adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019A&A...630A.111B (acknowledgments)
We thank the anonymous referee for the constructive comments and suggestions. GB acknowledges financial support under the INTEGRAL ASI-INAF agreement 2013-025-R.1. EP acknowledges financial support from the Italian Space Agency (ASI) under the contracts ASI-INAF I/037/12/0 and ASI-INAF n.2017-14-H.0. LZ acknowledges financial support under ASI/INAF contract I/037/12/0. FT acknowledges support by the Programma per Giovani Ricercatori – anno 2014 Rita Levi Montalcini. This research project was supported by the DFG Cluster of Excellence “Origin and Structure of the Universe” ( www.universe-cluster.de ). Funding for the Sloan Digital Sky Survey IV has been provided by the Alfred P. Sloan Foundation, the US Department of Energy Office of Science, and the Participating Institutions. SDSS-IV acknowledges support and resources from the Center for High-Performance Computing at the University of Utah. The SDSS web site is www.sdss.org . SDSS-IV 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 Astrofísica 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, Observatário 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: 2018ApJ...859..110G (acknowledgments)
The authors acknowledge helpful discussions with Amitava Bhattacharjee, Kristopher G. Klein, William H. Matthaeus, Michael A. Shay, and Jason M. TenBarge. The research at University of Southern California was supported largely by the National Science Foundation (NSF) grant AGS-1202603 under the NSF/DOE Partnership in Basic Plasma Science and Engineering. S.P.G. and T.N.P. were primarily supported by NSF-SHINE grant AGS-1460130; S.P.G. was also supported in part by NASA LWS grant NNX17AH87G. Computational resources were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center, as well as by the Yellowstone supercomputer sponsored by the NSF at the Computational and Information Systems Laboratory of the National Center for Atmospheric Research. The data used to produce the results described here are archived at the University of Southern California and are available from Dr. Joseph Wang.
Paper: 2018ApJ...852...29K (acknowledgments)
We thank Smadar Naoz for kindly sharing the triple-evolution code OSPE . We also thank the referee for the useful suggestions. This work was supported by NASA ATP Grant NNX14AP92G and NSF Grants AST-1312945 and AST-1716762. K.K. acknowledges support by the National Science Foundation Graduate Research Fellowship Program under Grant DGE-1324585. S.C. acknowledges support from CIERA, and from NASA Chandra Award TM5-16004X/NAS8-03060, issued by the Chandra X-ray Observatory Center (operated by the Smithsonian Astrophysical Observatory for and on behalf of NASA under contract NAS8-03060), and Hubble Space Telescope Archival research grant HST -AR-14555.001-A (from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555). Software: CMC (Joshi et al. 2000 , 2001 ; Fregeau et al. 2003 ; Fregeau Rasio 2007 ; Chatterjee et al. 2010 , 2013 ; Umbreit et al. 2012 ; Morscher et al. 2015 ; Rodriguez et al. 2016b ), Fewbody (Fregeau et al. 2004 ), BSE (Hurley et al. 2002 ), OSPE (Naoz et al. 2011 , 2013 ).
Paper: 2020A&A...633A..97K (acknowledgments)
Acknowledgements J.K. has been funded by ERDF postdoctoral grant No. 1.1.1.2/VIAA/I/16/194 “Chemical effects of cosmic ray induced heating of interstellar dust grains”. The work of J.R.K. has been funded by ERDF project “Physical and chemical processes in the interstellar medium”, No 1.1.1.1/16/A/213. Both projects are being implemented in Ventspils University of Applied Sciences. We also thank Ventspils City Council for its persistent support.
Paper: 2017MNRAS.464.4448W (acknowledgments)
The cosmological simulations were performed using the ENZO code ( http://enzo-project.org ) and were partially produced at Piz Daint (ETHZ-CSCS, http://www.cscs.ch ) in the Chronos project ID ch2 and s585, and on the JURECA supercomputer at the NIC of the Forschungszentrum Jülich, under allocations nos. 7006 and 9016 (FV) and 9059 (MB). DW acknowledges support from the Deutsche Forschungsgemeinschaft (DFG) through grants SFB 676 and BR 2026/17. FV acknowledges personal support from the grant VA 876/3-1 from the DFG. FV and MB also acknowledge partial support from the grant FOR1254 from DFG. The distances in Section 3.4 and Appendix C have been computed using the Ned Cosmology Calculator (Wright 2006 ). We thank our anonymous referee for the useful feedback that helped improving the final quality of this paper. We also acknowledge fruitful discussions with T. Jones, K. Dolag and C. Gheller.
Paper: 2015MNRAS.454.2472H (acknowledgments)
We thank Jacqueline van Gorkom, Robyn Sanderson, and Adrian Price-Whelan for useful comments and discussions and the anonymous referee for a constructive review. The authors acknowledge the Shared Research Computing Facility (Yeti 2 ) at Columbia University for providing HPC resources that have contributed to the results reported in this paper. This work was supported by NSF grant no. AST-131296.
Paper: 2015MNRAS.448.1541S (acknowledgments)
RS acknowledges IUCAA visitor programme and AP acknowledges seed money grant from Tezpur University and visiting associateship of IUCAA, Pune. This research made use of data obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA's Goddard Space Flight Center. The authors would like to thank the anonymous referee for useful suggestions which has enhanced the quality of the paper.
Paper: 2017A&A...601A..93S (acknowledgments)
We thank the collaboration of Richard Saxton to the correction of the pile-up in the EPIC-pn camera, and fruitful conversations with Jordi José. This work is based on observations obtained with XMM-Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. G.S. acknowledges support from the Faculty of the European Space Astronomy Centre (ESAC) and the Max-Planck-Institut für extraterrestrische Physik (MPE). We acknowledge the support of the Spanish MINECO grants AYA2014-59084-P (G.S.) and ESP2015-66134-R (M.H.), and the Generalitat de Catalunya grants SGR0038/2014 (G.S.) and SGR 1458/2014 (M.H.).
Paper: 2018ApJ...854...16E (acknowledgments)
I am grateful to Dr. Ralf Klessen for discussions at an early stage of this research and to the referee for a careful reading of the manuscript.
Paper: 2017ApJ...841...54T (acknowledgments)
Comments from the anonymous referee helped to sharpen the presentation of our results. H.Y. thanks Jonah Miller for discussion of the numerical implementation of wave equations. This research was supported in part by NSERC and in part by the 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 Canada and by the Province of Ontario through the Ministry of Research Innovation, and Science.
Paper: 2016MNRAS.463.4175L (acknowledgments)
We would like to thank M. McCarthy, A. Vanderburg, and B. Montet for productive discussion and helpful comments on the manuscript. We also thank two anonymous referees for providing comments that greatly improved the quality of the manuscript. RAL gratefully acknowledges support from a National Science Foundation Graduate Research Fellowship. CNS wishes to thank the National Science Foundation for supporting the Astrochemistry programme at the University of Virginia. BAM and PBC are grateful to G. A. Blake for his support. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2019A&A...624A..48D (acknowledgments)
We thank Martin White, Vinu Vikram, and Adam Lidz for useful discussions. We thank Carlos Hernández-Monteagudo for useful comments on an early version of our paper. AdG was supported by the Edinburgh School of Physics and Astronomy Career Development Summer Scholarship and the RSE Cormack Vacation Research Scholarship. YC, JAP, and CH were supported by the European Research Council under grant numbers 670193 (YC; JAP) and 647112 (CH). We thank the Planck collaboration for making the full-sky y -map and κ -map publicly available and the SDSS collaboration for making public the CMASS galaxy catalogue. 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 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.
Paper: 2016MNRAS.457.2749J (acknowledgments)
We sincerely thank the referee for valuable comments and suggestions that improved the paper significantly. The research work at the Physical Research Laboratory is funded by the Department of Space, Government of India. The authors would like to thank all the members of the Suzaku team for their contributions to the instrument preparation, spacecraft operation, software development and in-orbit instrumental calibration. This research has made use of data obtained through the HEASARC Online Service, provided by NASA/GSFC, in support of NASA High Energy Astrophysics Programmes.
Paper: 2018ApJ...868..118H (acknowledgments)
We are grateful to S. Okuzumi and S. Arakawa for their fruitful discussion and help. We also appreciate the careful reading and fruitful comments by the anonymous referee. This work was supported by JSPS KAKENHI (15K05266).
Paper: 2018MNRAS.478.1866H (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank M. Takada, T. Sunayama, and T. Nishimichi for useful discussions. RH is supported by Japan Society for the Promotion of Science, Research Fellowships for Young Scientists (No. 16J01773) and as a doctoral course student in Division for Interdisciplinary Advanced Research and Education, Tohoku University. DJE is supported by U.S. Department of Energy grant DE-SC0013718 and as a Simons Foundation Investigator.
Paper: 2016MNRAS.459L...6E (acknowledgments)
AR is indebted to Programa Banco de Santander for a UAB-distinguished postdoctoral research contract. Financial support from MINECO (projects CTQ2015-62635-ERC and CTQ2014-60119-P) and DIUE (project 2014SGR482)are gratefully acknowledged. NB acknowledges the financial support from the Université Joseph Fourier de Grenoble and the Observatoire de Grenoble, CC acknowledges the financial support from the French Space Agency CNES.
Paper: 2019A&A...631A.178T (acknowledgments)
We thank Marty Snow for motivating us to carry out this study. We confirm that no funding has been received for it other than from universities, research institutes, and research councils. We thank the International Space Science Institute, Bern, Switzerland for providing financial support and meeting facilities that allowed stimulating discussions (ISSI Team 373 “Towards a Unified Solar Forcing Input to Climate Studies”). The research leading to this paper has received funding from STFC consolidated grants ST/N000838/1 and ST/S000372/1, from the European Research Council under the European Union Horizon 2020 research and innovation programme (grant agreement No. 715947) and the German Federal Ministry of Education and Research (Bundesministerium für Bildung und Forschung) under Project No. 01LG1209A. The SATIRE-S TSI and SSI reconstructions are available at http://www2.mps.mpg.de/projects/sun-climate/data.html . Finally, we thank the referee for their critical assessment of our work and the useful suggestions that helped to improve it significantly.
Paper: 2017ApJ...834..184C (acknowledgments)
This work is based on observations made at the Apache Point Observatory, operated by New Mexico State University. The scientific results reported in this article are based on observations made with the Chandra X-ray Observatory. Support for this work was provided by the National Aeronautics and Space Administration through Chandra Award Number GO3-14112X issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8-03060. This research has made use of software provided by the Chandra X-ray Center (CXC) in the application packages CIAO and ChIPS. This research has made use of the NASA/IPAC Extragalactic Database (NED) and the NASA/IPAC Infrared Science Archive (IRSA), which are operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This work is based on observations made with the NASA/ESA Hubble Space Telescope , and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA), and the Canadian Astronomy Data Centre (CADC/NRC/CSA). Data for this paper are provided in a presistent repository Chandra ObsId 14988. Facilities: ARC , CXO , VLBA .
Paper: 2019A&A...625A.107G (acknowledgments)
Acknowledgements We wish to thank an anonymous referee for many useful suggestions, which helped to improve an earlier version of the manuscript. We thank F. Borsa, I. Carleo, M. Damasso, R. de Kok, A. Maggio, I. Pagano for lending initial impetus to this analysis. G.G. acknowledges the financial support of the 2017 PhD fellowship programme of INAF. P.G. gratefully acknowledges support from the Italian Space Agency (ASI) under contract 2018-24-HH.0. 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: 2019ApJ...887...17Z (acknowledgments)
This work was made possible by the efforts of Gerard Lemson and colleagues at the German Astronomical Virtual Observatory in setting up the Millennium Simulation database in Garching. We acknowledge useful discussions with participants of the Shanghai Assembly Bias workshop in the final stages of this work. We thank the anonymous referee for helpful comments that improved the presentation of the paper. I.Z., S.C., E.J., and N.P. acknowledge the hospitality of the ICC at Durham University. I.Z. and S.E.K. acknowledge support by NSF grant AST-1612085. S.C. is supported by a Juan de la Cierva Formacion Fellowship (FJCI-2017-33816). E.J. acknowledges support from “Centro de Astronomía y Tecnologías Afines” BASAL 170002. N.P. acknowledges support from Fondecyt Regular 1191813. This project received financial support from the European Union’s Horizon 2020 Research and Innovation programme under the Marie Sklodowska-Curie grant agreement number 734374.
Paper: 2015A&A...579A..41S (acknowledgments)
The authors are grateful to the anonymous referee for constructive comments and suggestions that have improved this paper. Ch.H. and C.R.S. are grateful for the financial support of the European Community under the FP7 by an ERC starting grant number 257431. D.A.D. is grateful for funding from the UK Science and Technology Funding Council via grant number ST/I001808/1. It is a pleasure to acknowledge stimulating discussions with Drs H. E. Potts and P. B. Rimmer. Further to this, the authors would like to thank D. Juncher for discussions regarding dust opacity. The authors would like to acknowledge our local IT support.
Paper: 2016MNRAS.463.2574A (acknowledgments)
This work has made use of data obtained at the TNO on Doi Inthanon, operated by NARIT, and the PROMPT-8 telescope, operated by the Skynet Robotic Telescope Network. SA gratefully acknowledges the support from the Thai Government Scholarship and the University of Manchester President's Doctoral Scholar Award. VSD acknowledges the support of the Science and Technology Facilities Council (STFC) and the Leverhulme Trust for ULTRASPEC operations. TRM acknowledges the support of STFC through grant ST/L0007333.
Paper: 2019MNRAS.482.5430B (acknowledgments)
ACKNOWLEDGEMENTS We thank Omer Bromberg, Pawan Kumar, and Dimitrios Giannios for helpful discussions.
Paper: 2017ApJ...844...63O (acknowledgments)
This work was supported by the National Science Foundation, grant AST-1210285. M.R. acknowledges support from CONICYT (Chile) through FONDECYT grant No. 1140839 and partial support through project BASAL PFB-06. We also thank the anonymous referee for helpful comments.
Paper: 2015A&A...582A.118K (acknowledgments)
The authors acknowledge the open policy for the use of NRAOs VLA. The National Radio Astronomy Observatory (NRAO) is operated by Associated Universities Inc., under cooperative agreement with the National Science Foundation. Kambiz Fathi acknowledges support from the Swedish Royal Academy of Sciences’ Crafoord Foundation. Furthermore, the extensive support from the Swedish National Space Board (Rymdstyrelsen) is gratefully acknowledged by Aage Sandqvist. We also acknowledge with gratitude the support from Miller Goss with concatenation of the observations with the VLA in its BnA and DnC configurations.
Paper: 2017A&A...597A.124L (acknowledgments)
This research has made use of the MAXI data provided by RIKEN, JAXA and the MAXI team; Swift /BAT transient monitor results provided by the Swift /BAT team and data from the Fermi /GBM pulsar project. The authors thank Iain Steele for his help. E.L. is grateful for the warm hospitality of the MAXI team and thanks the IPA program in RIKEN for the support.
Paper: 2018MNRAS.479.4216M (acknowledgments)
ACKNOWLEDGEMENTS JWM dedicates the work in this paper to his father, William McKee. We thank Francis Graham-Smith, Gemma Janssen, Benjamin Shaw, Patrick Weltevrede, and Cristina Ilie for very helpful discussions, and the anonymous referees for useful comments. The authors acknowledge the support of their colleagues at Jodrell Bank Observatory. This work was supported by the UK Science and Technology Research Council, under grant number ST/L000768/1.
Paper: 2018A&A...615A..10M (acknowledgments)
We acknowledge Dr. Angeles Pérez-Villegas for critical reading of the manuscript and useful suggestions. This work was supported by the São Paulo State Science Foundation, FAPESP, and the Brazilian National Research Council, CNPq. R.S.S.V. acknowledges FAPESP grant 2015/10577-9. This work has made use of the facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by FAPESP (grant 2009/54006-4) and the INCT-A. We acknowledge the anonymous referee for the detailed review and for the helpful suggestions which allowed us to improve the manuscript.
Paper: 2017MNRAS.468.3150M (acknowledgments)
Acknowledgments We thank Diederik Kruijssen and Henny Lamers for constructive and helpful discussions on cluster mass-loss. We, in particular FN, NB, IP and VK-P, gratefully acknowledge financial support for this project provided by NASA through grant HST-GO-14069 for the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS526555. NB gratefully acknowledges financial support from the Royal Society (University Research Fellowship) and the European Research Council (ERC-CoG-646928-Multi-Pop). We are grateful to Jay Anderson for sharing with us his ePSF software. DG gratefully acknowledges support from the Chilean BASAL Centro de Excelencia en Astrofsica y Tecnologas Afines (CATA) grant PFB-06/2007.
Paper: 2017A&A...604A..15R (acknowledgments)
We would like to thank Ruud Visser for providing a detailed and clear referee’s report that helped to improve the paper. We also want to thank Zhaohuan Zhu for providing the burst spectrum of FU Orionis. CH.R. and E.V. acknowledge funding by the Austrian Science Fund (FWF): project number I2549-N27. CH.R. and M.G. acknowledge funding by the Austrian Science Fund (FWF): project number P24790. M.A. and A.P. acknowledge funding by the Swiss National Science Foundation (SNSF): project number: 200021L_163172. The research leading to these results has received funding from the European Union Seventh Framework Programme FP7-2011 under grant agreement No. 284405. This publication was partly supported from the FFG ASAP 12 project JetPro* (FFG-854025). This publication was supported by the Austrian Science Fund (FWF). The computational results presented have been achieved using the Vienna Scientific Cluster (VSC). This research has made use of NASA’s Astrophysics Data System. All figures were made with the free Python module Matplotlib ( Hunter 2007 ). This research made use of Astropy, a community-developed core Python package for Astronomy ( Astropy Collaboration et al. 2013 ).
Paper: 2016ApJ...826...64B (acknowledgments)
We are grateful to M. Geller, J. Najita, D. Wilner, and an anonymous referee for comments and helpful discussions. NASA provided essential support for this program through a generous allotment of computer time on the NCCS “discover” cluster and Outer Planets Program grant NNX11AM37G.