adsabs/WIESP2022-NER huggingface dataset:
Paper: 2018MNRAS.473.3454B (acknowledgments)
Acknowledgements We thank Ross Parkin, Cornelia Lang, Naomi McClure-Griffiths, and Helga Denés for insightful discussions on the numerical setups and on the potential applications of the simulations presented here, and the anonymous referee for their comments which helped improve this work. WBB thanks the National Secretariat of Higher Education, Science, Technology, and Innovation of Ecuador (SENESCYT) for funding this project through a doctoral scholarship (CI:1711298438), and the Ecuadorian Network for Research and Education (RED CEDIA) for providing access to local computational resources. WBB is the recipient of the Olin Eggen Scholarship at Mount Stromlo Observatory. CF acknowledges funding provided by the Australian Research Council's Discovery Projects (grants DP130102078 and DP150104329). RMC is the recipient of an Australian Research Council Future Fellowship (FT110100108). This research was supported by the National Computational Infrastructure at Australian National University and the Pawsey Supercomputing Centre, with funding from the Australian Government and the Government of Western Australia, through grants n72 and ek9. CF thanks for high-performance computing resources provided by the Leibniz Rechenzentrum and the Gauss Centre for Supercomputing (grants pr32lo, pr48pi, and Gauss Centre for Supercomputing Large-scale project 10391), and the Partnership for Advanced Computing in Europe (PRACE grant pr89mu). The 3D plots and movies reported in this series of papers were generated using the VisIt visualization software (Childs et al. 2012 ).
Paper: 2017A&A...597A..16P (acknowledgments)
The authors are very grateful to Ulrike Heiter for writing and maintaining SME documentation, to Thomas Nordlander for contributing NLTE tools and testing the model atmosphere grid interpolation, and to Paul Barklem and Remo Collet for contributing the partition functions for atoms, molecules and negative ions as part of our collaboration on the EOS package. We would also like to thank all SME users for continuous and useful feedback on the package.
Paper: 2019ApJ...885...35L (acknowledgments)
We thank the referee for their helpful comments. This work was supported by the BK21 plus program through the National Research Foundation (NRF) funded by the Ministry of Education of Korea, the Basic Science Research Program through the NRF funded by the Ministry of Education (NRF-2016R1A2B4013131, NRF-2016R1A6A3A11932534, NRF-2019R1A2C1002634), the NRF of Korea Grant funded by the Korean Government (NRF-2013M1A3A3A02042232), the Korea Astronomy and Space Science Institute under the RD program supervised by the Ministry of Science, ICT and Future Planning, the Korea Astronomy and Space Science Institute under the RD program Development of a Solar Coronagraph on International Space Station (Project No. 2019-1-850-02) supervised by the Ministry of Science, ICT and Future Planning, and the Institute for Information communications Technology Promotion (IITP) grant funded by the Korea government (MSIP) (2018-0-01422, Study on analysis and prediction technique of solar flares). The data used here are provided courtesy of NASA/ SDO and the HMI science team, as well as the GOES team.
Paper: 2020MNRAS.tmp..303G (acknowledgments)
ACKNOWLEDGEMENTS We are grateful to the California- Kepler Survey team for making their data publicly available. We thank James Owen for valuable comments that helped to improve the manuscript. AG also thanks Erik Petigura and B.J. Fulton for useful discussions related to this work. HES gratefully acknowledges support from the National Aeronautics and Space Administration under grant No. 17 XRP17_2 – 0055 issued through the Exoplanet Research Program.
Paper: 2015MNRAS.450.1716S (acknowledgments)
We thank an anonymous referee for detailed comments that substantially improved both the scientific content and the presentation of our results. We also thank Erez Michaely, Hagai Perets and Robert Izzard for very valuable discussions and suggestions. This research was supported by a generous grant from the president of the Technion Professor Peretz Lavie, and by the Asher Fund for Space Research at the Technion.
Paper: 2018A&A...619A..84B (acknowledgments)
Part of this work was done while HMJB was visiting the IAC, thanks to a visitor grant in the framework of a Severo Ochoa excellence programme (SEV-2015-0548). This research made use of Astropy, a community-developed core Python package for Astronomy ( Astropy Collaboration 2013 , 2018 ), numpy ( Van Der Walt et al. 2011 ), matplotlib ( Hunter 2007 ) and corner ( Foreman-Mackey 2016 ). This research has been supported by the Spanish Ministry of Economy and Competitiveness (MINECO) under the grant AYA2017-83383-P. The authors thankfully acknowledge the technical expertise and assistance provided by the Spanish Supercomputing Network (Red Española de Supercomputación), as well as the computer resources used: the LaPalma Supercomputer, located at the Instituto de Astrofísica de Canarias. B.M. acknowledges support from the National Research Foundation (NRF) of South Africa. This work was partially funded by the Spanish MINECO through project AYA2016-78994-P. RW was supported by European Research Grant SNDUST 694520. 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: 2016MNRAS.462.4336M (acknowledgments)
We thank Alister Graham, Anne Samson, and the anonymous referee for helpful comments on this manuscript. SPD and AJM acknowledge funding support from the Australian Research Council under Discovery Project 130103505. GAMA is a joint European–Australasian project based around a spectroscopic campaign using the Anglo–Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programmes including GALEX MIS, VST KiDS, VISTA VIKING, WISE , Herschel -ATLAS, GMRT and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/ . Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U. S. 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 Web Site is http://www.sdss.org/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. The VIKING survey is based on observations with ESO Telescopes at the La Silla Paranal Observatory under the programme ID 179.A-2004.
Paper: 2017A&A...597A..93D (acknowledgments)
The work was supported by European FP7-PEOPLE-2010-IRSES-269299 project – SOLSPANET. The work was also supported by Shota Rustaveli National Science Foundation grant DI/14/6-310/12. B.M.S. and M.K. acknowledge the support by the Austrian Fonds zur Foerderung der Wissenschaftlichen Forschung within the project P25640-N27 and T.Z. – under project FWF26181-N27. We are grateful to the anonymous referee for the constructive comments on our manuscript that led to significant improvements.
Paper: 2020MNRAS.491.3820P (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank Ainulnabilah B. Nasirudin and the anonymous referee for their clear and constructive comments. We would also like to thank Lucie Bakels for the helpful comments and discussions. RP is supported by a University of Western Australia Scholarship. PJE is supported by the ARC Centre of Excellence ASTRO 3D through project number CE170100013 Part of this research was undertaken on Raijin, the NCI National Facility in Canberra, Australia, which is supported by the Australian commonwealth Government. Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. This research was undertaken with the assistance of resources from the National Computational Infrastructure (NCI Australia), an NCRIS enabled capability supported by the Australian Government.
Paper: 2019MNRAS.488.4207S (acknowledgments)
ACKNOWLEDGEMENTS This work has been supported by grant no. 366/15 of the Israel Science Foundation. The authors thank an anonymous reviewer whose insightful comments helped improve and clarify this manuscript.
Paper: 2016MNRAS.456.2957A (acknowledgments)
CA would like to thank the University of Kent for her 50th Anniversary PhD scholarship and Timothy Kinnear and Victor Ali-Lagoa for fruitful discussions. MCP and MJC thank the STFC, UK for funding this work. MD acknowledges support from the French Agence National de la Recherche (ANR) SHOCKS.
Paper: 2018A&A...612A..11H (acknowledgments)
Acknowledgments The support of the Namibian authorities and of the University of Namibia in facilitating the construction and operation of H.E.S.S. is gratefully acknowledged, as is the support by the German Ministry for Education and Research (BMBF), the Max Planck Society, the German Research Foundation (DFG), the French Ministry for Research, the CNRS-IN2P3 and the Astroparticle Interdisciplinary Programme of the CNRS, the UK Science and Technology Facilities Council (STFC), the IPNP of the Charles University, the Czech Science Foundation, the Polish Ministry of Science and Higher Education, the South African Department of Science and Technology and National Research Foundation, the Australian Research Council and by the University of Namibia. We appreciate the excellent work of the technical support staff in Berlin, Durham, Hamburg, Heidelberg, Palaiseau, Paris, Saclay, and in Namibia in the construction and operation of the equipment.
Paper: 2019MNRAS.485.5590R (acknowledgments)
ACKNOWLEDGEMENTS We thank an anonymous referee for valuable suggestions which helped to improve the paper and acknowledge useful discussions with Chris Fragile, Matthew Liska, and Anderson Caproni. We thank an anonymous referee for valuable suggestions which helped to improve the paper. This study was financed in part by the Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - Brasil (CAPES) - Finance Code 001, Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), and Fundação de Amparo à pesquisa do Estado do RS (FAPERGS). RN acknowledges funding by the Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) through grant 2017/01461-2. Based on observations obtained at the 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). SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS Collaboration including the Brazilian Participation Group, the Carnegie Institution for Science, Carnegie Mellon University, the Chilean Participation Group, the French Participation Group, Harvard-Smithsonian Center for Astrophysics, Instituto de Astrofisica de Canarias, The Johns Hopkins University, Kavli Institute for the Physics and Mathematics of the Universe (IPMU) / University of Tokyo, the Korean Participation Group, Lawrence Berkeley National Laboratory, Leibniz Institut für Astrophysik Potsdam (AIP), Max-Planck-Institut für Astronomie (MPIA Heidelberg), Max-Planck-Institut für Astrophysik (MPA Garching), Max-Planck-Institut für Extraterrestrische Physik (MPE), National Astronomical Observatories of China, New Mexico State University, New York University, University of Notre Dame, Observatório Nacional / MCTI, The Ohio State University, Pennsylvania State University, Shanghai Astronomical Observatory, United Kingdom Participation Group, Universidad Nacional Autónoma de México, University of Arizona, University of Colorado Boulder, University of Oxford, University of Portsmouth, University of Utah, University of Virginia, University of Washington, University of Wisconsin, Vanderbilt University, and Yale University.
Paper: 2019ApJ...878...78C (acknowledgments)
The authors are thankful for the referee’s kind and valuable comments on this manuscript. This work is supported by NSFC grants 11433006, 11790301, 11661161015, and 11573039, and by a Science Technology Facilities Council (STFC) consolidated grant ST/L000741/1. This work was also partly supported by the joint research program of the Institute for Space-Earth Environmental Research at Nagoya University and the International Space Science Institute-Beijing (ISSI-BJ).
Paper: 2017MNRAS.467.3775P (acknowledgments)
Acknowledgments JAP would like to thank the University of Surrey for the computational resources required to perform the simulations used in this paper. We are grateful to Sverre Aarseth and Keigo Nitadori for making nbody6 publicly available; we also thank Mr David Munro of the University of Surrey for hardware and software support.
Paper: 2019ApJ...874...55L (acknowledgments)
This work was supported in part by the Specialized Research Fund for State Key Laboratories, NSFC under grants 41874201, 41531071, 11873018, 11790302, and 11761131007. We thank the STEREO /PLASTIC team and NASA’s CDAWeb for making these data available. The authors also would like to thank Drs. L. Xiang, Y. F. Hao, and H. Y. Sun for their useful suggestions and discussions.
Paper: 2018MNRAS.481.1658S (acknowledgments)
ACKNOWLEDGEMENTS We thank N. Schartel for providing us with the possibility to perform the ToO observation in the Director Discretionary Time, and the XMM–Newton team for the technical support. We also use Director Discretionary Time on NuSTAR , for which we thank Fiona Harrison for approving and the NuSTAR team for the technical support. We acknowledge financial contribution from the agreements ASI-INAF I/037/12/0 and ASI-INAF 2017-14-H.O. This work was partially supported by the Regione Autonoma della Sardegna through POR-FSE Sardegna 2007-2013, L.R. 7/2007, Progetti di Ricerca di Base e Orientata, Project N. CRP-60529. AP acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement 660657-TMSP-H2020-MSCA-IF-2014, as well as the International Space Science Institute (ISSIBern) which funded and hosted the international team ‘The disc magnetosphere interaction around transitional millisecond pulsar’.
Paper: 2019A&A...632A..22C (acknowledgments)
We thank the referee for the useful comments on the manuscript. F.C. acknowledges financial contribution from the agreement ASI-INAF n.2017-14-H.0 and PRIN MIUR 2015 Cosmology and Fundamental Physics: Illuminating the Dark Universe with Euclid.
Paper: 2018A&A...614A.131Y (acknowledgments)
Acknowledgements We would like to acknowledge help of Derek Homeier and France Allard with Phoenix format. We thank Ingo Waldmann and Marco Rocchetto for testing E XO C ROSS . E XO C ROSS uses the Fortran 90 input parsing module input.f90 supplied by Anthony J. Stone, which is gratefully acknowledged. This work was supported by the UK Science and Technology Research Council (STFC) No. ST/M001334/1 and the COST action MOLIM No. CM1405. This work made extensive use of UCL’s Legion and STFC’s DiRAC@Darwin high performance computing facilities.
Paper: 2018ApJ...854...97D (acknowledgments)
We are grateful to the referee, Prof. Takeuchi, for his helpful comments. We thank Bade Uzgil for insightful discussions. Support for R.D. was provided by the DFG priority program 1573 “The physics of the interstellar medium.” F.W., B.P.V., and E.P.F. acknowledge support through ERC grant Cosmic_Dawn. D.R. acknowledges support from the National Science Foundation under grant number AST-1614213 to Cornell University. Facility: ALMA data: 2015.1.01115.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ.
Paper: 2015MNRAS.453.3068B (acknowledgments)
This work is partially supported by programmes number HST/GO 11700, 12587, 12905 and 13767 from NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc, under NASA contract NAS5-26555. JSBW acknowledges the support of an Australian Research Council Laureate Fellowship. MT acknowledges the support of an Australia Research Council Future Fellowship. We would like to acknowledge the anonymous referee for their helpful comments, Sharon Rapoport for her initial lens modelling of the system and Stephanie Bernard for her help with the BoRG data.
Paper: 2017MNRAS.468...97L (acknowledgments)
Acknowledgments This paper has gone through internal review by the DES collaboration. Funding for the DES Projects has been provided by the US Department of Energy, the US National Science Foundation, the Ministry of Science and Education of Spain, the Science and Technology Facilities Council of the United Kingdom, the Higher Education Funding Council for England, the National Center for Supercomputing Applications at the University of Illinois at Urbana-Champaign, the Kavli Institute of Cosmological Physics at the University of Chicago, the Center for Cosmology and Astro-Particle Physics at the Ohio State University, the Mitchell Institute for Fundamental Physics and Astronomy at Texas AM University, Financiadora de Estudos e Projetos, Fundao Carlos Chagas Filho de Amparo Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Cientfico e Tecnolgico and the Ministrio da Cincia, Tecnologia e Inovao, the Deutsche Forschungsgemeinschaft and the Collaborating Institutions in the DES. The DES data management system is supported by the National Science Foundation under Grant Number AST-1138766. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2012-39559, ESP2013-48274, FPA2013-47986 and Centro de Excelencia Severo Ochoa SEV-2012-0234, some of which include ERDF funds from the European Union. The Collaborating Institutions are Argonne National Laboratory, the University of California at Santa Cruz, the University of Cambridge, Centro de Investigaciones Enrgeticas, Medioambientales y Tecnolgicas-Madrid, the University of Chicago, University College London, the DES-Brazil Consortium, the University of Edinburgh, the Eidgenssische Technische Hochschule (ETH) Zrich, Fermi National Accelerator Laboratory, the University of Illinois at Urbana-Champaign, the Institut de Cincies de lEspai (IEEC/CSIC), the Institut de Fsica dAltes Energies, Lawrence Berkeley National Laboratory, the Ludwig-Maximilians Universitt Mnchen and the associated Excellence Cluster Universe, the University of Michigan, the National Optical Astronomy Observatory, the University of Nottingham, the Ohio State University, the University of Pennsylvania, the University of Portsmouth, SLAC National Accelerator Laboratory, Stanford University, the University of Sussex and Texas AM University. The DES data management system is supported by the National Science Foundation under Grant Number AST-1138766. The DES participants from Spanish institutions are partially supported by MINECO under grants AYA2012-39559, ESP2013-48274, FPA2013-47986 and Centro de Excelencia Severo Ochoa SEV-2012-0234. Research leading to these results has received funding from the European Research Council under the European Unions Seventh Framework Programme (FP7/2007-2013) including ERC grant agreements 240672, 291329 and 306478. EB acknowledges financial support from the European Research Council (ERC-StG-335936, CLUSTERS).
Paper: 2016ApJ...826...57B (acknowledgments)
We thank John Beacom, Keith Bechtol, Chris Belczynski, Michal Dominik, Alex Drlica-Wagner, Jennifer Johnson, Vicky Kalogera, Paul Lasky, Adam Martin, Grant Mathews, Annika Peter, Kris Sigurdson, Rebecca Surman, Todd Thompson, and MacKenzie Warren for helpful discussions, and the ABHM Workshop for their hospitality while this work was completed. J.B. thanks the Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1066293. T.L. is supported by the National Aeronautics and Space Administration through Einstein Postdoctoral Fellowship Award No. PF3-140110.
Paper: 2018MNRAS.473.5324Y (acknowledgments)
Acknowledgements This work was supported by the UK Science and Technology Research Council (STFC) No. ST/M001334/1 and the COST action MOLIM No. CM1405. This work made extensive use of UCL’s Legion high performance computing facility.
Paper: 2018A&A...619A.158V (acknowledgments)
We thank our anonymous referee for the useful comments and suggestions. This work has been supported by PRA Università di Pisa 2018-2019 ( Le stelle come laboratori cosmici di Fisica fondamentale , PI: S. Degl’Innocenti) and by INFN ( Iniziativa specifica TAsP ).