adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017MNRAS.472.4551E (acknowledgments)
Acknowledgements The anonymous referee is thanked for providing comments and feedback that improved the overall quality of the paper. ECE acknowledges the support of the South African National Astrophysics and Space Science Programme (NASSP).
Paper: 2019A&A...629A.134G (acknowledgments)
We thank the anonymous referee for a constructive report that helped improve the manuscript. The authors also acknowledge various people for helpful and inspiring discussion at various stages during the preparation of this manuscript, including Evan Bauer, Jared Brooks, Maria Drout, JJ Eldridge, Chris Evans, Rob Farmer, Miriam Garcia, Stephan Geier, Zhanwen Han, Edward van den Heuvel, Stephen Justam, Lex Kaper, Alex de Koter, Søren Larsen, Danny Lennon, Pablo Marchant, Colin Norman, Philipp Podsiadlowski, Onno Pols, Mathieu Renzo, Hugues Sana, Tomer Shenar, Nathan Smith, Elizabeth Stanway, Silvia Toonen, Jorick Vink, Manos Zapartas and the VFTS collaboration. This work was carried out on the Dutch national e-infrastructure with the support of SURF Cooperative. The authors acknowledges John Hillier for making his code, CMFGEN, publicly available. YG thank Martin Heemskerk for providing computing expertise and support throughout the project and Alessandro Patruno for allowing us to use the Taurus computer. SdM has received funding under the European Union’s Horizon 2020 research and innovation program from the European Research Council (ERC) (Grant agreement No. 715063). JHG acknowledges support from the Irish Research Council New Foundations Award 206086.14414 “Physics of Supernovae and Stars”. This work made use of v2.2.1 of the Binary Population and Spectral Synthesis (BPASS) models as last described in Eldridge et al. (2017) and Stanway Eldridge (2018) .
Paper: 2016A&A...586A.106G (acknowledgments)
We thank Christophe Sandt (SOLEIL) for his help with the infrared microscope at the SMIS beam line. VUV measurements were made at the DISCO beam line of the SOLEIL synchrotron radiation facility (projects: 20141074 and 20130778). This work has been supported by the French program “Physique et Chimie du Milieu Interstellaire”, the ANR COSMISME project (grant ANR-2010-BLAN-0502). L.G. acknowledges support from the CNES post-doctoral fellowship program.
Paper: 2016MNRAS.461..908B (acknowledgments)
This scientific work makes use of the Murchison Radio-astronomy Observatory, operated by CSIRO. We acknowledge the Wajarri Yamatji people as the traditional owners of the Observatory site. Support for the operation of the MWA is provided by the Australian Government Department of Industry and Science and Department of Education (National Collaborative Research Infrastructure Strategy: NCRIS), under a contract to Curtin University administered by Astronomy Australia Limited. We acknowledge the iVEC Petabyte Data Store and the Initiative in Innovative Computing and the CUDA Center for Excellence sponsored by NVIDIA at Harvard University. JKS is supported from NSF Physics Frontier Center award number 1430284. DLK and SDC acknowledge support from the US National Science Foundation (grant AST-1412421). Parts of this research were conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020. This work was supported by the Flagship Allocation Scheme of the NCI National Facility at the ANU.
Paper: 2015MNRAS.450.2094G (acknowledgments)
We acknowledge financial support from PRIN MIUR 2010-2011, project ‘The Chemical and dynamical Evolution of the Milky Way and Local Group Galaxies’, prot. 2010LY5N2T. NR acknowledges support from the Swedish Research Council, VR (project number 621-2014-5640), Funds from Kungl. Fysiografiska Sällskapet i Lund. (Stiftelsen Walter Gyllenbergs fond and Märta och Erik Holmbergs donation). NR acknowledges the supports from Knut och Alice Wallenbergs stiftelse. We thank I. J. Danziger for reading the manuscript. Finally, we thank an anonymous referee for his/her important suggestions which improved the paper.
Paper: 2017A&A...608A..88B (acknowledgments)
The authors thank the referee for his/her comments. The scientific results reported in this article are based on data obtained from the Chandra Data Archive and observations obtained with XMM - Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP72007-2013) ERC grant agreement No. 340519. M.A., P.M., E.P., and G.W.P. acknowledge partial funding support from NASA grant NNX14AC22G. F.A.-S. acknowledges support from Chandra grant GO3-14131X.
Paper: 2016ApJ...832..153L (acknowledgments)
The authors would like to thank the anonymous referee whose constructive comments helped to improve the clarity of the manuscript. This work was supported by funds from the Academia Sinica Institute of Astronomy and Astrophysics (ASIAA), and the Ministry of Science and Technology (MoST) of Taiwan by grant NSC 102-2119-M-001-008-MY3. This work is partly based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme 084.C-1095(A). The HST /STIS spectra were obtained from the Mikulski Archive for Space Telescopes (MAST) at the Space Telescope Science Institute (STScI). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. Facilities: HST (STIS) , VLT:Kueyen (X-Shooter) .
Paper: 2016A&A...590A.114M (acknowledgments)
The research leading to these results was funded by the European Community’s Seventh Framework Programme (FP7/2007–2013) under grant agreement number ITN 215212 “Black Hole Universe” and by the Bundesministerium für Wirtschaft und Technologie under grant numbers DLR 50 OR 0701 and 50 OR 1113. This work was partially completed by Lawrence Livermore National Laboratory (LLNL) under Contract DE-AC52-07NA27344, and is supported by NASA grants to LLNL. Support for this work was also provided by NASA through the Smithsonian Astrophysical Observatory (SAO) contract SV3-73016 to MIT for Support of the Chandra X-Ray Center (CXC) and Science Instruments; CXC is operated by SAO for and on behalf of NASA under contract NAS8-03060. We acknowledge the support by the DFG Cluster of Excellence “Origin and Structure of the Universe” and are grateful for the support by MCB through the Computational Center for Particles and Astrophysics (C2PAP). We are thankful to John E. Davis for the SLXfig package that was used to create the figures throughout this paper, to David Huenemoerder for the AGLC routines that handled the grating lightcurves and routines related to plasma diagnostics, and to Thomas Dauser for parallel computing routines. This research has made use of the MAXI data provided by RIKEN, JAXA, and the MAXI team.
Paper: 2015MNRAS.450.4109B (acknowledgments)
The Parkes telescope and the ATCA are both part of the Australia Telescope which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. Financial support for this work was provided by the Australian Research Council. This research has made use of NASA's Astrophysics Data System Abstract Service; and the SIMBAD data base, operated at CDS, Strasbourg, France. SLB is the recipient of an Australian Research Council DECRA Fellowship (project number DE130101270). The authors dedicate this paper to the memory of J. L. Caswell, who was the driving force behind the MMB survey, and will continue to inspire maser studies for years to come.
Paper: 2015MNRAS.446.1380P (acknowledgments)
Pulsar research at the Jodrell Bank Centre for Astrophysics and the observations using the Lovell Telescope is supported by a consolidated grant from the STFC in the UK.
Paper: 2017MNRAS.469.4422C (acknowledgments)
Acknowledgments We thank Eric Huff, Melanie Simet and Rachel Mandelbaum for useful discussions, and also the anonymous referee for pointing out problems with the method involving the mixing of deconvolved and directly measured parameters and several other changes which improved the paper. This work is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique (CNRS) of France and the University of Hawaii. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency. CFHTLenS data processing was made possible thanks to significant computing support from the NSERC Research Tools and Instruments grant program.
Paper: 2019MNRAS.485.3296W (acknowledgments)
ACKNOWLEDGEMENTS We gratefully acknowledge useful discussions with Isabella Söldner-Rembold regarding the velocity ellipsoid, and numerous helpful discussions with Matias Blaña. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 798384. This work has made use of data from the European Space Agency (ESA) mission Gaia , processed by the Gaia Data Processing and Analysis Consortium ( DPAC ). Funding for the DPAC has been provided by national institutions, in particular the institutions participating in the Gaia Multilateral Agreement. The Pan-STARRS1 Surveys (PS1) and the PS1 public science archive have been made possible through contributions by the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society, and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, the Queen’s University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, and the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation Grant No. AST-1238877, the University of Maryland, Eotvos Lorand University (ELTE), the Los Alamos National Laboratory, and the Gordon and Betty Moore Foundation.
Paper: 2018ApJ...854..187L (acknowledgments)
We thank Slavko Bogdanov, Simin Mahmoodifar, Sharon Morsink, Joonas Nättilä, Feryal Özel, Juri Poutanen, Dimitrios Psaltis, and Tod Strohmayer for useful discussions.
Paper: 2016MNRAS.459...70V (acknowledgments)
This work was strongly supported by computing resources from the Swiss National Supercomputing Centre (CSCS) under projects ID ch2 and s585 in 2014–2015. FV acknowledges personal support from the grant VA 876/3-1 from the Deutsche Forschungsgemeinschaft. FV and MB also acknowledge partial support from the grant FOR1254 from the Deutsche Forschungsgemeinschaft. We acknowledge the use of computing resources under allocations no. 7006 and 9016 (FV) and 9059 (MB) on supercomputers at the NIC of the Forschungszentrum Jülich. We acknowledge the use of the online ‘Cosmology Calculator’ by Wright ( 2006 ). We thank K. Dolag for very fruitful discussions at an early stage of this work, and our referee H. Kang for very useful comments on the manuscript.
Paper: 2015A&A...575L...1P (acknowledgments)
We thank A.S. Rivkin and P. Vernazza for kindly providing their spectral data. The research of Z.K. is supported by VEGA – The Slovack Agency for Science, Grant No. 2/0032/14. This program was supported by the French national space agency CNES and French INSU – PNP program.
Paper: 2016MNRAS.457.4179H (acknowledgments)
We thank the referee for a very helpful report. Herschel is an ESA space observatory with instruments provided by European-led Principal Investigator consortia and with participation from NASA. The Herschel spacecraft was designed, built, tested, and launched under a contract to ESA managed by the Herschel / Planck Project team by an industrial consortium under the overall responsibility of the prime contractor Thales Alenia Space (Cannes), and including Astrium (Friedrichshafen) responsible for the payload module and for system testing, Thales Alenia Space (Turin) responsible for the service module, and Astrium (Toulouse) responsible for the telescope, with in excess of a hundred subcontractors. SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including: Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); and Caltech, JPL, NHSC, Univ. Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC, UKSA (UK); and NASA (USA). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the U.S. Department of Energy Office of Science. 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. AF acknowledges support from the ERC via an Advanced Grant 321323-NEOGAL.
Paper: 2015ApJ...799...18C (acknowledgments)
We thank Wesley Even, Sean M. Couch, Donald Q. Lamb, Ryan Chornock, Ken Chen, Alexandra Kozyreva, and Ragnhild Lunnan for useful discussions and comments. This work was supported in part by the STScI grants AR 12820 and 13276 and the National Science Foundation under grants AST-0909132 and PHY-0822648 for the Physics Frontier Center “Joint Institute for Nuclear Astrophysics” (JINA). E.C. thanks the Enrico Fermi Institute for its support via the Enrico Fermi Fellowship.
Paper: 2019A&A...624A.108L (acknowledgments)
The authors would like to thank Profs. Guillermo Muñoz Caro and Maria Palumbo for conversations about laboratory studies of sulfur-containing ices, Prof. Susanna Widicus Weaver about gas-grain modeling, and Profs. John Black and David Neufeld about observations. JL would also like to thank Dr. Wing-Fai Thi for helpful feedback during the development of the astrochemical code.
Paper: 2017MNRAS.465.3011C (acknowledgments)
Acknowledgments This work was supported by the UKs Science and Technology Facilities Council, grant numbers ST/J001333/1, ST/M001008/1 and ST/L001403/1. We gratefully acknowledge the use of data from the ESO Public Survey program 179.B-2002 taken with the VISTA 4.1m telescope and data products from the Cambridge Astronomical Survey Unit. Support for DM and CC is provided by the Ministry of Economy, Development, and Tourisms Millennium Science Initiative through grant IC120009, awarded to the Millennium Institute of Astrophysics, MAS. DM is also supported by the Center for Astrophysics and Associated Technologies PFB-06 and Fondecyt Project No. 1130196. MSNK is supported by the Marie-Curie Intra-European fellowship project GESTATE (661249). This research has made use of the SIMBAD data base, operated at CDS, Strasbourg, France; also the SAO/NASA Astrophysics data (ADS). ACG was supported by the Science Foundation of Ireland, grant 13/ERC/I2907. We also acknowledge the support of CONICYT REDES project No. 140042 Young variables and proper motion in the Galactic plane. ValparaisoHertfordshire collaboration C. Contreras Pea was supported by a University of Hertfordshire PhD studentship in the earlier stages of this research. We thank Janet Drew for her helpful comments on the structure of the paper.
Paper: 2019MNRAS.487.5721G (acknowledgments)
ACKNOWLEDGEMENTS We thank Francis-Yan Cyr-Racine, Giulia Despali, Chuck Keeton, Stacy Kim, Alex Kusenko, Leonidas Moustakas, Annika Peter, and Simona Vegetti for helpful suggestions and interesting discussions throughout the course of this project. We also thank the anonymous referee for comments that improved the quality of this work. DG, TT, and SB acknowledge support by the US National Science Foundation through grant AST-1714953. DG, TT, SB and AN acknowledge support from HST-GO-15177. Support for Program number GO-15177 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. AN acknowledges support from the NASA Postdoctoral Program Fellowship. This work used computational and storage services associated with the Hoffman2 Shared Cluster provided by the UCLA Institute for Digital Research and Education’s Research Technology Group. This work also used computational and storage services associated with the Aurora and Halo supercomputers. These resources were provided by funding from the JPL Office of the Chief Information Officer.
Paper: 2018ApJ...859...12G (acknowledgments)
We thank the anonymous referee for her/his helpful and thorough reading of the manuscript, as well as for suggestions that improved the paper. B.G., E.A.C., and I.R.S. acknowledge support from the ERC Advanced Programme DUSTYGAL (321334) and STFC (ST/P0000541/1). I.R.S. also acknowledges support from a Royal Society Wolfson Merit Award. J.L.W. acknowledges support from a European Union COFUND/Durham Junior Research Fellowship (EU grant agreement number 609412) and from STFC (via an Ernest Rutherford Fellowship: ST/P004784/1, and additionally ST/P0000541/1) E.I. acknowledges partial support from FONDECYT through grant N° 1171710. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.00456.S ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada), MOST and ASIAA (Taiwan), as well as KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ.
Paper: 2019MNRAS.489.2395T (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank the referee, Artie Hatzes, for carefully reading the manuscript and supporting its conclusions. We also thank the members of the EXPRES and HARPS-N GTO teams for useful input and fruitful discussions. Our simulations involved an extensive amount of coordinate transformations made possible with the excellent astropy.coordinates module 3 (Astropy Collaboration et al. 2013 ; Price-Whelan et al. 2018 ). All figures were prepared with matplotlib 4 (Hunter 2007 ). The Center for Exoplanets and Habitable Worlds is supported by the Pennsylvania State University, the Eberly College of Science, and the Pennsylvania Space Grant Consortium.
Paper: 2019MNRAS.488.4440A (acknowledgments)
ACKNOWLEDGEMENTS This work is supported by the Simons Foundation. JA was partially supported by the research project grant ‘Fundamental Physics from Cosmological Surveys’ funded by the Swedish Research Council (VR) under Dnr 2017-04212. BW acknowledges support by the Labex Institut Lagrange de Paris (ILP) (reference ANR-10-LABX-63) part of the Idex SUPER, and received financial state aid managed by the Agence Nationale de la Recherche, as part of the programme Investissements d’avenir under the reference ANR-11-IDEX-0004-02. TC is supported by the ANR BIG4 grant ANR-16-CE23-0002 of the French Agence Nationale de la Recherche and would like to thank NVIDIA for the donation of the Quadro P6000 used in building and testing pydelfi .
Paper: 2019MNRAS.482.3341C (acknowledgments)
ACKNOWLEDGEMENTS It is a pleasure to thank David Alonso, Philip Bull, and Laura Wolz for very useful discussions and feedback. We also extend our gratitude to the referee whose report improved the quality of this paper. SC is supported by the University of Portsmouth. AP’s work for this project was partly supported by a Dennis Sciama Fellowship at the University of Portsmouth. DB is supported by STFC consolidated grant ST/N000668/1.
Paper: 2018ApJ...863..196M (acknowledgments)
The authors thank Julian Carlin for assistance with the preparation of Figures 2 and 4 . This research was supported by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav), grant number CE170100004. G.H. is the recipient of an Australian Postgraduate Award. This work was performed in part at the Aspen Center for Physics, which is supported by National Science Foundation grant PHY–1607611.
Paper: 2019ApJ...879...82P (acknowledgments)
The authors acknowledge the use of the Wind MFI magnetic field and SWE proton data. This work is supported by the Czech Grant Agency under contracts 19-18993S. A.P. thanks the Charles University Grant Agency, project No. 1484217. We appreciate the fruitful discussions with Owen Roberts, Simone Landi, Peter Hellinger, and Honghong Wu. This research was partially supported by the UK Science and Technology Facilities Council (STFC) grant ST/P000622/. Facilities: Wind , Spektr-R .
Paper: 2017ApJ...840..108K (acknowledgments)
We thank the staff of the Giant Metrewave Radio Telescope (GMRT), who have made these observations possible. The GMRT is run by the National Centre for Radio Astrophysics of the Tata Institute of Fundamental Research. This research was partially supported by the grant DEC-2013/09/B/ST9/02177 of the Polish National Science Centre.
Paper: 2015MNRAS.454.1697X (acknowledgments)
Phoenix and Aquarius are projects of the Virgo Consortium. Most simulations were carried out on the Lenova Deepcomp7000 supercomputer of the Supercomputing Center of Chinese Academy of Sciences, Beijing, China, and on Cosmology machine at the Institute for Computational Cosmology (ICC) at Durham. The Cosmology machine is part of the DiRAC facility jointly founded by STFC, the large facilities capital fund of BIS, and Durham University. LG acknowledges support from NSFC grants (nos. 11133003 and 11425312), MPG partner Group family, and an STFC Advanced Fellowship, as well as the hospitality of the Institute for Computational Cosmology at Durham University.
Paper: 2017A&A...606L...2A (acknowledgments)
Based on observations obtained with Planck and Herschel , ESA science missions with instruments and contributions directly funded by ESA Member States, NASA, and Canada. This research has made use of NASA’s Astrophysics Data System. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. This research has made use of Astropy, a community-developed core Python package for Astronomy ( Astropy Collaboration et al. 2013 ). This research has made use of TOPCAT, an interactive graphical viewer and editor for tabular data ( Taylor 2005 ).