adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017MNRAS.471.2013A (acknowledgments)
Acknowledgments I wish to thank Eduardo Balbinot, Nora Shipp, Alex Drlica-Wagner for the comparison between my MW stream candidates and theirs; and Elizabeth Buckley-Geer, Huan Lin, Paul Schechter and Tommaso Treu for discussions on quasar lens searches. Careful comments by the anonymous referee have led to clarifications and improvements of this paper. I gratefully acknowledge hospitality by the ITC-Harvard, where this work was completed. 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 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: 2019A&A...631A..40S (acknowledgments)
We thank M. Auger for useful discussions. SS, GC, SHS, and AY thank the Max Planck Society for support through the Max Planck Research Group for SHS. This research was supported in part by Perimeter Institute for Theoretical Physics. Research at Perimeter Institute is supported by the Government of Canada through the Department of Innovation, Science and Economic Development and by the Province of Ontario through the Ministry of Research, Innovation and Science. The analysis is based on the following: (1) observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations were done in May 2010 with Proposal ID 11602 and in November 2011 with Proposal ID 12266; (2) 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 National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina), and Ministério da Ciência, Tecnologia e Inovação (Brazil).
Paper: 2015ApJ...798...47G (acknowledgments)
We are indebted to Brian Marsden, who performed the orbit calculations that made these observations possible. S.G. and J.C.R. thank the International Space Science Institute (Bern, Switzerland) for the opportunity to discuss this work within the International Study Team program. SOHO is a project of international cooperation between ESA and NASA. UVCS is a joint project of NASA, Italian Space Agency (ASI), and the Swiss Funding Agencies. LASCO was built by a consortium of the Naval Research Laboratory, USA; the Laboratoire d'Astrophysique de Marseille (formerly Laboratoire d'Astronomie Spatiale), France; the Max-Planck-Institut für Sonnensystemforschung (formerly Max Planck Institute für Aeronomie), Germany; and the School of Physics and Astronomy, University of Birmingham, UK. This work was supported by NASA grant NAG5-12814. Facility: SOHO (UVCS, LASCO)
Paper: 2017A&A...607A..76W (acknowledgments)
T.W. thanks Durham University Department of Mathematical Sciences for funding his Ph.D. studentship. A.R.Y. thanks STFC for financial support. A.R.Y. and G.J.D.P. thank ISSI, Bern for supporting their collaboration as part of an International Team on global magnetic modelling. A.M.J. is very grateful to George Fisher and Stuart Bale for their support at the University of California, Berkeley, and Phil Scherrer for his support at Stanford University. This research is partly funded by the NASA Grand Challenge grant NNH13ZDA001N and NASA LWS grant NNX16AB77G. Data were acquired by SOLIS instruments operated by NISP/NSO/AURA/NSF. We are grateful to David Hathaway for also supplying data for this study and to Ian Vernon for his invaluable statistical advice as well as to the anonymous referee for useful suggestions.
Paper: 2016MNRAS.455..659W (acknowledgments)
We acknowledge useful conversations with Dan Coe on this topic, who has been attempting similar measurements on his triply imaged z ∼ 11 candidate. SMW acknowledges support from the Science and Technology Facilities Council. IL acknowledges support from the European Research Council grant HIGHZ no. 227749 and the Netherlands Organization for Scientific Research Spinoza grant. The Dark Cosmology Centre is funded by the Danish National Research Foundation.
Paper: 2016A&A...593A..73A (acknowledgments)
We would like to thank J.C. Augereau for providing the GraTeR code used to create our disk models. R. Asensio-Torres and M. Janson gratefully acknowledge funding from the Knut and Alice Wallenberg foundation. J. Carson acknowledges support via the US National Science Foundation under Award No. 1009203.
Paper: 2015A&A...575A..72B (acknowledgments)
S.B. thanks the Wihuri Foundation for continued funding throughout the project, the Finnish Cultural Foundation for funding the last part of the research, and the University of Turku Foundation and the StarryStory Foundation for funding travel related to the project. We are grateful for the help provided by Marina Rejkuba during the telescope application period and analysis of the 40 kpc NGC 5128 halo field, to Glen Mackie for very useful discussions, and for the care and interest taken by the referee during the reviewal process. This work has made use of BaSTI web tools.
Paper: 2018MNRAS.474.2012B (acknowledgments)
Acknowledgements Most of this work was made possible by support from the US National Science Foundation grant 09-68296 as well as National Aeronautics and Space Administration (NASA) Space Grants. One of us (JR) also thanks the Anton Pannekoek Astronomical Institute of the University of Amsterdam for their support. The Arecibo Observatory is operated by SRI International under a cooperative agreement with the US National Science Foundation, and in alliance with SRI, the Ana G. Méndez-Universidad Metropolitana and the Universities Space Research Association. This work made use of the NASA ADS astronomical data system. One of us (KS) thanks the US National Science Foundation for their support under the Physics Frontiers Center award number 1430284.
Paper: 2018ApJ...860...27I (acknowledgments)
A.I. and N.J.T. thank Mario Flock, Cornelis Dullemond, Thomas Henning, Wilhelm Kley, Wladimir Lyra, and Roy van Boekel for helpful discussions, and Ruobing Dong, Nienke Van der Marel, and Myriam Benisty for sharing images of SAO206463 and J1604. A.I. and N.J.T. acknowledge support from the NASA Origins of Solar Systems program through award NNX15AB06G and from the JPL Research Technology Development Program through award R.16.183.037. A.I. acknowledges support from the NSF Grants Nos. AST-1535809 and AST-1715718. This work was carried out in part at the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA.
Paper: 2017MNRAS.469.4683C (acknowledgments)
Acknowledgments We thank the anonymous referee for their constructive comments. AC (ORCID 0000-0003-4578-514X) acknowledges support from the UK Science and Technology Facilities Council (STFC) consolidated grant ST/L000652/1. MTS acknowledges support from a Royal Society Leverhulme Trust Senior Research Fellowship (LT150041). We acknowledge financial support from the Swiss National Science Foundation (AC, project PBEZP2_137312), from the Agence Nationale de la Recherche (AC and ElF, contract no. ANR- 12-JS05-0008-01) and from the E. C. through an ERC grant (AC and FB, StG-257720). GEM acknowledges support from the ERC Consolidator Grant funding scheme (project ConTExt, grant no. 648179) and a research grant (13160) from Villum Fonden. WR is supported by a CUniverse Grant (CUAASC) from Chulalongkorn University and JSPS KAKENHI grant no. JP15K17604. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.01271.S. ALMA is a partnership of European Southern Obseratory (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. The research leading to these results has received funding from the European Commission Seventh Framework Programme (FP/2007-2013) under grant agreement no. 283393 (RadioNet3).
Paper: 2017MNRAS.467.1819C (acknowledgments)
We thank the anonymous referee for the very useful comments that improved the content and clarity of the manuscript. This work was partially supported by the Consejo Nacional de Investigaciones Cientficas y Tcnicas (CONICET, Argentina) and the Secretara de Ciencia y Tecnologa de la Universidad Nacional de Crdoba (SeCyT-UNC, Argentina). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation and the US Department of Energy Office of Science. The SDSS-III website is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington and Yale University. This research has made use of NASAs Astrophysics Data System and Cornell University arXiv repository. We made an extensive use of the following python libraries: http://www.numpy.org/ , http://www.scipy.org/ , http://roban.github.com/CosmoloPy/ and http://www.matplotlib.org/ .
Paper: 2018MNRAS.476.2092L (acknowledgments)
Acknowledgements JLS and EJL acknowledge the support of the STFC. We thank members of the Institute of Astronomy Streams group for discussions and comments as this work was in progress. The anonymous referee is thanked for a number of helpful suggestions.
Paper: 2018MNRAS.473.4986O (acknowledgments)
ACKNOWLEDGEMENTS AO acknowledges support from the Deutsche Forschungsgemeinschaft (DFG) through the excellence cluster ‘The Hamburg Center for Ultrafast Imaging - Structure, Dynamics and Control of Matter at the Atomic Scale’ (CUI, EXC1074). SY acknowledges support from the COST action MOLIM No. CM1405. VS acknowledges the research project RVO:61388963 (IOCB) and support from the Czech Science Foundation (grant P209/15-10267S).
Paper: 2019A&A...624A..79B (acknowledgments)
We thank the enitre T’DA team for useful comments and discussions, in particular Andrew Tkachenko. We also acknowledge Marc Hon, Keaton Bell, and James Kuszlewicz for useful comments on the manuscript. L.B. and R.A.G. acknowledge the support from PLATO and GOLF CNES grants. S.M. acknowledges support by the Ramon y Cajal fellowship number RYC-2015-17697. O.J.H. and B.M.R. acknowledge the support of the UK Science and Technology Facilities Council (STFC). M.N.L. acknowledges the support of the ESA PRODEX programme (PEA 4000119301). Funding for the Stellar Astrophysics Centre is provided by the Danish National Research Foundation (Grant DNRF106).
Paper: 2020MNRAS.491.4382S (acknowledgments)
ACKNOWLEDGEMENTS This work is a part of the Project 176002 ‘Influence of collisional processes on astrophysical plasma line shapes’ supported by the Ministry of Education, Science and Technological Development of Serbia.
Paper: 2020A&A...633A.124P (acknowledgments)
Acknowledgements The authors thank the ESO staff for conducting the observations. We are grateful to D. Lachapelle for providing the spectra of HIP 78530 B and USco 1610-1913 B. We also thank J. Bouvier for advising us on accretion process and chromospheric activity effects. We acknowledge financial support from the Programme National de Planétologie (PNP), the Programme National de Physique Stellaire (PNPS) of CNRS-INSU in France, and the Agence Nationale de la Recherche (GIPSE project; grant ANR-14-CE33-0018). This research has made use of the SIMBAD database and VizieR catalogue access tool (operated at CDS, Strasbourg, France). This research has made use of NASA’s Astrophysics Data System and of the Extrasolar Planet Encyclopedia ( http:// exoplanet.eu/ ). This publication makes use of VOSA, developed under the Spanish Virtual Observatory project supported from the Spanish MINECO through grant AyA2017-84089. G-DM acknowledges the support of the DFG priority program SPP 1992 “Exploring the Diversity of Extrasolar Planets” (KU 2849/7-1).
Paper: 2019A&A...625A.143V (acknowledgments)
We would like to thank Thorsten Lisker for the valuable help and discussions during the whole FDS project. A.V. would like to thank the Vilho, Yrjö, and Kalle Väisälä Foundation of the Finnish Academy of Science and Letters for the financial support during the writing of this paper. GvdV acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program under grant agreement No 724857 (Consolidator Grant ArcheoDyn). R.F.P., T.L., E.L., H.S., E.I., and J.J. acknowledge financial support from the European Union’s Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No. 721463 to the SUNDIAL ITN network. H.S., E.L., and A.V. are also supported by the Academy of Finland grant n:o 297738. C.W. is supported by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) through project 394551440. J.F-B acknowledges support from grant AYA2016-77237-C3-1-P from the Spanish Ministry of Economy and Competitiveness (MINECO).
Paper: 2015ApJ...802..118B (acknowledgments)
Studies of the evolution of hot gas in elliptical galaxies at UC Santa Cruz were supported during the earlier phases of this work by the NSF and are currently supported by a NASA-funded Chandra Theory Grant for which we are very grateful. F.B. is supported in part by the Prin MIUR grant 2010LY5N2T “The Chemical and Dynamical Evolution of the Milky Way and Local Group Galaxies.”
Paper: 2017ApJ...834...63R (acknowledgments)
The Arecibo Observatory is operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968) and in alliance with Ana G. Méndez-Universidad Metropolitana and the Universities Space Research Association. Facilities : Planck , Arecibo, IRAS.
Paper: 2015MNRAS.453.3015W (acknowledgments)
We thank Hanno Rein, Daniel Tamayo, and Edmund Bertschinger for helpful discussions. DMH acknowledges support by an NSF Graduate Research Fellowship under grant no. 1122374.
Paper: 2016MNRAS.461..321S (acknowledgments)
The authors wish to thank the referee, Dan Taranu, for his thorough revision of the manuscript and insightful comments and suggestions, which have helped to improve both the justification of the initial conditions of our simulations and the presentation of the results. This work was supported by the Programme for Promotion of High-Level Scientific and Technical Research of Spain under contracts AYA2010-15169 and AYA2013-40609-P. The simulations of the present work have been performed with the Computer Service Infrastructure of the Spanish Instituto de Astrofísica de Andalucía (IAA). This research is part of the IDILICO (Investigation of the DIffuse LIght COmponent in CGs of galaxies) project, an international collaboration that runs simulations of the formation of groups of galaxies using high-performance computing resources (see our website at http://www.am.ub.edu/extragalactic/idilico/ ). Initially born to shed light on the origin of the unusually large fractions of diffuse IGL found in some CGs of galaxies, IDILICO has now among its goals the creation of a comprehensive and unbiased sample of forming galaxy associations suited for investigating the aspects of galaxy evolution governed by gravitational dynamics, especially those driven by the multiple interactions and mergers that galaxies undergo in dense environments. Subsets of our numerical experiments are available upon request.
Paper: 2018MNRAS.477L.128S (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee Duncan Lorimer for constructive suggestions that improved this Letter and Prof. D. Li for helpful conversation. This work was supported by the Natural Science Foundation of China (Nos. 11603010, 11133001, 11333004, 11773015, and 11563003), the National Program on Key Research and Development Project (Grant No. 2016YFA0400803), and the Natural Science Foundation for the Youth of Jiangsu Province (No. BK20160611).
Paper: 2018MNRAS.480.4817P (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank the anonymous referee for his/her detailed reading of our work and the many suggestions which improved this manuscript considerably. The authors gratefully acknowledge the Gauss Centre for Supercomputing e.V. ( www.gauss-centre.eu ) for funding this project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre ( http://www.lrz.de ) through project pr49zo, and the Leibniz Gemeinschaft for funding this project through grant SAW-2012-AIP-5 129.
Paper: 2017ApJ...845...89V (acknowledgments)
The authors thank Russell Keeney for his tireless efforts in maintaining and operating the OVRO 40 m Telescope. We thank Sterl Phinney and Shrinivas Kulkarni for useful discussions. The OVRO 40 m program has been supported by NASA grants NNG06GG1G, NNX08AW31G, NNX11A043G, and NNX13AQ89G and NSF grants AST-0808050, and AST-1109911. 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. H. Vedantham is an RA and GB Millikan fellow of experimental physics. T. Hovatta was supported in part by the Academy of Finland project number 267324. R. Reeves gratefully acknowledges support from the Chilean Basal Centro de Excelencia en Astrofisica y Tecnologias Afines (CATA) grant PFB-06/2007. Facilities: OVRO:40 m, Keck:I (LRIS), Metsähovi Radio Observatory, SMA.
Paper: 2017MNRAS.466..838G (acknowledgments)
Acknowledgments We would like to thank Aseem Paranjape, Sowgat Muzahid and Charles Danforth for useful discussion on statistics and observations. All the computations were performed using the PERSEUS cluster at IUCAA and the HPC cluster at NCRA.
Paper: 2020ApJ...891...50U (acknowledgments)
We wish to thank the anonymous referee for a careful reading and useful comments on our manuscript. The Kagoshima University 1 m telescope is a member of the Optical and Near-infrared Astronomy Inter-University Cooperation Program and supported by it. This publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. 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. R.B. acknowledges support through the EACOA Fellowship from the East Asian Core Observatories Association.
Paper: 2015MNRAS.449.1495Y (acknowledgments)
We would like to thank M. Serylak and the anonymous referee for useful comments which have improved this manuscript. NJY also acknowledges financial support from the South African SKA (SKA SA) project.
Paper: 2015ApJ...802...41L (acknowledgments)
This work is supported by NASA Origins of the Solar System grant No. NNX13AH79G. The authors thank A.A. Vidotto (Geneva) L. Fletcher (Glasgow) for providing helpful comments and suggestions. We would also like to thank the anonymous referee for feedback and thought-provoking questions on the manuscript.
Paper: 2015ApJ...804..119V (acknowledgments)
This project has received funding from the European Union’s Seventh Framework Programme for research, technological development, and demonstration under grant agreement no. 284515 (SHOCK). Website: project-shock.eu/home/. A.V. acknowledges the Interuniversity Attraction Poles Programme initiated by the Belgian Science Policy Office (IAP P7/08 CHARM). P.H. acknowledges grant P209/12/2023 of the Grant Agency of the Czech Republic. Computational resources were provided by CINECA (grant 2014 HP10CLF0ZB and HP10CNMQX2M).
Paper: 2019A&A...626A..24T (acknowledgments)
Acknowledgements The authors warmly thank Julien Milli, Grant Kennedy, and Jean-Charles Augereau for enlightening discussions.
Paper: 2017A&A...600A.124M (acknowledgments)
We thank the ISCRA staff for allowing us to perform our simulations on the Cineca Supercomputing Cluster GALILEO. We acknowledge P. F. Hopkins and G. Lodato for very useful discussion and comments on this work. E.R.C. acknowledges support by NASA through the Einstein Fellowship Program, grant PF6-170150. This work was also supported by the Packard grant and NASA ATP grant NNX14AH37G (ER). We also thank the referee, H. B. Perets, for valuable comments on the manuscript and very constructive suggestions.
Paper: 2015ApJ...804...19C (acknowledgments)
We acknowledge the CLUSTER FGM and EFW P.Is. and teams and the ESA Cluster Science Archive team for making the data used in this work available. The research leading to these results has received funding from the European Community’s Seventh Framework Programme ([FP7/2007–2013]) under grant agreement No. 313038/STORM. S.G. acknowledges support from the Agenzia Spaziale Italiana (ASI) under contract ASI-INAF n. I/022/10/2.
Paper: 2016MNRAS.460.4086M (acknowledgments)
This paper is based on observations made at the Laboratório Nacional de Astrofísica (LNA), Itajubá-MG, Brazil. The authors thank the referee Dr D. Pascu for his constructive comments. BM thanks the financial support by the CAPES/Brazil. MA thanks the CNPq (Grants 473002/2013-2 and 308721/2011-0) and FAPERJ (Grant E-26/111.488/2013). RVM acknowledges the following grants: CNPq-306885/2013, CAPES/Cofecub-2506/2015, FAPERJ/PAPDRJ-45/2013 and FAPERJ/CNE/05-2015. JIBC acknowledges CNPq for a PQ2 fellowship (process number 308489/2013-6). ADO is thankful for the support of the CAPES (BEX 9110/12-7) FAPERJ/PAPDRJ (E-26/200.464/2015) grants. ARGJ thanks CAPES/Brazil.