adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019MNRAS.490.1518O (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank Fabrizio Arrigoni Battaia for insightfull discussions related to this manuscript. This research was carried out on the High Performance Computing resources at New York University Abu Dhabi; on the theo cluster of the Max-Planck-Institut für Astronomie and on the hydra clusters at the Rechenzentrum in Garching. We greatly appreciate the contributions of these computing allocations. All figures in this work have been made with matplotlib (Hunter 2007 ), using the open-source python libraries: pynbody (Pontzen et al. 2013 ), numpy (Walt, Colbert Varoquaux 2011 ), and scipy (Eric Jones et al. 2001 ). AO and BM are funded by the Deutsche Forschungsgemeinschaft (DFG, German Research Foundation) – MO 2979/1-1. TB acknowledges support from by the European Research Council under ERC- CoG grant CRAGSMAN-646955. RK acknowledges support from NASA through Einstein Postdoctoral Fellowship grant number PF7-180163 awarded by the Chandra X-ray Center, which is operated by the Smithsonian Astrophysical Observatory for NASA under contract NAS8-03060.
Paper: 2019ApJ...870...70S (acknowledgments)
We would like to thank the anonymous referee for the many constructive remarks and suggestions that greatly helped us to improve the content and layout of the paper. MS thanks Giulia Despali, Chiara Mancini, and Alessia Moretti for helpful discussions and hints. CC would like to thank Rosaria Tantalo and Emanuela Chiosi for valuable collaboration and the Department of Physics and Astronomy of the Padua University for the friendly hospitality and computational support. The tool HMFcalc and the public data from the ILLUSTRIS project have been amply used in this study.
Paper: 2019MNRAS.484.1800S (acknowledgments)
ACKNOWLEDGEMENTS Our results are based on observations with the 2.2-m telescope of the University of Hawaii and we thank Colin Aspin and Mark Willman for their interest and support. Special thanks go to László Szabados for a careful reading of the manuscript and for the suggestions to improve it. We would like to thank Péter Ábrahám for the 13 CO data. This work makes use of observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This research has made use of the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with NASA. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in Ochsenbein, Bauer Marcout ( 2000 ). 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 thank the anonymous referee for helpful suggestions.
Paper: 2019ApJ...883..145J (acknowledgments)
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2015.1.01520.S. ALMA is a partnership of the ESO (representing its member states), NSF (USA), and NINS (Japan), together with the NRC (Canada), MOST and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by the ESO, AUI/NRAO, and NAOJ. This research has made use of the HyperLeda database ( http://leda.univ-lyon1.fr ). We thank Jonathan Braine, the referee of the paper, for helpful comments that improved the quality of this paper substantially. P.J. acknowledges support through project LM2015067 of the Ministry of Education, Youth and Sports of the Czech Republic. P.J. and J.P. acknowledge support from the project 19-18647S of the Czech Science Foundation and from the institutional research project RVO:67985815. M.S. acknowledges support from NASA grants GO6-17111X and 80NSSC18K0606 and NSF grant 1714764. L.C. is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. T.S. acknowledges support through fellowship SFRH/BPD/103385/2014 funded by FCT (Portugal) and POPH/FSE (EC). This work was supported by Fundação para a Ciência e a Tecnologia (FCT) through national funds (UID/FIS/04434/2013) and by FEDER through COMPETE2020 (POCI-01-0145-FEDER-007672). T.S. also acknowledges support from DL 57/2016/CP1364/CT0009. This work was supported by FCT/MCTES through national funds (PIDDAC) by grant PTDC/FIS-AST/29245/2017. E.B. acknowledges support from the UK Science and Technology Facilities Council (grant No. ST/M001008/1). M.F. acknowledges support by the Science and Technology Facilities Council (grant No. ST/P000541/1). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 757535). Facility: ALMA. Software: CASA (McMullin et al. 2007 ), GILDAS (Guilloteau Lucas 2000 ), astropy (Astropy Collaboration et al. 2013 ).
Paper: 2016ApJ...818..118C (acknowledgments)
The research activities of the Observational Astronomy Stellar Board at the Federal University of Rio Grande do Norte are supported by continuous grants from the Brazilian agencies CNPq and FAPERN and by the INCT-INEspaço. C.C. acknowledges a PDJ/CAPES fellowship (Process n °88887.114342/2015-00). B.B. acknowledges the support of the NASA Einstein Postdoctoral Fellowship. A.L. acknowledges the support from the Center for Magnetic Self-Organization, a distinguished visitor PVE/CAPES appointment at the Physics Graduate Program at UFRN, Natal, Brazil and thanks the DFTE/UFRN for hospitality.
Paper: 2019ApJ...883...15G (acknowledgments)
R.G. and J. G. are supported by the Israeli Science Foundation under grant No. 719/14. F.D.C. acknowledges support from the UNAM-PAPIIT grant IN117917. We acknowledge the support from the Miztli-UNAM supercomputer (project LANCAD-UNAM-DGTIC-281) in which the simulations were performed.
Paper: 2015A&A...580A.102C (acknowledgments)
We thank the anonymous referee for comments and suggestions that improved the paper. We acknowledge financial support from INAF under the contracts PRIN-INAF-2011 (“Black Hole growth and AGN feedback through cosmic time”) and PRIN MIUR 2010-2011 (“The dark Universe and the cosmic evolution of baryons”). M.B. acknowledges support from the FP7 Career Integration Grant “eEASy” (CIG 321913). C.F. gratefully acknowledges financial support from PRIN MIUR 2010-2011, project “The Chemical and Dynamical Evolution of the Milky Way and Local Group Galaxies”, prot. 2010LY5N2T. E.P. acknowledges financial support from INAF under the contract PRIN-INAF-2012. Funding for this work has also been provided by the Israel Science Foundation grant 284/13.
Paper: 2015MNRAS.453..721V (acknowledgments)
We thank the anonymous referee for insightful comments that helped improve the manuscript. MV and MC thank Henk Hoekstra and Rachel Mandelbaum for useful and stimulating discussions. MC acknowledges support from NWO VIDI grant number 639.042.814 and ERC FP7 grant 278594. 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. We also gratefully acknowledge PRACE for awarding us access to the resource Curie based in France at Très Grand Centre de Calcul. This work was sponsored by the Dutch National Computing Facilities Foundation (NCF) for the use of supercomputer facilities, with financial support from the Netherlands Organization for Scientific Research (NWO). The research was supported in part by the European Research Council under the European Union's Seventh Framework Programme (FP7/2007-2013) / ERC Grant agreements 278594-GasAroundGalaxies, GA 267291 Cosmiway, and 321334 dustygal, the UK Science and Technology Facilities Council (grant numbers ST/F001166/1 and ST/I000976/1), Rolling and Consolodating Grants to the ICC, Marie Curie Reintegration Grant PERG06-GA-2009-256573. TT acknowledges the Interuniversity Attraction Poles Programme initiated by the Belgian Science Policy Office ([AP P7/08 CHARM]).
Paper: 2017ApJ...851..104H (acknowledgments)
We would like to thank Eric Herbst and Ilsa Cooke for their helpful suggestions and Xixin Liang for technical assistance. We are grateful to an anonymous referee for the constructive comments that helped to improve the paper. This work was supported by NSF Astronomy and Astrophysics Research Grants No. 1311958 and No. 1615897.
Paper: 2017A&A...601A..81C (acknowledgments)
F.M. gratefully acknowledges the financial support of the Programma Giovani Ricercatori – Rita Levi Montalcini – Rientro dei Cervelli (2012) awarded by the Italian Ministry of Education, Universities and Research (MIUR). Part of this work is based on the NVSS (NRAO VLA Sky Survey): The National Radio Astronomy Observatory is operated by Associated Universities, Inc., under contract with 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. This research made use of the NASA/IPAC Infrared Science Archive and Extragalactic Database (NED), which are operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. We acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ). Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III website is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration, including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, University of Cambridge, 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: 2020ApJ...889...54M (acknowledgments)
We thank the anonymous referee for a prompt and insightful report. G.M. and A.N. acknowledge the financial support from the National Science Centre, Poland through grant No. 2016/23/B/ST9/00579. A.N. is also supported by the National Science Centre, Poland through grant No. 2015/19/B/ST9/02937. E.V. acknowledges support from the Spanish Ministerio de Ciencia, Innovación y Universidades under the project PGC2018-101950-B-I00. M.K. is supported by the Polish National Science Center (NCN) through grant 2017/27/B/ST9/02727. Facility: TNG(HARPS-N).
Paper: 2017MNRAS.470.1960H (acknowledgments)
Acknowledgements This work is based upon observations carried out at the OAN SPM, Baja California, Mexico. GT and SZ acknowledge PAPIIT grants IN108316, IN100617 and CONACyT grant 166376. We are grateful to Dr J. V. Hernndez Santisteban for the opportunity to work with the original data of 1RXS J064434.5334451. We thank the daytime and night support staff at the OAN-SPM for facilitating and helping to obtain our observations.
Paper: 2019MNRAS.489.1379N (acknowledgments)
ACKNOWLEDGEMENTS The authors thank the reviewer for her/his valuable comments on the submitted manuscript. NN thanks T. Fischer for providing neutrino-driven wind trajectories used in this study. This work has been partially supported by the European Research Council (EU-FP7-ERC-2012-St Grant 306901, EU-FP7 Adv Grant GA321263-FISH), the EU COST Action CA16117 (ChETEC), the UK STFC (ST/M000958/1), and MEXT Japan (‘Priority Issue on Post-K computer: Elucidation of the Fundamental Laws and Evolution of the Universe’ and ‘the World Premier International Research Centre Initiative: WPI Initiative’). GC acknowledges financial support from the EU Horizon2020 programme under the Marie Skłodowska-Curie grant 664931. CF acknowledges support by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award No. DE-FG02-02ER41216. Parts of the computations were carried out on COSMOS (STFC DiRAC Facility) at DAMTP in University of Cambridge. This equipment was funded by BIS National E-infrastructure capital grant ST/J005673/1, STFC capital grant ST/H008586/1, and STFC DiRAC Operations grant ST/K00333X/1. DiRAC is part of the UK National E-Infrastructure. Further computations were carried out at CfCA, National Astronomical Observatory of Japan, and at YITP, Kyoto University. The University of Edinburgh is a charitable body, registered in Scotland, with Registration No. SC005336.
Paper: 2015ApJ...811...70R (acknowledgments)
This work is dedicated to our colleague and friend Tomas Dahlen, for whom this supernova has been named in memoriam. He is dearly missed. We thank the Hubble Frontier Fields team at STScI for their substantial efforts to make the HFF program successful. In particular, thanks are due to Matt Mountain for the allocation of discretionary orbits for the HFF program; to Jennifer Lotz, Norman Grogin, and Patricia Royle for accommodations in strategy and implementation to make the FrontierSN program possible; to Anton Koekemoer for HFF data processing support. We also thank the CLASH team, led by Marc Postman, for observations, catalogs, and high level science products that were of significant value for this analysis. Thanks to Jonatan Selsing for helpful comments on the manuscript. This work utilizes gravitational lensing models produced by modeling teams that were funded as part of the HST Frontier Fields program conducted by STScI. STScI is operated by the Association of Universities for Research in Astronomy, Inc. under NASA contract NAS 5-26555. The lens models were obtained from the Mikulski Archive for Space Telescopes (MAST). Financial support for this work was provided to S.A.R. by NASA through grants HST-HF-51312 and HST-GO-13386 from STScI, which is operated by Associated Universities for Research in Astronomy, Inc. (AURA), under NASA contract NAS 5-26555. A.M. acknowledge the financial support of the Brazilian funding agency FAPESP (Post-doc fellowship—process number 2014/11806-9). Support for this research at Rutgers University was provided in part by NSF CAREER award AST-0847157 to SWJ. The Dark Cosmology Centre is supported by the Danish National Research Foundation. J.M.D. acknowledges support of the consolider project CSD2010-00064 and AYA2012–39475-C02-01 funded by the Ministerio de Economia y Competitividad. J.M. contributed to this research from the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA and acknowledges support from NASA Grants HST-GO-13343.05-A and HST-GO-13386.13-A. The research leading to these results has received funding from the People Programme (Marie Curie Actions) of the European Union’s Seventh Framework Programme (FP7/20072013) under REA grant agreement number 627288. A.Z. acknowledges financial support from NASA through grant HST-HF-51334.01-A awarded by STScI and operated by AURA. T.T. acknowledges support by the Packard Foundation in the form of Packard Research Fellowship. GLASS is funded by NASA through HST grant GO-13459. L.L.R.W. acknowledges the support of the Minnesota Supercomputing Institute. Facility: HST (WFC3).
Paper: 2018MNRAS.478.4317H (acknowledgments)
ACKNOWLEDGEMENTS Erica Hammerstein thanks the National Science Foundation for support through a Research Experience for Undergraduates program at Wayne State University (National Science Foundation Grant No. PHY-1460853). We thank Manuel Torres for helpful comments that improved the paper. We thank the referee, and author of ELC, Jerry Orosz, for a helpful referee report and guidance in using the latest MCMC version of ELC. This paper includes data gathered with the 6.5-m Magellan Telescopes located at Las Campanas Observatory, Chile. This paper 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.
Paper: 2015A&A...582A..88W (acknowledgments)
The authors thank Drs. Alan Heays, Kenji Furuya, and Mihkel Kama for useful discussions and an anonymous referee for their insightful comments. C.W. acknowledges support from the European Union A-ERC grant 291141 CHEMPLAN and from the Netherlands Organisation for Scientific Research (NWO, program number 639.041.335). H.N. acknowledges the Grant-in-Aid for Scientific Research 23103005 and 25400229. She also acknowledges support from the Astrobiology Project of the CNSI, NINS (grant numbers AB261004, AB261008). A portion of the numerical calculations were carried out on SR16000 at YITP in Kyoto University.
Paper: 2019ApJ...885...17C (acknowledgments)
Positive criticism from an anonymous referee led to substantial improvements in the paper. This research was supported by NSERC of Canada. Computations were performed on the niagara supercomputer at the SciNet HPC Consortium. SciNet is funded by: the Canada Foundation for Innovation; the Government of Ontario; Ontario Research Fund—Research Excellence; and the University of Toronto.
Paper: 2019A&A...622A..57C (acknowledgments)
We wish to thank the anonymous referee for the useful comments which significantly improved the paper.
Paper: 2017A&A...602A...9C (acknowledgments)
T.-W. Chen thanks the organisers and participants of MIAPP workshop “Supernovae: The Outliers” for stimulating discussions: You-Hua Chu for interacting galaxy, Maryam Modjaz for metallicity and Ken’ichi Nomoto for CSM model. T.-W. Chen thanks Stefan Taubenberger for bolometric light curve comparison and participants in the Garching SN meeting for useful advise. T.W.C, T.K., R.Y. and P.W. acknowledge the support through the Sofia Kovalevskaja Award to P. Schady from the Alexander von Humboldt Foundation of Germany. S.J.S. acknowledges ERC grant 291222 and STFC grants ST/I001123/1 and ST/L000709/1. L.G. was supported in part by the US National Science Foundation under Grant AST-1311862. A.J. acknowledges funding by the European Union’s Framework Programme for Research and Innovation Horizon 2020 under Marie Sklodowska-Curie grant agreement No. 702538. M.S. acknowledges support from EU/FP7-ERC grant 615929. K.M. acknowledges support from the STFC through an Ernest Rutherford Fellowship. The Liverpool Telescope is operated on the island of La Palma by Liverpool John Moores University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias with financial support from the UK Science and Technology Facilities Council. Part of the funding for GROND (both hardware as well as personnel) was generously granted from the Leibniz-Prize to Prof. G. Hasinger (DFG grant HA 1850/28-1). We acknowlegde use of the Pan-STARRS1 photometric reference catalogue: the Pan-STARRS1 Surveys (PS1) have been made possible through contributions of 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, 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, 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 under Grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE) and the Los Alamos National Laboratory.
Paper: 2015A&A...583A..55O (acknowledgments)
We thank a number of unnamed colleagues for interesting discussions. G.Ö. is a Royal Swedish Academy of Science research fellow (supported by a grant from the Knut Alice Wallenbergs foundation). This work was supported by the Swedish Research Council and the Swedish National Space Board. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. This research has made use of NASA’s Astrophysics Data System.
Paper: 2016MNRAS.460.1790G (acknowledgments)
This work is supported by the National Natural Science Foundation of China under grant Nos 11203016 and 11143012. This work is partly supported by the Young Scholars Program of Shandong University, Weihai. We are also grateful for data taken and assembled by the WEBT collaboration and stored in the WEBT archive at the Osservatorio Astrofisico di Torino-INAF ( http://www.oato.inaf.it/blazars/webt/ ) and data from the Steward Observatory spectropolarimetric monitoring project supported by Fermi Guest Investigator grants NNX08AW56G, NNX09AU10G and NNX12AO93G, as well as data from the variable star observations from the AAVSO International Database contributed by observers worldwide.
Paper: 2016A&A...588A.148H (acknowledgments)
S.K. and P.M.W. received funding through BMBF Verbundforschung (project MUSE-AO, grant 05A14BAC and 05A14MGA). 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).
Paper: 2018A&A...610L..13D (acknowledgments)
Acknowledgments We thank the referee, James Reeves, for his helpful comments. 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 the USA (NASA). M.D. acknowledges financial under contract ASI – INAF grant I/037/12/0. G.P. acknowledges the Bundesministerium für Wirtschaft und Technologie/Deutsches Zentrum für Luft- und Raumfahrt (BMWI/DLR, FKZ 50 OR 1408) and the Max Planck Society. B.D.M. acknowledges support from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 665778 via the Polish National Science Center grant Polonez UMO-2016/21/P/ST9/04025.
Paper: 2019A&A...627A..14N (acknowledgments)
This research was supported by the Korea Astronomy and Space Science Institute under the RD program (Project No. 3348-20160002) supervised by the Ministry of Science, ICT and Future Planning. Support by the Deutsche Forschungsgemeinschaft (DFG), Grant No. Yo 194/1-1, is gratefully acknowledged. P.N. would like to thank Phillip Podsiadlowski and Stephan Geier for useful discussions.