adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019ApJ...882...90L (acknowledgments)
The authors wish to thank Julia Lawless for useful discussions and the anonymous referee for very detailed suggestions that helped clarify the manuscript. D.M.L. acknowledges support from the European Commission’s H2020 Programme under the following Grant Agreements: GREST (No. 653982) and Pre-EST (No. 739500) as well as support from the Leverhulme Trust for an Early Career Fellowship (ECF-2014-792) and is grateful to the Science Technology and Facilities Council for the award of an Ernest Rutherford Fellowship (ST/R003246/1). G.V. was funded by the Leverhulme Trust under grant 2014-051. J.M.J. thanks the STFC for support via funding given in his PhD Studentship. Facilities: SDO , GONG. Software: SolarSoftWare (Freeland Handy 1998 ).
Paper: 2017MNRAS.471.4637K (acknowledgments)
Acknowledgements This work is supported by Labex ESEP (ANR N 2011-LABX-030) and by the Russian Foundation for Basic Research, project no. 16-52-150005-CNRS-a. The work of RSS was carried out while he was working at Université de Lille – Laboratoire Paul Painlevé.
Paper: 2017MNRAS.471.3888S (acknowledgments)
Acknowledgements We thank the anonymous referee for comments and suggestions which have improved this paper. This work is based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the Science and Technology Facilities Council (United Kingdom), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência e Tecnologia (Brazil) and south-eastCYT (Argentina). This work has been partially supported by the Brazilian institution CNPq.
Paper: 2015A&A...576A.106P (acknowledgments)
The development of Planck has been supported by: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MICINN, JA and RES (Spain); Tekes, AoF and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); and PRACE (EU). A description of the Planck Collaboration and a list of its members, including the technical or scientific activities in which they have been involved, can be found at http://www.sciops.esa.int/index.php?project=planckpage=Planck_Collaboration . The research leading to these results has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP7/20072013) / ERC grant agreement No. 267934. This research has made use of the SIMBAD database and the VizieR catalogue access tool, operated at CDS, Strasbourg, France, and NASA’s Astrophysics Data System Service.
Paper: 2017ApJ...847...62L (acknowledgments)
This work was supported by the National Natural Science Foundation of China under grant Nos. 11473024, 11363005, 11763007, 11503008, and 11365022 and the XinJiang Science Fund for Distinguished Young Scholars under grant No. QN2016YX0049.
Paper: 2015MNRAS.454..550G (acknowledgments)
We thank Jie Wang and Liang Gao for helpful discussion. QG acknowledges support from the NSFC grant (No. 11133003), the Strategic Priority Research Program ‘The Emergence of Cosmological Structure’ of the Chinese Academy of Sciences (No. XDB09000000), the ‘Recruitment Program of Global Youth Experts’ of China, the NAOC grant (Y434011V01), MPG partner Group family and a Royal Society Newton International Fellowship, as well as the hospitality of the Institute for Computational Cosmology at Durham University. APC is supported by a COFUND/Durham Junior Research Fellowship under EU grant [267209] and thanks Liang Gao for support in the early stages of this work under a CAS International Research Fellowship and NSFC grant [11350110323]. CF acknowledges an ERC Advanced Investigator grant COSMIWAY (GA 267291). This work was supported in part by the Science and Technology Facilities Council Consolidated Grant for Durham Astronomy (grant number ST/I00162X/1). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1 and STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure. The COCO simulations were run at the University of Warsaw HPC centre and we would like to thank Maciej Cytowski and Arkadiusz Niegowski for their help with these simulations.
Paper: 2019MNRAS.484.2281S (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for the useful and constructive comments that improved the presentation of the results.This work is based on observations carried out at the Large Binocular Telescope (LBT) under program ID 2015_2016_28. The LBT is an international collaboration among institutions in the US, Italy and Germany. We acknowledge the support from the LBT-Italian Coordination Facility for the execution of the observations, the data distribution and for support in data reduction. We thank D. Thomas and J. Lian for having provided us with the median metallicity values of eBOSS galaxies from Comparat et al. ( 2017 ). PS would like to thank T. Durden for the useful suggestions.
Paper: 2019MNRAS.487.4809S (acknowledgments)
ACKNOWLEDGEMENTS The author AKS acknowledges IUCAA and IIA, India, for providing funds and telescope facilities for cometary observation.
Paper: 2018ApJ...859...53M (acknowledgments)
The authors thank the anonymous referee for the enlightening suggestions, which helped to improve the quality of this manuscript. This work is based on observations taken at ESO/VLT in Paranal, and we would like to thank the ESO staff for their assistance and support during the MUSE GTO campaigns. This work was supported by the Swiss National Science Foundation. We thank Amanda Bluck for proofreading the manuscript. We thank J. Woo and M. Maseda for their comments on the draft. S.C. gratefully acknowledges support from Swiss National Science Foundation grant PP00P2_163824. R.B. acknowledges support from the ERC advanced grant 339659-MUSICOS. J.R. acknowledges support from the ERC starting grant 336736-CALENDS. J.B. acknowledges support by Fundação para a Ciência e a Tecnologia (FCT) through national funds (UID/FIS/04434/2013) and Investigador FCT contract IF/01654/2014/CP1215/CT0003., and by FEDER through COMPETE2020 (POCI-01-0145-FEDER-007672). T.C. acknowledges support of the ANR FOGHAR (ANR-13-BS05-0010-02), the OCEVU Labex (ANR-11-LABX-0060), and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the “Investissements davenir” French government program managed by the ANR. J.S. and S.M. acknowledge support from European Research Council (ERC), grant agreement 278594-GasAroundGalaxies. J.S. acknowledges support from the Netherlands Organisation for Scientific Research (NWO) VICI grant 639.043.409. This research made use of Astropy, a community-developed core Python package for astronomy (Astropy Collaboration et al. 2013 ), NumPy and SciPy (Oliphant 2007 ), Matplotlib (Hunter 2007 ), IPython (Perez Granger 2007 ), and of NASA’s Astrophysics Data System Bibliographic Services.
Paper: 2018ApJ...859..157G (acknowledgments)
This research was supported by NNSFC grants 41674146, 41731070, and 41574159, in part by the Specialized Research Fund for State Key Laboratories of China and NSSC research fund for key development directions, and by the Strategic Pioneer Program on Space Science of CAS grant XDA15052500, and by NASA grants NNX13AF99G, QYZDJ-SSW-JSC028 and NNX17AB85G.
Paper: 2017A&A...606A...8D (acknowledgments)
We acknowledge the anonymous referee for her/his helpful comments and suggestions that improved the presentation of this paper. This project was partially financed by CONICET of Argentina under projects PIP 00356, and PIP00107, and from UNLP, 2012-2014 PPID/G002 and 11/G120. L.B. acknowledges support by CONICYT project PFB-06. Support for J.B. is provided by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. M.A.K. was supported by a Chilean FONDECYT fellowship grant (No. 3150319) from the Comisión Nacional de Investigación Científica y Tecnológica (CONICYT) and the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics.
Paper: 2019MNRAS.483.4060L (acknowledgments)
ACKNOWLEDGEMENTS This work is supported in part by the NSF grant AST-1715246 and NASA grant NNX14AP31G. BL is also supported in part by grants from NSFC (No. 11703068 and No. 11661161012). This work made use of the High Performance Computing Resource in the Core Facility for Advanced Research Computing at Shanghai Astronomical Observatory.
Paper: 2017ApJ...844...44J (acknowledgments)
We would like to thank the referee for her/his useful comments. We also thank the SMA staff for their support, which makes these studies possible. 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. We thank Mauricio Tapia for thoughtful discussions about the origin of the infrared emission in NGC 6334 V. We thank Marco Padovani for his valuable support with ARTIST and Gilberto Zavala Pérez and Alfonso H. Ginori González for their computational support. C.J. acknowledges support from MINECO (Spain) grant No. BES-2012-052481. C.J. and J.M.G. acknowledge support from MICINN (Spain) grant No. AYA2014-57369-C3. J.M.G. also acknowledges the support from the MECD (Spain) PRX15/00435 travel grant. A.P. and M.Z.-A. acknowledge financial support from the UNAM-DGAPA-PAPIIT IA 102815 grant (Mexico). M.Z.-A. also acknowledges CONACyT for a postdoctoral fellowship at the University of Michigan. P.M.K. acknowledges support from the Ministry of Science and Technology in Taiwan through grant MoST 103-2119-M-001-009 and an Academia Sinica Career Development Award. J.B.-P. acknowledges UNAM-PAPIIT grant No. IN110816 and UNAM’s DGAPA-PASPA Sabbatical program. He also is indebted to the Alexander von Humboldt Stiftung for its invaluable support. K.Q. acknowledges the support from National Natural Science Foundation of China (NSFC) through grants NSFC 11473011 and NSFC 11590781.
Paper: 2016MNRAS.459.2806A (acknowledgments)
The authors would like to thank Charles Danforth and John Stocke for very helpful discussions and for assistance with reducing and co-adding COS data and the anonymous referee for thoughtful reports which helped to improve this work. Based on observations made with the NASA/ESA HST , 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). STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555.
Paper: 2019MNRAS.482..639F (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for their work which much improved the paper. We also thank Stephen Kane for his useful feedback and advice. This work was funded in part by the Natural Sciences and Engineering Research Council of Canada Discovery Grants program.
Paper: 2016MNRAS.457..875P (acknowledgments)
An anonymous referee is gratefully acknowledged for the suggestions/comments which improved the paper. MP and PKP gratefully acknowledge support by the CSIR, New Delhi under the NET fellowship programme. This research has made use of (i) NASA's Astrophysics Data System, (ii) the SIMBAD data base, operated at CDS, Strasbourg, France, (iii) observations obtained with XMM–Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA, and (iv) data, software and/or web tools obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), a service of the Astrophysics Science Division at NASA/GSFC and of the Smithsonian Astrophysical Observatory's High Energy Astrophysics Division.
Paper: 2019MNRAS.485.1454P (acknowledgments)
ACKNOWLEDGEMENTS This work has made use of light curves provided by the University of California, San Diego Center for Astrophysics and Space Sciences, X-ray Group (R.E. Rothschild, A.G. Markowitz, E.S. Rivers, and B.A. McKim), obtained at http://cass.ucsd.edu/rxteagn/ .
Paper: 2015ApJ...809...74F (acknowledgments)
This paper is based in part on data collected at Subaru Telescope, which is operated by the National Astronomical Observatory of Japan. A.F. thanks Oscar A. Gonzalez for kindly providing VVV data. A.F. was supported by the Astrobiology Project of the Center for Novel Science Initiatives (CNSI), National Institutes of Natural Sciences (NINS; Grant Number AB261005). T.S. acknowledges the financial support from the JSPS, JSPS23103002, JSPS24253004, and JSPS26247023. The MOA project is supported by grants JSPS25103508 and 23340064. NJR is a Royal Society of New Zealand Rutherford Discovery Fellow. Work by C.H. was supported by Creative Research Initiative Program (2009-0081561) of National Research Foundation of Korea. S.D. is supported by “the Strategic Priority Research Program—The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (grant No. 09000000). The OGLE project has received funding from the National Science Centre, Poland, grant MAESTRO 2014/14/A/ST9/00121 to A.U. C.S. received funding from the European Union Seventh Framework Programme (FP7/2007–2013) under grant agreement No. 268421. K.A., D.M.B., M.D., K.H., M.H., C.L., C.S., R.A.S., and Y.T. would like to thank the Qatar Foundation for support from QNRF grant NPRP-09-476-1-078. Facilities : Subaru (IRCS) , FTN , FTS , Liverpool:2m , LCOGT .
Paper: 2019A&A...622A.179B (acknowledgments)
Acknowledgements The authors thank an anonymous referee for interesting comments and suggestions. We acknowledge financial support from the Spanish Ministry of Economy and Competitiveness through grants AYA2012-30789, AYA2015-66211-C2-1-P and AYA2015-66211-C2-2. CJB, ACS and PC thank CNPq for partially financing this work. LSJ acknowledges support from FAPESP (0800) and CNPq. We acknowledge the OAJ Data Processing and Archiving Unit (UPAD) for reducing and calibrating the OAJ data used in this work. Based on observations made with the JAST/T80 telescope at the Observatorio Astrofísico de Javalambre, in Teruel, owned, managed and operated by the Centro de Estudios de Física del Cosmos de Aragón. We acknowledge the OAJ Data Processing and Archiving Unit (UPAD) for reducing and calibrating the OAJ data used in this work. Funding for the J-PLUS Project has been provided by the Governments of Spain and Aragón through the Fondo de Inversiones de Teruel, the Aragón Government through the Reseach Groups E96 and E103, the Spanish Ministry of Economy and Competitiveness (MINECO; under grants AYA2015-66211-C2-1-P, AYA2015-66211-C2-2, AYA2012-30789 and ICTS-2009-14), and European FEDER funding (FCDD10-4E-867, FCDD13-4E-2685). RAD acknowledges support from CNPq through BP grant 312307/2015-2, CSIC through grant COOPB20263, FINEP grants REF. 1217/13 – 01.13.0279.00 and REF 0859/10 – 01.10.0663.00 for partial hardware support for the J-PLUS project through the National Observatory of Brazil.
Paper: 2016ApJ...827...26B (acknowledgments)
The research of B.B. is supported by the NASA Einstein Postdoctoral Fellowship.
Paper: 2015MNRAS.452.3475B (acknowledgments)
This research has made use of the following data and software packages: observations made by the Chandra X-ray Observatory, data obtained from the Chandra Data Archive, software provided by the Chandra X-ray Center (CXC) in the application package ciao , and software provided by the High Energy Astrophysics Science Archive Research Center in the heasoft package. We acknowledge extensive use of the ADS and arXiv. AB thanks G.R. Sivakoff and T.J. Maccarone for helpful discussions. COH acknowledges financial support from NSERC Discovery Grants, an Alberta Ingenuity New Faculty Award, and an Alexander von Humboldt Fellowship. ND acknowledges support via an EU Marie Curie Intra-European fellowship under contract no. FP-PEOPLE-2013-IEF-627148. LC acknowledges support from a Chandra grant associated with Obs.ID 15761. WCGH acknowledges support from STFC in the UK. This work was partially supported by the NSF through grant AST-1308124.
Paper: 2019MNRAS.490.2880S (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank the reviewer for the careful and thorough reading of this manuscript and for the thoughtful comments and constructive suggestions that help to improve the quality of this manuscript.
Paper: 2016ApJ...817..182W (acknowledgments)
We thank Kate Scholberg, André Rubbia, Masayuki Nakahata, and Lutz Köpke for useful conversations. We also thank Gabriel Martinez-Pinedo for providing us with tables for the 40 Ar cross sections. The authors acknowledge support provided by the NSF PetaApps program, under award OCI-0905046 via subaward no. 44592 from Louisiana State University to Princeton University, and by the Max-Planck/Princeton Center (MPPC) for Plasma Physics (NSF PHY-1144374). The authors employed computational resources provided by the TIGRESS high-performance computer center at Princeton University, which is jointly supported by the Princeton Institute for Computational Science and Engineering (PICSciE) and the Princeton University Office of Information Technology and by the National Energy Research Scientific Computing Center (NERSC), which is supported by the Office of Science of the US Department of Energy under contract DE-AC03-76SF00098. This work is part of the “Three Dimensional Modeling of Core-Collapse Supernovae” PRAC allocation support by the National Science Foundation (award number ACI-1440032). In addition, this research is part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (awards OCI-0725070 and ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications.
Paper: 2019MNRAS.486.2032B (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the A*MIDEX project (no. ANR-11-IDEX-0001-02) funded by the ‘Investissements d’Avenir’ French Government programme, managed by the French National Research Agency (ANR). This work is also supported OPTICON H2020 WP10. NAB acknowledges UKRI STFC funding (ST/P000541/1).
Paper: 2019A&A...625A.134R (acknowledgments)
Acknowledgement SPIRE has been developed by a consortium of institutes led by Cardiff University (UK) and including University of Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, University of Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, University of Sussex (UK); and Caltech, JPL, NHSC, University of 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). PACS has been developed by a consortium of institutes led by MPE (Germany) and including UVIE (Austria); KU Leuven, CSL, IMEC (Belgium); CEA, LAM (France); MPIA (Germany); INAF-IFSI/OAA/OAP/OAT, LENS, SISSA (Italy); IAC (Spain). This development has been supported by the funding agencies BMVIT (Austria), ESA-PRODEX (Belgium), CEA/CNES (France), DLR (Germany), ASI/INAF (Italy), and CICYT/MCYT (Spain). This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. K.L.J.R. acknowledges financial support by the Italian Ministero dell’Istruzione Università e Ricerca through the grant Progetti Premiali 2012-iALMA (CUP C52I13000140001). N.S. and S.B. acknowledge support by the french ANR and the german DFG through the project “GENESIS” (ANR-16-CE92-0035-01/DFG1591/2-1). GLW gratefully acknowledges support from The Leverhulme Trust. We acknowledge financial support from “Programme National de Physique Stellaire” (PNPS) and programme “Physique et Chime du Milieu Interstellaire” (PCMI) of CNRS/INSU, France. A.Z. thanks the support of the Institut Universitaire de France.
Paper: 2019MNRAS.486.4252M (acknowledgments)
ACKNOWLEDGEMENTS The authors acknowledge support from the PRIN-MIUR project Multi-scale Simulations of High-Energy Astrophysical Plasmas (Prot. 2015L5EE2Y). We would also grateful to the referee for his/her constructive comments which helped to improve the quality of this manuscript. We wish to thank L. Pareschi for valuable comments on the development of the Riemann solver in the context of IMEX schemes.
Paper: 2016MNRAS.457..695P (acknowledgments)
The authors thank the anonymous referee for important suggestions and comments that led to an improvement in the presentation of the paper. IP acknowledges the support from the Leibniz-DAAD research fellowship. NIL is supported by the DFG. ET is supported by the grants IUT26-2, IUT40-2 of the Estonian Ministry of Education and Research. JGS acknowledges support from the Alexander von Humboldt foundation.
Paper: 2017A&A...597A..64D (acknowledgments)
This research was supported by the FFG ASAP-12 project JetPro* (FFG-854025) and in part by the EU FP7-2011 project under Grant Agreement No. 284405.
Paper: 2017MNRAS.467.2061E (acknowledgments)
Acknowledgments It is a pleasure to thank Martin Sparre for providing data for the figures. We thank the anonymous referee for suggestions that improved this paper. We thank Gary Mamon for constructive comments. This project is partially funded by the Danish Council for Independent Research, under the project Fundamentals of Dark Matter Structures, DFF - 6108-00470.
Paper: 2015MNRAS.452.3010Z (acknowledgments)
The research presented in this paper was financed by the European Research Council (ERC) under the European Union's Seventh Framework Programme (FP7/2007-2013) with the research project STiMulUs , ERC Grant agreement no. 278267. The authors are also very grateful for the subsequent financial support of the present research, already granted by the European Commission under the H2020-FETHPC-2014 programme with the research project ExaHyPE , grant agreement no. 671698. We are grateful to Bruno Giacomazzo and Luciano Rezzolla for providing the numerical code for the exact solution of the Riemann problem in RMHD. We would also like to acknowledge PRACE for awarding access to the SuperMUC supercomputer based in Munich, Germany at the Leibniz Rechenzentrum (LRZ), and ISCRA, for awarding access to the FERMI supercomputer based in Casalecchio (Italy).
Paper: 2018MNRAS.477.3257A (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee who reviewed the previous version carefully and help us to strengthen the results in this version. This work was partially supported by Consejo Nacional de Ciencia y Tecnología México under grants CB-2011 No. 166212, CB-2014-01 No. 240512, Project No. 269652, and Fronteras Project 281; Xiuhcoatl and Abacus clusters at Centro de Investigación y de Estudios Avanzados, Instituto Politécnico Nacional; I0101/131/07 C-234/07 of the Instituto Avanzado de Cosmología (IAC) collaboration ( http://www.iac.edu.mx ). AAA and LEP acknowledge financial support from CONACyT fellowships.