adsabs/WIESP2022-NER huggingface dataset:
Paper: 2020A&A...634A..98G (acknowledgments)
We thank the referee for constructive comments that helped us to improve the manuscript. This research has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No. 682903, P.I. H. Bouy), and from the French State in the framework of the “Investments for the future” Program, IdEx Bordeaux, reference ANR-10-IDEX-03-02. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. 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. 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 publication makes use of VOSA, developed under the Spanish Virtual Observatory project supported by the Spanish MINECO through grant AyA2017-84089.
Paper: 2019MNRAS.489.2746U (acknowledgments)
ACKNOWLEDGEMENTS FUZ, MF, AGAJ, DRMC and CAA acknowledge funding through Fondecyt Regular No. 1180291 and BASAL Centro de Astrofisica y Tecnologias Afines (CATA) AFB-170002. MF acknowledges funding through the Concurso Proyectos Internacionales de Investigacion No. PII20150171 and Conicyt Quimal 170001. AGAJ acknowledges financial support from Carnegie Observatories through the Carnegie-Chile fellowship.
Paper: 2016MNRAS.461.2309R (acknowledgments)
This material is based upon work supported by the National Science Foundation under Grant No. AST 0507473.
Paper: 2018ApJ...857...87L (acknowledgments)
We thank the anonymous referee for carefully reading our manuscript and providing many thoughtful comments that greatly improved the quality of this paper. A.I. acknowledges support from the NSF grant No. AST-1535809. A.I., S.L., and H.L. acknowledge the support from Center for Space and Earth Sciences at LANL, and H.L. acknowledges the support from LANL/LDRD program. S.J. acknowledges support from the National Natural Science Foundation of China (grant No. 11503092). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00601.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan) and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Facility: ALMA . Software: LA-COMPASS (Li et al. 2005 , 2009 ; Fu et al. 2014 ), RADMC-3D (Dullemond 2012 ), radmc3dPy ( http://www.ast.cam.ac.uk/juhasz/radmc3dPyDoc/index.html ).
Paper: 2018MNRAS.478.3494C (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for useful comments. We also thank A. Ballone, S. Gillessen and G. Hajdu for very helpful discussions. This work was partially developed while JC was on sabbatical leave at MPE. DC and JC acknowledge the kind hospitality of MPE, and funding from the Max Planck Society through a ‘Partner Group’ grant. We acknowledge support from CONICYT-Chile through FONDECYT (1141175) and Basal (PFB0609) grants. DC is supported by CONICYT-PCHA/Doctorado Nacional (2015-21151574).
Paper: 2017MNRAS.464..680C (acknowledgments)
This research was supported by the Ministerio de Economía y Competitividad under project FIS2012-31079. We would like to thank the technical staff of the Calar Alto Observatory in Spain for all its help with the observations.
Paper: 2016A&A...588A.112G (acknowledgments)
This paper makes use of the following ALMA data: ADS/JAO.ALMA#2011.0.000010.SV. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. We are grateful to Antonio Garufi for many discussions and for sharing his infrared polarization images. We thank Sebastian Stammler for insightful discussions on the effect of the CO snowline on dust and for showing us the results of his simulations in advance of publication. We thank the anonymous referee for the helpful comments. Part of this research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration. The fits have been carried out on the computing facilities of the Computational Center for Particle and Astrophysics (C2PAP) as part of the approved project “Dust evolution in protoplanetary disks”. M.T. and L.T. are grateful for the experienced support by F. Beaujean (C2PAP). This work was partly supported by the Italian Ministero dell’Istruzione, Università e Ricerca through the grant Progetti Premiali 2012 – iALMA (CUP C52I13000140001).
Paper: 2016ApJ...832..194K (acknowledgments)
This work is supported by the Japan Society for the Promotion of Science KAKENHI grant numbers 16K17673 (S.K.), 26800100 (K.M.), 16K17667 (Y.S.). The work by K.M. is supported by the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan.
Paper: 2018A&A...614A..26A (acknowledgments)
Acknowledgements We thank the anonymous referee for a number of good suggestions helping to improve the presentation of this work. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00955.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAOand NAOJ. The group of JKJ acknowledges support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement No 646908) through ERC Consolidator Grant “S4F”. Research at the Centre for Star and Planet Formation is funded by the Danish National Research Foundation.
Paper: 2016MNRAS.459.2054D (acknowledgments)
We wish to thank Roelof de Jong and Ned Taylor for valuable discussions, and Dustin Lang for making the WISE magnitudes of Lang et al. ( 2014 ) available for testing before their publication. We also wish to thank the anonymous referee for their helpful suggestions on presenting some aspects of our results. This work was partially supported by NSF-AST 1514835. This research has made use of NASA's Astrophysics Data System Bibliographic Services. 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 publication makes use of data products from the Two Micron All Sky Survey, which is a joint project of the University of Massachusetts and the Infrared Processing and Analysis Center/California Institute of Technology, funded by the National Aeronautics and Space Administration and the National Science Foundation. 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: 2016ApJ...826....4H (acknowledgments)
V.A. acknowledges financial support from NASA/ Chandra grants GO3-14051X, AR4-15003X, NNX15AR30G, and NASA/ADAP grant NNX10AH47G. A.Z. acknowledges financial support from NASA/ADAP grant NNX12AN05G, and funding from the European Research Council under the European Union’s Seventh Framework Programme (FP/2007–2013)/ERC Grant Agreement no. 617001. J.D., P.P., and T.G. acknowledge financial support from NASA contract NAS8-03060. M.S. acknowledges support by the the Deutsche Forschungsgemeinschaft through the Heisenberg Programme (SA 2131/3-1). S.L. acknowledges financial support from NASA/ADAP grant NNX14-AF77G. The OGLE project has received funding from the National Science Centre, Poland, Grant MAESTRO 2014/14/A/ST9/00121 to AU. We thank the anonymous referee for helpful comments and suggestions.
Paper: 2015MNRAS.450.3331M (acknowledgments)
The work of JHM and CK is supported by the Science and Technology Facilities Council (STFC), via studentships and a consolidated grant, respectively. The work of NSH is supported by NASA under Astrophysics Theory Program grants NNX11AI96G and NNX14AK44G. We would like to thank the anonymous referee for a helpful and constructive report, and we are grateful to A. F. Palah and B. T. Gaensicke for the IX Vel XSHOOTER data set. We would also like to thank J. V. Hernandez Santisteban, S. W. Mangham and I. Hubeny for useful discussions. We acknowledge the use of the IRIDIS High Performance Computing Facility, and associated support services at the University of Southampton, in the completion of this work.
Paper: 2018MNRAS.473..241H (acknowledgments)
Acknowledgements The anonymous referee of our paper offered many helpful suggestions for improvement, and we thank him/her for performing such a careful review. We also thank Paolo Ventura and Sergio Cristallo for providing answers to our enquiries regarding the details of the ATON (Ventura) and FRUITY (Cristallo) model predictions and in some cases sending us additional output. We also appreciate the help provided by Gloria Delgado-Inglada concerning her group's recently updated ICFs. Portions of the UV data employed in our project came from HST programme number GO12600. BGS is grateful for summer support by the US National Science Foundation (NSF) through the Research Experience for Undergraduates programme. MMBB was supported by ANPCyT through grant PICT-2014-2708 and by a Return Fellowship from the Alexander von Humboldt Foundation. Finally, RBCH, BGS, KBK, and BB are grateful to their home institutions for travel support.
Paper: 2018MNRAS.478..733L (acknowledgments)
ACKNOWLEDGEMENTS The authors thank the anonymous referee, Iain A. Steele, Phil James, Dan Hoak, David Bersier, and Hendrik van Eerten for useful comments. This research was supported by Science Technology and Facilities Council grants. GPL was partially supported by International Astronomical Union and Royal Astronomical Society grants.
Paper: 2017MNRAS.468.1917R (acknowledgments)
Acknowledgments We dedicate this paper to our colleague Y.Y. Zhang: we are indebted to her work (Zhang etal. 2011 ) for the analysis discussed in Paper I , on which this paper is based. We thank H. Ebeling for useful information about the ME-MACS sample and T. Reiprich for providing the concentration parameters of HIFLUGCS clusters.
Paper: 2019A&A...621A..35L (acknowledgments)
The current work benefited from discussions with visiting researchers at the institute for Solar Physics in Stockholm. The authors specially wish to thank Carlos Díaz Baso, Andrés Asensio Ramos, Marian Martínez Gonzalez, Lindsey Fletcher and Paulo Simões for useful advice on the presented work. We also wish to thank the anonymous referee for valuable comments which improved the content of the paper. We made use of routines by Rob Rutten to align SDO data with SST data. The observers thank Pit Sutterlin for support during the observing campaign at the SST. TL acknowledges financial support from the C HROMOBS project funded by the Knut and Alice Wallenberg Foundation. JdlCR is supported by grants from the Swedish Research Council (2015-03994) and the Swedish National Space Board (128/15) and has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (SUNMAG, grant agreement 759548). JdlCR and SD are also supported by the Swedish Civil Contingencies Agency (MSB). The inversions were performed on resources provided by the Swedish National Infrastructure for Computing (SNIC) at the High Performance Computing Center North at Umeå University. The Swedish 1 m Solar Telescope is operated on the island of La Palma by the Institute for Solar Physics of Stockholm University in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. This research has made use of NASA’s Astrophysics Data System Bibliographic Services.
Paper: 2017MNRAS.466.1857G (acknowledgments)
Based on observations obtained at the Gemini Observatory (processed using the Gemini iraf package), 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 National Research Council (Canada), CONICYT (Chile), Ministerio de Ciencia, Tecnologa e Innovacin Productiva (Argentina), and Ministrio da Cincia, Tecnologia e Inovao (Brazil), and observations collected at the Centro Astronmico Hispano Alemn (CAHA), operated jointly by the Max-Planck Institut fr Astronomie and the Instituto de Astrofisica de Andalucia (CSIC). VVG acknowledges the Russian Science Foundation grant 14-12-01096. JM acknowledges funding from a Royal Society Science Foundation Ireland University Research Fellowship (No. 14/RS-URF/3219). AYK acknowledges support from the National Research Foundation (NRF) of South Africa and the Russian Foundation for Basic Research grant 16-02-00148. TJH is funded by an Imperial College Junior Research Fellowship. This research was supported by the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., on behalf of the international Gemini partnership of Argentina, Brazil, Canada, Chile, and the United States of America, and 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 the National Aeronautics and Space Administration, the SIMBAD data base and the VizieR catalogue access tool, both operated at CDS, Strasbourg, France.
Paper: 2017A&A...606A..69A (acknowledgments)
We thank Willy Benz for insightful discussions. This work was supported in part by the European Research Council under grant 239605. This work has been carried out within the framework of the NCCR PlanetS supported by the Swiss National Science Foundation. The author acknowledges the financial support of the SNSF.
Paper: 2017A&A...598L...7K (acknowledgments)
We are grateful to Dr J. S. Jenkins for discussions that led to important improvements of this Letter. C.L. acknowledges the financial support of the Swiss National Science Foundation (SNSF). This research made use of Astropy 2 (Astropy Collaboration 2013) , and of the SIMBAD (Wenger et al. 2000) , VIZIER (CDS, Strasbourg, France) and NASA’s Astrophysics Data System databases.
Paper: 2016MNRAS.462..532M (acknowledgments)
This work was supported by Australian Research Council grants ( DP0662810, DP1096533 ). The Mopra Telescope is part of the Australia Telescope and is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. The University of New South Wales Mopra Spectrometer Digital Filter Bank used for these Mopra observations was provided with support from the Australian Research Council, together with the University of New South Wales, University of Sydney, Monash University and the CSIRO. We would like to thank the anonymous referee whose comments served to increase the quality of our manuscript and maximize the exploitation of our data.
Paper: 2017ApJ...839...60H (acknowledgments)
We would like to thank the anonymous referee for their detailed and helpful comments which improved the quality of this work.
Paper: 2016ApJ...829..100Y (acknowledgments)
This work was supported by the National Research Foundation of Korea (NRF-2012 R1A2A1A 03670387). Facilities: Big Bear Solar Observatory
Paper: 2018MNRAS.474.5560I (acknowledgments)
Acknowledgements This work is supported by the European Community through the grant LENA (ERC StG no. 678282) within the H2020 Framework Program.
Paper: 2019MNRAS.482.5597A (acknowledgments)
ACKNOWLEDGEMENTS I thank R. Srianand and Neeraj Gupta for their invaluable comments and inputs, that helped in improving the paper significantly. I also thank the staff of the 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 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. Further, I acknowledge support from the Indo-French Centre for the Promotion of Advanced Research under Project 5504-B (PIs: N. Gupta, P. Noterdaeme). I thank the anonymous referee for a very helpful report that significantly improved the quality of the paper.
Paper: 2019MNRAS.485.3930D (acknowledgments)
ACKNOWLEDGEMENTS Based on observations obtained with SITELLE, a joint project of Université Laval, ABB, Université de Montréal, and the Canada–France–Hawaii Telescope (CFHT), which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. The authors wish to recognize and acknowledge the very significant cultural role that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most grateful to have the opportunity to conduct observations from this mountain. We thank the referee for a very thorough and constructive report, leading to significant improvements on this paper. LD, CR, GJ, and ST are grateful to the Natural Sciences and Engineering Research Council of Canada, the Fonds de Recherche du Québec, and the Canada Foundation for Innovation for funding. LD and CR are very grateful to the Department of Physics and Astronomy, University of Hawaii Hilo, as well as the CFHT, for having provided them with an ideal and very enjoyable working environment during their sabbatical stay on the Big Island.
Paper: 2019MNRAS.487.3702O (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for a constructive report which improved the manuscript. We are grateful to Richard Booth, Cathie Clarke, Ruth Murray-Clay, and Giovanni Rosotti for interesting discussions. JEO is supported by a Royal Society University Research Fellowship.
Paper: 2018MNRAS.481.5331A (acknowledgments)
ACKNOWLEDGEMENTS We thank Daniele Viganò for useful comments. This work is supported in part by the Spanish MINECO/FEDER grants AYA2015-66899-C2-1-P, AYA2015-66899-C2-2-P, the grant of Generalitat Valenciana PROMETEOII-2014-069, and by the PHAROS COST action CA16214. PC acknowledges the support from the Ramón y Cajal program of the Spanish MINECO (RYC-2015-19074).
Paper: 2018ApJ...869..106M (acknowledgments)
This material is based upon work supported by the National Science Foundation under grant AST-1614018 to C.W.M. and grants AST-1515876 and AST-1814440 to C.S.K. COSMOGRAIL is made possible thanks to the continuous work of all observers and technical staff obtaining the monitoring observations, in particular, at the Swiss Leonhard Euler telescope at La Silla Observatory, which is supported by the Swiss National Science Foundation. V.B. and F.C. are also supported by the Swiss National Science Foundation (SNSF). This work is partly based on observations obtained with the Small and Moderate Aperture Research Telescope System (SMARTS) 1.3 m, which is operated by the SMARTS Consortium. Thanks are due to V. Motta for helpful discussions about black hole masses and to R. Witt for many hours of help with the USNA High Performance Computing Cluster.
Paper: 2020A&A...634A.139W (acknowledgments)
Acknowledgements The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Y.W., H.B., S.B., and J.D.S. acknowledge support from the European Research Council under the Horizon 2020 Framework Program via the ERC Consolidator Grant CSF-648505, and R.S.K. via the ERC AdvancedGrant 339177 (STARLIGHT). H.B., S.C.O.G., and M.R. acknowledge support from the Deutsche Forschungsgemeinschaft in the Collaborative Research Center (SFB 881) “The Milky Way System” (subproject B1, B2, B8). R.S.K. and S.C.O.G. also acknowledge support from the DFG via Germany’s Excellence Strategy EXC-2181/1 - 390900948 (the Heidelberg STRUCTURES Cluster of Excellence). This work was carried out in part at the Jet Propulsion Laboratory which is operated for NASA by the California Institute of Technology. N.S. acknowledges support by the french ANR and the german DFG through the project “GENESIS” (ANR-16-CE92-0035-01/DFG1591/2-1). F.B. acknowledges funding from the European Union’s Horizon 2020 research and innovation program (grant agreement No 726384). This research made use of Astropy and affiliated packages, a community-developed core Python package for Astronomy ( Astropy Collaboration 2018 ), Python package SciPy 3 , APLpy, an open-source plotting package for Python ( Robitaille Bressert 2012 ), and software TOPCAT ( Taylor 2005 ). The authors thank the anonymous referee for the constructive comments that improve the paper.
Paper: 2015ApJ...798...22L (acknowledgments)
We thank Sera Markoff, Heino Falcke, and Geoffrey Bower for constructive discussions and the anonymous referee for useful comments. This work was supported in part by the Natural Science Foundation of China (grants 11103061, 11133005, 11121062, and 11103059), the National Basic Research Program of China (973 Program, grant 2014CB845800), and the Strategic Priority Research Program “The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (grant XDB09000000).
Paper: 2015A&A...578A.118L (acknowledgments)
We thank Marta Volonteri and Stefano Bovino for interesting discussions and helpful suggestions. The research leading to these results has received funding from the European Research Council under the European Community’s Seventh Framework Programme (FP7/20072013 Grant Agreement no. 614199, project “BLACK”). DRGS is indebted to the Scuola Normale Superiore (SNS) in Pisa for an invitation as a “Distinguished Scientist”, which has stimulated the research described in this manuscript.