adsabs/WIESP2022-NER huggingface dataset:
Paper: 2016MNRAS.456..692M (acknowledgments)
The first author wish to thank the School of Astronomy, IPM for providing support while working on this paper. AM also acknowledges the Isaac Newton Group of Telescopes (ING) and the Instituto de Astrofísica de Canarias (IAC) for hospitality and support while this paper was in progress. We also thank an anonymous referee for a lot of constructive comments. The authors acknowledge support from the Spanish Ministry of Economy and Competitiveness (MINECO) through grants AYA2009-11137, AYA2013-48226-C3-1-P, AYA2013-46886-P and AYA2014-58308-P. JFB also acknowledges financial support from the DAGAL network from the People Programme (Marie Curie Actions) of the European Unions Seventh Framework Programme FP7/2007-2013/ under REA grant agreement number PITN-GA-2011-289313. 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 web site 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 Astrofísica 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.
Paper: 2015A&A...576A..11G (acknowledgments)
We are infinitely grateful to the staff members at the Nordic Optical Telescope for their valuable and unique support during the observations. We thank the editor and the anonymous referee for their careful review and very positive feedback. Davide Gandolfi thanks Gabriele Cologna for the interesting conversations on the properties of the planetary system. Hannu Parviainen has received support from the Rocky Planets Around Cool Stars (RoPACS) project during this research, a Marie Curie Initial Training Network funded by the European Commission’s Seventh Framework Programme. He has also received funding from the Väisälä Foundation through the Finnish Academy of Science and Letters and from the Leverhulme Research Project grant RPG-2012-661. Financial supports from the Spanish Ministry of Economy and Competitiveness (MINECO) are acknowledged by Hans J. Deeg for the grant AYA2012-39346-C02-02, by Sergio Hoyer for the 2011 Severo Ochoa program SEV-2011-0187, and Roi Alonso for the Ramón y Cajal program RYC-2010-06519. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission Directorate. The Kepler data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts. This research has made an intensive use of the Simbad database and the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in AAS, 143, 23.
Paper: 2017MNRAS.465.4658M (acknowledgments)
Acknowledgments The authors thank Volker Springel for providing us with gadget 3 , and Giuseppe Murante for useful discussion. Data post-processing and storage has been done on the CINECA facility PICO, granted us thanks to our expression of interest. Partial support from Consorzio per la Fisica di Trieste is acknowledged. EM has been supported by PRIN MIUR 2010-2011 J91J12000450001 The dark Universe and the cosmic evolution of baryons: from current surveys to Euclid and by a University of Trieste grant. PM has been supported by PRIN-INAF 2009 Towards an Italian Network for Computational Cosmology and by a F.R.A. 2012 grant by the University of Trieste. SB has been supported by PRIN MIUR 01278X4FL grant and by the InDark INFN Grant. SA has been supported by a Department of Energy grant de-sc0009946 and by NSF-AST 0908241.
Paper: 2017ApJ...842...18D (acknowledgments)
Most of the numerical calculations presented in this study were performed on the Savio computational cluster provided by the Berkeley Research Computing program at the University of California, Berkeley (supported by the UC Berkeley Chancellor, Vice Chancellor of Research, and Office of the CIO). We would like to thank the anonymous referee for the very thorough and detailed review, which resulted in a substantially improved manuscript. We would like to specifically acknowledge the referee for having the idea to estimate the value of from the “effective gravitational energy” released upon mixing.
Paper: 2019MNRAS.483.4551E (acknowledgments)
ACKNOWLEDGEMENTS We thank Carles Badenes for suggesting that we investigate the size distributions of SNRs. This material is based upon work supported by the National Science Foundation under grant no. 1313036.
Paper: 2018ApJ...865...38N (acknowledgments)
This work was supported by the International Center of Future Science of Jilin University (P.R. China) and the project of Ministry of Education and Science of Ukraine “Dynamics, evolution and physical effects in the formation of structure of the universe, supernova remnants and close binary stars with relativistic components” (state registration no. 0116U001544).
Paper: 2016ApJ...823...58M (acknowledgments)
The authors thank Rachel Akeson, John Carpenter, Kevin Flaherty, Lynne Hillenbrand, Heather Knutson, Patrick Ogle, Inseok Song, Karl Stapelfeldt, and Barbara Whitney for their contributions to the YSOVAR project and valuable discussions on this work. H.Y.A.M. acknowledges support from the IPAC Visiting Graduate Research Fellowship program. P.P. acknowledges the work of Nancy Silbermann, William Mahoney, and the Spitzer scheduling team in scheduling the data volume-intensive observations, and thanks Greg Doppmann for providing the Keck/NIRSPEC spectrum. K.C. acknowledges support provided by the NSF through grant AST-1449476. A.M.W. thanks the staff of the Observatorio Astronómico Nacional in Sierra San Pedro Mártir. This work is based in part on observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. Support for this work was provided by NASA through an award issued by JPL/Caltech. Facilities: CTIO:1.3 m , Mayall , OANSPM:HJT , SOAR , Spitzer (IRAC).
Paper: 2015A&A...574A..83K (acknowledgments)
Dust studies at Leiden Observatory are supported through the Spinoza Premie of the Dutch science agency, NWO. S.K. would like to thank C.P. Dullemond, J. Dra ̧żkowska and T. Birnstiel for useful discussions, and S. Okuzumi for comments and helping with the comparison to his work. The authors thank B. Gundlach and J. Blum for sharing a version of their manuscript. C.W.O. acknowledges support for this work by NASA through Hubble Fellowship grant No. HST-HF-51294.01-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: 2016MNRAS.456.2636L (acknowledgments)
This work has been supported by the Australian Research Council (grants FL110100012, FT140100554 and DP120100991). JM thanks support by FAPESP (2012/24392-2). DLL thanks the Robert A. Welch Foundation of Houston, Texas for support through grant F-634. TB was supported by the project grant ‘The New Milky Way’ from the Knut and Alice Wallenberg Foundation. Australian access to the Magellan Telescopes was supported through the Collaborative Research Infrastructure Strategy of the Australian Federal Government. The Canada–France–Hawaii Telescope is operated by the National Research Council of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The Hobby–Eberly Telescope is a joint project of the University of Texas at Austin, the Pennsylvania State University, Ludwig-Maximilians-Universität München, and Georg-August-Universität Göttingen.
Paper: 2017MNRAS.469.1414K (acknowledgments)
Acknowledgments DW was supported by NSF grant 1518246. We thank Marua Brada, Marcus Brggen, James Bullock, Will Dawson, James Jee, Manoj Kaplinghat, Reinout van Weeren and David Sobral for discussions that shaped the direction of this project, and for their careful reading of the manuscript. The Merging Cluster Collaboration has provided valuable input to this project. We thank the Ohio Supercomputer Center for the use of the Ruby cluster during its commissioning phase.
Paper: 2015MNRAS.450..333S (acknowledgments)
We thank F. Mignard and Ch. Ordenovich (OCA, Nice) for putting at our disposal the use of the Gaia simulator of Solar system observations. The work of TSR was carried out through the Gaia Research for European Astronomy Training (GREAT-ITN) network. He received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement no. 264895. The work of AC was partly funded by ASI contract I/058/10/0.
Paper: 2018ApJ...866..109S (acknowledgments)
We thank the anonymous referee for constructive comments.
Paper: 2019ApJ...884....6M (acknowledgments)
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. We acknowledge support provided by the NSF through grant AST-1449476, and from the Research Corporation via a Time Domain Astrophysics Scialog award (#24217). We acknowledge funding support for this work from NASA ADAP grant 80NSSC19K0591.
Paper: 2017MNRAS.465.2862S (acknowledgments)
Acknowledgments We would like to thank Tamara Davis for useful comments on a draft of this paper. DS thanks the Faculty of Technology of the University of Portsmouth for support during his PhD studies. DB, EM and RCN acknowledge funding from STFC grant ST/N000668/1 and EM acknowledges the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020.
Paper: 2016MNRAS.460.1529U (acknowledgments)
This work is partially supported by the grants ANR-12-BS05-0002 and ANR-13-BS05-0005 of the French Agence Nationale de la Recherche. CU is supported by the Delta-ITP consortium, a program of the Netherlands organization for scientific research (NWO) that is funded by the Dutch Ministry of Education, Culture and Science (OCW). CU thanks IAP for hospitality when this project was initiated and the Balzan Centre for Cosmological Studies for financial support during the visit. The simulations were run on the Horizon cluster. We acknowledge support from S. Rouberol for running the cluster for us.
Paper: 2016MNRAS.463.2864A (acknowledgments)
SNXM acknowledges IMPRS for a PhD research scholarship. SJA, WJH and SNXM would like to thank DGAPA-UNAM for financial support through projects PAPIIT IN101713 and IN112816. This work has made use of NASA's Astrophysics Data System.
Paper: 2016A&A...591A.122S (acknowledgments)
Herschel is a European Space Agency space observatory with science instruments provided by European-led principal investigator consortia and with important participation from NASA. HIFI has been designed and built by a consortium of institutes and university departments from across Europe, Canada, and the United States under the leadership of SRON Netherlands Institute for Space Research, Groningen, The Netherlands, and with major contributions from Germany, France, and the US. Consortium members are: Canada: CSA, U. Waterloo; France: IRAP (formerly CESR), LAB, LERMA, IRAM; Germany: KOSMA, MPIfR, MPS; Ireland, NUI Maynooth; Italy: ASI, IFSI-INAF, Osservatorio Astrofisico di Arcetri-INAF; Netherlands: SRON, TUD; Poland: CAMK, CBK; Spain: Observatorio Astronmico Nacional (IGN), Centro de Astrobiología (CSIC-INTA). Sweden: Chalmers University of Technology MC2, RSS GARD; Onsala Space Observatory; Swedish National Space Board, Stockholm University Stockholm Observatory; Switzerland: ETH Zurich, FHNW; USA: Caltech, JPL, NHS. Support for this work was provided by NASA ( Herschel OT funding) through an award issued by JPL/Caltech. This work was partially supported by grants from the Netherlands Organization for Scientific Research (NWO) and the Netherlands Research School for Astronomy (NOVA). The data presented here are archived at the Herschel Science Archive, http://archives.esac.esa.int/hda/ui , under OBSID 1342198337 and 1342201585.
Paper: 2016MNRAS.457.1190G (acknowledgments)
We thank Laurent Gizon and Gert Lube for encouragement and support. Research funding by the Deutsche Forschungsgemeinschaft (DFG) under grant SFB963/1, project A11, is gratefully acknowledged.
Paper: 2017MNRAS.464.2910S (acknowledgments)
This research was based in part 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 (USA), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovaļão (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina). Elements of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. 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 research has made use of NASA's Astrophysics Data System. 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. This research was conducted with the support of Australian Research Council DP130101667. We thank the International Telescope Support Office and Gemini Observatory for contributing travel funding.
Paper: 2015MNRAS.448.1360W (acknowledgments)
AAW is supported by the Science and Technology Facilities Council. We thank Jason Sanders and Carlo Nipoti for some useful conversations, as well as the referee for a thorough and useful report.
Paper: 2016ApJ...828...58G (acknowledgments)
C.F.G.’s work was supported, in part, by a Romano Professorial Scholar appointment, a Simons Fellowship in Theoretical Physics, and a Visiting Fellowship at All Souls College, Oxford. We thank S. Desch, C. Thompson, M. Chandra, B. Ryan, J. Papaloizou, and C. Terquem for comments, and the referee, S. Charnoz, for a thoughtful report that greatly improved the manuscript.
Paper: 2016ApJ...827...20S (acknowledgments)
We thank the referee for thoughtful and constructive feedback on this work. We acknowledge our colleagues in the CANDELS collaboration for very useful comments and suggestions. We also thank the great effort of all the CANDELS team members for their work to provide a robust and valuable data set. We thank Karl Gordon for insightful discussions on the physical implications of these results. We also thank Daniela Calzetti and Veronique Buat for helpful comments and comments. This work is based in part on observations taken by the CANDELS Multi-Cycle Treasury Program with the NASA/ESA HST , which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. This work is supported by HST program No. GO-12060. Support for Program No. GO-12060 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555. We acknowledge the Spanish MINECO grant AYA2012-31277 for funding the contribution from Pablo Pérez-González. This work is based in part on observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology under contract with the National Aeronautics and Space Administration (NASA). The authors acknowledge the Texas AM University Brazos HPC cluster that contributed to the research reported here. URL: http://brazos.tamu.edu .
Paper: 2016ApJ...827..145R (acknowledgments)
The authors also thank the anonymous referee for comments that strengthened the arguments in this paper. The authors thank Lucas Tarr and George Doschek for discussions that improved the modeling and understanding of this event. This research was performed while J.W.R. held an NRC Research Associateship award at the US Naval Research Laboratory with the support of NASA. The research leading to these results has received funding from the European Community’s Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 606862 (F-CHROMA) (PJAS). IRIS is a NASA Small Explorer developed and operated by LMSAL with mission operations executed at NASA Ames Research center and major contributions to downlink communications funded by the Norwegian Space Center through an ESA PRODEX contract. CHIANTI is a collaborative project involving George Mason University, the University of Michigan (USA) and the University of Cambridge (UK).
Paper: 2018ApJ...859..116K (acknowledgments)
This work was supported by the National Key RD Program of China (2016YFA0400702), the National Science Foundation of China (11473002, 11721303), the National Youth Fund (11303008), and the Youth Foundation of Hebei Province of China (A2011205067). We thank Jenny Greene for sending the data from Greene Ho ( 2005a ). M.K. is grateful to Jian-Min Wang for his hospitality and help during her visit to IHEP and to JinLin Han for his help during her stay at NAOC. She thanks Song Huang, Ligang Hou, Xianmin Meng, Jinyi Shangguan, Jiayi Sun, and Junzhi Wang for their help. Funding for the SDSS 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 website 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.
Paper: 2015A&A...578A...3G (acknowledgments)
The observations have been supported by the OPTICON project (observing proposals 2010B/01, 2011A/014 and 2012A/015), which is funded by the European Commission under the Seventh Framework Programme (FP7). Part of the observations have been taken under service mode (service proposal AO171) and the authors gratefully acknowledge the help of the AAO support astronomers. This research is partially supported by the Spanish Ministerio de Economía y Competitividad (Mineco) under grant AYA2012-39364-C02-02. The work reported on in this publication has been partially supported by the European Science Foundation (ESF), in the framework of the GREAT Research Networking Programme. This research was achieved using the POLLUX database ( http://pollux.graal.univ-montp2.fr ) operated at LUPM (Université Montpellier II CNRS, France with the support of the PNPS and INSU. This research made use of the Simbad, Vizier, and Aladin services developed at the Centre de Données Astronomiques de Strasbourg, France. 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.
Paper: 2018A&A...612A..65B (acknowledgments)
Acknowledgements We are grateful to our referee Mike Bessell for his very thorough and useful report of our paper. The project is supported by fondation MERAC. N.C., H.G.L., and A.J.G. were supported by Sonderforschungsbereich SFB 881 “The Milky Way System” (subproject A4) of the German Research Foundation (DFG). R.S.K. acknowledges support from the European Research Council via the Advanced Grant “STARLIGHT: Formation of the First Stars” (project number 339177). C.A. acknowledges funding from the Alexander von Humboldt Foundation.
Paper: 2015A&A...574A.117M (acknowledgments)
We thank the referee for the helpful comments, and R. Schulz and P.G. Edwards for the useful discussions that improved the manuscript. C.M. acknowledges the support of the Bundesministerium für Wirtschaft und Technologie (BMWi) through Deutsches Zentrum für Luft- und Raumfahrt (DLR) grant 50 OR 1404 and of the Studienstiftung des Deutschen Volkes. This research was funded in part by the National Aeronautics and Space Administration (NASA) through Fermi Guest Investigator grants NNH09ZDA001N, NNH10ZDA001N, and NNH12ZDA001N, by BMWi through DLR grant 50 OR 1311, by Deutsche Forschungsgemeinschaft grant WI1860/10-1, and by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA. We thank J. E. Davis for the development of the slxfig module that has been used to prepare the figure in this work. This research has made use of ISIS functions provided by ECAP/Dr. Karl Remeis-Observatory (Bamberg, Germany) and MIT ( http://www.sternwarte.uni-erlangen.de/isis/ ).
Paper: 2019MNRAS.487.5549B (acknowledgments)
ACKNOWLEDGEMENTS We are most grateful to Volker Springel for allowing us to use the gadget -3 code. This work is supported by the Brazilian Agencies FAPESP (grants 2016/01355-5, 2016/22183-8, and 2013/10559-5) and by CNPq (grant 308643/2017-8).
Paper: 2019A&A...623A.123G (acknowledgments)
The authors thank the referee, Kyle Oman, for the excellent suggestions and for providing us with the APOSTLE/EAGLE V Rlast and V rot (2 kpc) simulated data points. We also thank Aaron Dutton for providing us with the NIHAO RAR at 2 kpc. We acknowledge useful discussions with Federico Lelli and Stacy McGaugh.