Walt et al. 2011 ).
Paper: 2017A&A...597A..24R (acknowledgments)
We thank the anonymous referee for constructive criticism that helped to improve the readability of the paper. We thank A. Biviano, H. Böhringer, and J. Dietrich for their numerous suggestions that helped this work. Furthermore, we thank A. L. Serra and A. Diaferio for the communication on the caustic method and kindness to cross-check our results with their code, as well as Heinz Andernach for his hint on a case with a lack of clearity. The Guide Star Catalogue-II is a joint project of the Space Telescope Science Institute and the Osservatorio Astronomico di Torino. Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, for the National Aeronautics and Space Administration under contract NAS5-26555. The participation of the Osservatorio Astronomico di Torino is supported by the Italian Council for Research in Astronomy. Additional support is provided by European Southern Observatory, Space Telescope European Coordinating Facility, the International GEMINI project and the European Space Agency Astrophysics Division. We have made use of VLT/VIMOS observations taken with the ESO Telescope at the Paranal Observatory under programme 087.A-0096 and WFI observations partially supported by the Deutsche Forschungsgemeinschaft (DFG) through Transregional Collaborative Research Centre TRR 33. The XMM-Newton project is an ESA Science Mission with instruments and contributions directly funded by ESA Member States and the USA (NASA). The XMM-Newton project is supported by the Bundesministerium für Wirtschaft und Technologie/Deutsches Zentrum für Luft- und Raumfahrt (BMWI/DLR, FKZ 50 OX 0001) and the Max-Planck Society. 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. We used the version 13SEPpl1.4 of ESO-MIDAS for data reduction and STILTS 1 for table processing and plotting of figures. Y.Y.Z. acknowledges support by the German BMWi through the Verbundforschung under grant 50 OR 1506. T.H.R. acknowledges support from the DFG through the Heisenberg research grant RE 1462/5.
Paper: 2017MNRAS.464.3486Z (acknowledgments)
This work was supported by NSF grants AST-1105835 and AST-1440343. AL acknowledges support from the University of California Office of the President Multicampus Research Programs and Initiatives through award MR-15-328388, and from NASA through Hubble Fellowship grant HST-HF2-51363.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. The NASA funding for the eGSM is NASA grant no. NNX16AF55G. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center. 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. We wish to thank Jacqueline Hewitt, Gianni Bernardi, Douglas Finkbeiner, Aaron M. Meisner for helpful comments and suggestions, and Angelica de Oliveira-Costa for pioneering the GSM approach. We also wish to thank our anonymous referee for extremely helpful and detailed feedback.
Paper: 2020MNRAS.491.1506D (acknowledgments)
ACKNOWLEDGEMENTS The authors thank the anonymous referee and also Jeff J. Andrews, Deepto Chakrabarty, Pat Slane, Bradford Snios, and Johan Samsing for useful comments and discussions. Financial support was provided from NASA through Einstein Postdoctoral Fellowship award number PF6-170151 (DJD) and also through the Smithsonian Institution.
Paper: 2015ApJ...802...36Y (acknowledgments)
This research was supported by the National Natural Science Foundation of China under grant Nos. 11321064, 11233004, 11390371, 11473033, U1331122, and by National Key Basic Research Program of China 2014CB845700.
Paper: 2017A&A...608A.110M (acknowledgments)
The authors would like to thank G. Aarts and M. Hanauske for helpful discussions and M. Strickland for carefully reading the manuscript. The authors also acknowledge the support from NewCompStar COST Action MP1304, from GSI, HIC for FAIR, and from BMBF. The computational resources were provided by the Frankfurt Centre for Scientific Computing (CSC) and Center for Nuclear Research (Kent State University). In addition, the authors acknowledge the insights and comments of the referee who took the time to review this paper.
Paper: 2015MNRAS.452.1743T (acknowledgments)
This work was initiated during the International Summer Institute for Modelling in Astrophysics (ISIMA) in 2014, hosted at CITA at the University of Toronto. This work was in part supported by NASA grant NNX13AI27G. We also thank Kristen Menou, Linda Strubbe, Pascale Garaud, Jeremy Leconte, Yanqin Wu, Subu Mohanty, Man-Hoi Lee, Eric Lopez, John Papaloizou, Dan Fabrycky and Arieh Konigl for helpful discussions and correspondence. We also thank the anonymous referee for helpful suggestions. JT is supported by STFC through grant ST/L000636/1. JEO acknowledges support by NASA through Hubble Fellowship grant HST-HF2-51346.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555.
Paper: 2019MNRAS.482.4673J (acknowledgments)
ACKNOWLEDGEMENTS We thank the reviewer for helpful suggestions that improved the manuscript. MRJ is funded by the President’s PhD scholarship of the Imperial College London and the ‘Dositeja’ stipend from the Fund for Young Talents of the Serbian Ministry for Youth and Sport. TJH is funded by an Imperial College Junior Research Fellowship. JDI gratefully acknowledges support from the DISCSIM project, grant agreement 341137, funded by the European Research Council under ERC-2013-ADG and support from the STFC (grant number ST/R000549/1). DF gratefully acknowledges support from the ECOGAL project, grant agreement 291227, funded by the European Research Council under ERC-2011-ADG. CJC acknowledges support from the STFC (grant number ST/M001296/1). CW acknowledges financial support from the University of Leeds. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2019A&A...632A..42B (acknowledgments)
We thank TASC WG8.2 for supporting this project and providing valuable feedback, especially D. Kilkenny and R. Raddi. We thank the anonymous referee whose comments helped to improve this manuscript. KJB is supported by an NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-1903828. MHM acknowledges support from NSF grant AST-1707419 and the Wootton Center for Astrophysical Plasma Properties under the United States Department of Energy collaborative agreement DE-FOA-0001634. ASB gratefully acknowledges financial support from the Polish National Science Center under project No. UMO-2017/26/E/ST9/00703. ZsB acknowledges the financial support of the K-115709 and PD-123910 grants of the Hungarian National Research, Development and Innovation Office (NKFIH), and the Lendület Program of the Hungarian Academy of Sciences, project No. LP2018-7/2018. Support for this work was provided by NASA through the TESS Guest Investigator program through grant 80NSSC19K0378. This paper includes data collected with the TESS mission, obtained from the MAST data archive at the Space Telescope Science Institute (STScI). Funding for the TESS mission is provided by the NASA Explorer Program. STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5–26555. 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.
Paper: 2015ApJ...812...93G (acknowledgments)
S.G. acknowledges support from the European Commission via the Marie Curie Actions—Intra-European Fellowships Project No. 328138. D.H.M. acknowledges financial support from the STFC, the Leverhulme Trust, and NASA. The simulations in the present paper use the STFC funded UKMHD supercomputer in St Andrews.
Paper: 2015A&A...584A..52L (acknowledgments)
This research was partially supported by the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence “Origin and Structure of the Universe”. S.L., A.S., E.C., A.B. acknowledge partial support from PRIN-MIUR 2010-2011 PI Francesca Matteucci Evoluzione chimica e dinamica della nostra galassia e delle galassie del gruppo locale. E.V. acknowledges support by grants NASA-NNX13AF45G and HST-12830.01-A.
Paper: 2016MNRAS.460.3873B (acknowledgments)
MCPB acknowledges support from Maja Vučković and the Joint Committee ESO-Government of Chile (grant 2014). TRM, EB, VSD, SPL, TB and RWW are grateful to the Science and Technology Facilities Council for financial support in the form of grant nos ST/L000733, ST/L00075X/1 and ST/M001350/1. SGP and CC acknowledge support from CONICYT FONDECYT grants 3140585 and 3140592, respectively. CC also acknowledges support from the Millennium Nucleus RC130007 (Chilean Ministry of Economy). JJH acknowledges support from NASA through Hubble Fellowship grant no. HST-HF2-51357.001-A, awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. DK is partially funded by the University of the Western Cape and the National Research Foundation (NRF) of South Africa. The research leading to these results has also received funding from the European Research Council under ERC Grant Agreement n. 320964 (WDTracer).
Paper: 2018A&A...610A...5C (acknowledgments)
We acknowledge Bruce Elmegreen for useful discussions. We thank the referee for helping us to polish the results section. S.C. and H.S. acknowledge support from the Academy of Finland. J.H.K. acknowledges financial support from the European Union’s Horizon 2020 research and innovation programme under Marie Skłodowska-Curie grant agreement No. 721463 to the SUNDIAL ITN network, and from the Spanish Ministry of Economy and Competitiveness (MINECO) under grant number AYA2016-76219-P. We acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ). 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.
Paper: 2017MNRAS.464.3871S (acknowledgments)
We warmly thank the anonymous referee for his/her helpful comments and suggestions. AS acknowledges the PRIN INAF 2011 ‘Multiple populations in globular clusters: their role in the Galaxy assembly’ (PI E. Carretta) and the PRIN INAF 2014 ‘Probing the internal dynamics of globular clusters. The first one is comprehensive radial mapping of individual star kinematics with the generation of multi-object spectrographs’ (PI: L. Origlia). ED and CP acknowledge support from the European Research Council (ERC-2010-AdG-267675, COSMIC-LAB). Based on FOcal Reducer and low dispersion Spectrograph (FORS) observations collected with the Very Large Telescope of the European Southern Observatory, Cerro Paranal, Chile, within the observing programmes 091.D-0562(A) and 093.D-0228(A) (PI: Dalessandro), and on observations made with the Large Binocular Camera at the Large Binocular Telescope within program INAF.D07-2010A (PI: Ferraro) and with the Advanced Camera for Surveys (ACS) on board to the NASA/ESA Hubble Space Telescope under programs GO-10775 (PI: Sarajedini).
Paper: 2018ApJ...865...21Y (acknowledgments)
We thank the referee for his/her very helpful comments. We appreciate Jian Li, Feifei Kou, Xian Hou, and Shanshan Weng for their useful suggestions and discussions. We thank the High Energy Astrophysics Science Archive Research Center and Fermi Science Support Center for maintaining its online archive service that provided the data used in this research. This work is supported by the National Key RD Program of China (2016YFA0400803, 2016YFA0400800), National Science Foundation of China (11233001, 11503027 and 61471003), the Strategic Pionner Program on Space Science, Chinese Academy of Sciences, grant No. XDA15051400, and Anhui Province Key Laboratory of Intelligent Building Building Energy Saving.
Paper: 2015A&A...581A...8R (acknowledgments)
We gratefully acknowledge support from the Royal Commission for the Exhibition of 1851 through their Research Fellowship scheme (A.J.B.R.), the European Commission through HESPE (FP7-SPACE-2010-263086) (P.J.A.S., L.F.) and the Science and Technology Facilities Council through grants ST/I001808 (P.J.A.S., L.F.) and ST/L000741/1 (L.F.) to the University of Glasgow, as well as ST/K000993/1 (A.J.B.R.) to the University of Dundee. AIA data were supplied courtesy of SDO (NASA) and the AIA science team.