adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019ApJ...885..117G (acknowledgments)
We acknowledge the anonymous referee for useful comments and suggestions, the use of the Fermi -LAT data provided by the Fermi Science Support Center, the SIMBAD database operated at CDS, Strasbourg, France and the data of Herschel provided by European-led Principal Investigator consortia and with important participation from NASA. This work is supported by National Key Program for Research and Development (2016YFA0400200), the National Natural Science Foundation of China (Nos. 11433009, 11525313, 11722328, 11703093), the Joint Research Fund in Astronomy under cooperative agreement between the National Natural Science Foundation of China and Chinese Academy of Sciences (grant No. U1738126), and the Natural Science Foundation for Young Scholars of Jiangsu Province, China (No. BK20191109).
Paper: 2017A&A...598A..39H (acknowledgments)
The support of the Namibian authorities and of the University of Namibia in facilitating the construction and operation of H.E.S.S. is gratefully acknowledged, as is the support by the German Ministry for Education and Research (BMBF), the Max Planck Society, the German Research Foundation (DFG), the French Ministry for Research, the CNRS-IN2P3 and the Astroparticle Interdisciplinary Programme of the CNRS, the UK Science and Technology Facilities Council (STFC), the IPNP of the Charles University, the Czech Science Foundation, the Polish Ministry of Science and Higher Education, the South African Department of Science and Technology and National Research Foundation, the University of Namibia, the Innsbruck University, the Austrian Science Fund (FWF), and the Austrian Federal Ministry for Science, Research and Economy, and by the University of Adelaide and the Australian Research Council. We appreciate the excellent work of the technical support staff in Berlin, Durham, Hamburg, Heidelberg, Palaiseau, Paris, Saclay, and in Namibia in the construction and operation of the equipment. This work benefited from services provided by the H.E.S.S. Virtual Organisation, supported by the national resource providers of the EGI Federation.
Paper: 2018A&A...614A.112L (acknowledgments)
Acknowledgements The authors wish to thank Nathan Crockett for providing the data on Orion KL and Sgr B2, and Peter Schilke for the data on NGC6334I. We also thank Frederik Dhooghe for discussing his results on halogens in 67P/C–G and David Neufeld and Catherine Walsh for discussions on the chemistry. MK is supported by an Intra-European Marie Sklodowska-Curie Fellowship. Astrochemistry in Leiden is supported by the Netherlands Research School for Astronomy (NOVA), by a Royal NetherlandsAcademy of Arts and Sciences (KNAW) professor prize, and by the European Union A-ERC grant 291141 CHEMPLAN. HIFI has been designed and built by a consortium of institutes and university departments from across Europe, Canada andthe United States under the leadership of SRON Netherlands Institute for Space Research, Groningen, The Netherlands and with major contributions from Germany, France and the US. Consortium members are: Canada: CSA, U.Waterloo; France: CESR, LAB, LERMA, IRAM; Germany: KOSMA, MPIfR, MPS; Ireland, NUI Maynooth; Italy: ASI, IFSI-INAF, Osservatorio Astrofisico di Arcetri-INAF; Netherlands: SRON, TUD; Poland: CAMK, CBK; Spain: Observatorio Astronómico Nacional (IGN), Centro de Astrobiología (CSIC-INTA). Sweden: Chalmers University of Technology - MC2, RSS GARD; Onsala Space Observatory; Swedish National Space Board, Stockholm University - Stockholm Observatory; Switzerland: ETH Zurich, FHNW; USA: Caltech, JPL, NHSC.
Paper: 2020ApJ...888..122H (acknowledgments)
We thank Y. L. Yung, J. F. Kasting, C. E. Harman, and S. Seager for a helpful discussion of atmospheric photochemistry. R.Y.H. was supported by NASA grant No. 80NM0018F0612 and grant No. 15038.004 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. The research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Paper: 2019MNRAS.489.4513S (acknowledgments)
ACKNOWLEDGEMENTS The author would like to thank N. Cornish, K. Kyutoku, T. Narikawa, T. Robson, H. Sugiura, and D. Toyouchi for their help. This work is supported by JSPS Kakenhi Grants-in-Aid for Scientific Research (nos. 17H06358 and 19K03870).
Paper: 2018MNRAS.477.1285D (acknowledgments)
Acknowledgements We are grateful to Matthew Walker for providing us with the observational data. We are also grateful to Nana Cabo, Oscar Loaiza, Octavio Obregón, Jorge Peñarrubia, Miguel Sabido, and Erik Verlinde for useful discussions. AXGM acknowledges support from Cátedras CONACYT and UCMEXUS-CONACYT collaborative project funding. This work is supported by CONACyT-Mexico grants 182445, 167335, 179208, 179881, and Fronteras de la Ciencia 281, and also by DAIP-Universidad de Guanajuato grants 1,046/2016 and 878/2016.
Paper: 2019MNRAS.483.3488B (acknowledgments)
ACKNOWLEDGEMENTS We would like to thank Harley Katz, Yohan Dubois, and Marta Volonteri for useful discussion, and the anonymous referee for constructive comments. The research of RSB is supported by Science and Technologies Facilities Council (STFC) and by the Centre National de la Recherche Scientifique (CNRS) on grant ANR-16-CE31-0011, and the research of AS and JD at Oxford is supported by Adrian Beecroft. This work is part of the Horizon-UK project, which used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC High Perforamce Computing Facility ( http://www.dirac.ac.uk ). This equipment is funded by National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National E-Infrastructure. All visualizations in this work were produced using the yt-project (Turk et al. 2011 ).
Paper: 2015MNRAS.449.2668S (acknowledgments)
We would like to thank the referee, Johan Hamaker, for extremely valuable comments that improved the paper. This work is based upon research supported by the South African Research Chairs Initiative of the Department of Science and Technology and National Research Foundation. Trienko Grobler originally pointed us in the direction of Wirtinger derivatives.
Paper: 2019MNRAS.483.3919V (acknowledgments)
ACKNOWLEDGEMENTS I thank the referee for their careful reading of the manuscript and their thoughtful and astute comments, which have led to clear improvements. I gratefully acknowledge the support of the STFC via an Ernest Rutherford Fellowship (grant ST/P003850/1).
Paper: 2019ApJ...881...30T (acknowledgments)
This research has made use of NASA’s Astrophysics Data System. The authors thank the referee, Prof. Shri Kulkarni, for offering comments that significantly improved this manuscript. Facility: TESS .
Paper: 2017A&A...597A.138R (acknowledgments)
We thank Tiago Pereira for his help during the observations. Comments from the referee led to considerable improvement of the presentation. IRIS is a NASA small explorer mission developed and operated by LMSAL with mission operations executed at NASA Ames Research Center and major contributions to downlink communications funded by the Norwegian Space Center through an ESA PRODEX contract. The SST 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 received funding from both the Research Council of Norway and the European Research Council under the European Union’s Seventh Framework Programme (FP7/20072013)/ERC grant agreement No. 291058. We made much use of the SolarSoft and ADS libraries.
Paper: 2017MNRAS.466..974C (acknowledgments)
We thank the anonymous referee for constructive comments which helped us to improve this paper. We are grateful to Kathryn Kreckel for providing us the filtered density contrast of the galaxies from Grogin Geller ( 1999 ) and to Margaret Geller for valuable discussion. EMC was supported by Padua University through grants 60A02-5857/13, 60A02-5833/14, 60A02-4434/15, CPDA133894, and BIRD164402/16. EMC acknowledges the Max-Planck-Institut fr extraterrestrische Physik for the hospitality while this paper was in progress. This investigation was based on observations obtained at the Michigan-Dartmouth-MIT (MDM) Observatory and at the Gemini Observatory under program GN-2011B-9-80. MDM Observatory, Kitt Peak, Arizona is operated by a consortium of Dartmouth College, the University of Michigan, Columbia University, the Ohio State University, and Ohio University. Gemini Observatory 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). Parts of the data used in this research were acquired through the Sloan Digital Sky Survey (SDSS) Archive ( http://www.sdss.org/ ). Funding for the creation and distribution of the SDSS Archive has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the US Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society. The SDSS is managed by the Astrophysical Research Consortium (ARC) for the Participating Institutions. The Participating Institutions are The University of Chicago, Fermilab, the Institute for Advanced Study, the Japan Participation Group, The Johns Hopkins University, the Korean Scientist Group, Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPI), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington. This research also made use of the HyperLeda Database ( http://leda.univ-lyon1.fr/ ) and 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 ( http://ned.ipac.caltech.edu/ ).
Paper: 2017A&A...606A.105R (acknowledgments)
T.R. and D.H. are supported by the German Aerospace Center (DLR, grants 05 OR 1507 and 50 OR 1501, respectively). The GAVO project had been supported by the Federal Ministry of Education and Research (BMBF) at Tübingen (05 AC 6 VTB, 05 AC 11 VTB) and is funded at Heidelberg (05 AC 11 VH3). Financial support from the Belgian FRS-FNRS is also acknowledged. P.Q. is research director of this organization. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. The TIRO ( http://astro.uni-tuebingen.de/~TIRO ), TMAD ( http://astro.uni-tuebingen.de/~TMAD ), and TOSS ( http://astro.uni-tuebingen.de/~TOSS ) services were constructed as part of the Tübingen project of the German Astrophysical Virtual Observatory (GAVO, http://www.g-vo.org ). This research has made use of NASA’s Astrophysics Data System and the SIMBAD database, operated at CDS, Strasbourg, France.
Paper: 2017MNRAS.466.2927R (acknowledgments)
Acknowledgments MMRau thanks the anonymous referee, Gary Bernstein, Michael Troxel and Sarah Bridle for invaluable comments on the manuscript. This work was supported by SFB-Transregio 33 The Dark Universe by the Deutsche Forschungsgemeinschaft (DFG) and the DFG cluster of excellence Origin and Structure of the Universe.
Paper: 2016A&A...591A..15D (acknowledgments)
We acknowledge support by the Spanish Ministerio de Economía y Competitividad (MINECO) under grants AYA2013-47447-C3-1-P, and MDM-2014-0369 of ICCUB (Unidad de Excelencia “María de Maeztu”). This research has been supported by the Marie Curie Career Integration Grant 321520. V.B.-R. also acknowledges financial support from MINECO and European Social Funds through a Ramón y Cajal fellowship. X.P.-F. also acknowledges financial support from Universitat de Barcelona and Generalitat de Catalunya under grants APIF and FI (2015FI_B1 00153), respectively. D.K. acknowledges financial support by a grant-in-aid for Scientific Research (KAKENHI, No. 24105007-1) from the Ministry of Education, Culture, Sports, Science and Technology of Japan (MEXT). M.P. is a member of the working team of projects AYA2013-40979-P and AYA2013-48226-C3-2-P, funded by MINECO.
Paper: 2015ApJ...800...33A (acknowledgments)
We thank Jamie Stevens for carrying out the ATCA observations. The Australia Telescope Compact Array is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO. 9 9 http://www.atnf.csiro.au/research/publications/Acknowledgements.html R.F.A. receives support from a Walter C. Sumner Memorial Fellowship. V.M.K. receives support from an NSERC Discovery Grant and Accelerator Supplement, Centre de Recherche en Astrophysique du Quebec, an R. Howard Webster Foundation Fellowship from the Canadian Institute for Advanced Study, the Canada Research Chairs Program and the Lorne Trottier Chair in Astrophysics and Cosmology. We thank M. Lyutikov, D. Tsang, and K. Gourgouliatos for useful discussions. We also thank an anonymous referee for comments that improved the manuscript. We acknowledge the use of public data from the Swift data archive. This research has made use of data and software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory. The scientific results reported in this article are based in part on observations made by the Chandra X-ray Observatory. This research has made use of CIAO software provided by the Chandra X-ray Center (CXC).
Paper: 2017ApJ...836...34M (acknowledgments)
We thank Andrew Youdin for a helpful discussion. This work is based on observations made with the cryogenic mission of the Spitzer Space Telescope , which was operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. 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. It also 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 project was partially supported by contracts 1255094 and 1256424 from Caltech/JPL to the University of Arizona, and by NASA Grant NNX10AD38G. Facilities: Spitzer (MIPS , IRAC) , WISE .
Paper: 2019MNRAS.489.4001G (acknowledgments)
ACKNOWLEDGEMENTS GBTrans activities are supported by a National Science Foundation (NSF) award AST-1516958. DRL was supported by NSF award number OIA-1458952. GG would like to thank Mayuresh Surnis and Dan Werthimer for useful discussions and Nate Garver-Daniels for the technical support for this work. GG, DRL, RP, and MAM are members of the NANOGrav Physics Frontiers Center that is supported by NSF award 1430284. SWE was supported by NSF award AST-1516170 to Virginia Tech. KR would like to acknowledge financial support from European Research Council Horizon 2020 grant (no. 694745). The Green Bank Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We thank the referee for very helpful comments on an earlier version of the manuscript.
Paper: 2017ApJ...844....7M (acknowledgments)
This work was partially supported by NASA grants NNX09AC46G and NNX13AF31G. We thank Randall Smith for helpful discussions.
Paper: 2018MNRAS.479.5440L (acknowledgments)
ACKNOWLEDGEMENTS This paper makes use of the following ALMA data: ADS/JAO.ALMA2013.1.00521.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with 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 ESO, AUI/NRAO, and NAOJ.
Paper: 2016ApJ...833..112S (acknowledgments)
We warmly thank the German ALMA ARC node for their excellent support for this project and R. Somerville for providing the information on the simulation predictions for our redshift range of interest. We also thank the referee for constructive comments. E.S. acknowledges fruitful discussions with R. Somerville, R. Feldmann, N.Z. Scoville, N. Bouché, and C. de Breuck that helped to significantly focus the paper. B.G. gratefully acknowledges the support of the Australian Research Council as the recipient of a Future Fellowship (FT140101202). A.K. acknowledges support by the Collaborative Research Council 956, sub-project A1, funded by the Deutsche Forschungsgemeinschaft (DFG). Support for B.M. was provided by the DFG priority program 1573 “The physics of the interstellar medium.” V.S. acknowledges funding from the European Union’s Seventh Framework program under grant agreement 337595 (ERC Starting Grant, “CoSMass”). This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00151.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/NRAO, and NAOJ. Based on data obtained with the European Southern Observatory Very Large Telescope, Paranal, Chile, under Large Program 185.A-0791. Facility: ALMA.
Paper: 2018ApJ...858..116F (acknowledgments)
We thank Qiang Yuan and Zhao-Huan Yu for helpful discussions. This work is supported by the National Natural Science Foundation of China (NSFC) under grant nos. 11375277, 11410301005, 11647606, and 11005163, the Fundamental Research Funds for the Central Universities, the Natural Science Foundation of Guangdong Province under grant no. 2016A030313313, and the Sun Yat-Sen University Science Foundation.
Paper: 2019ApJ...883...26K (acknowledgments)
K.J.K. gratefully acknowledges funding for this work received through a NASA Earth and Space Science Fellowship, as well as the use of codes written by B. J. Lynch. The numerical simulations were performed under a grant of NASA High-End Computing resources to C.R.D. on Discover at NASA’s Center for Climate Simulation. Grants from NASA’s Living With a Star, Heliophysics Supporting Research, and Heliophysics Internal Scientist Funding Model programs partially supported K.J.K., S.K.A., J.A.K., and C.R.D.
Paper: 2015MNRAS.451.1307Z (acknowledgments)
Based on observations made with the WHT operated on the island of La Palma by the Isaac Newton Group of Telescopes in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. This research has been supported by the Spanish Ministry of Economy and Competitiveness (MINECO) under the grants AYA2007-67625-CO2-01, AYA2009-12903 and AYA2012-39408-C02-02. JEB acknowledge financial support to the DAGAL network from the People Programme (Marie Curie Actions) of the European Union's Seventh Framework Programme FP7/2007-2013/ under REA grant agreement number PITN-GA-2011-289313. This research made use of astropy , a community-developed core python package for astronomy (Astropy Collaboration et al. 2013 ), aplpy , an open-source plotting package for python hosted at http://aplpy.github.com , and astrodendro , a python package to compute dendrograms of astronomical data ( http://www.dendrograms.org/ ). We acknowledge the usage of the HyperLeda data base ( http://leda.univ-lyon1.fr ). We thank Roberto Terlevich, the referee of the paper, whose comments have led to important improvements on the original version of the paper.
Paper: 2019A&A...621A..76M (acknowledgments)
Acknowledgements We thank the IRAM staff for their support in carrying out the CALYPSO observations, and the anonymous referee for a detailed reading that significantly helped us to improve the paper. We thank Kees Dullemond, Ralf Klessen, Sandrine Bottinelli, Benoit Commercon, and Ralf Launhardt for their participation to the preparation of the CALYPSO project. We thank the INSU “Action Spécifique ALMA” for their financial support to the CALYPSO collaboration. This work has benefited from the support of the European Research Council under the European Union’s Seventh Framework Programme (Advanced Grant ORISTARS with grant agreement No. 291294 and Starting Grant MagneticYSOs with grant agreement No. 679937).
Paper: 2017A&A...607A...6M (acknowledgments)
This work has been funded by the ANR GIPSE ANR-14-CE33-0018. This work has made use of the VALD database, operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna. This work has made use of the BASS2000 data base at http://bass2000.obspm.fr/ . Our group is part of the LabEx OSUG@2020 (Investissement d’avenir – ANR10 LABX56).
Paper: 2017MNRAS.471.2002L (acknowledgments)
Acknowledgments Guang-Xing Li thanks Xun Shi for discussions and for comments on the paper, and thanks Manuel Behrendt and Andi Burket for introducing him the problem and for sharing their views. Alexei Kritsuk is acknowledged for a discussion at MIAPP (Munich) where he introduced the Marochnik etal. ( 1983 ) paper, and Masataka Fukugita is acknowledged for a discussion on H I /H 2 transition. Jens Kauffman and Pavel Kroupa are acknowledge for critical comments. Bruce Elmegreen is acknowledged for an in-depth discussion on the multiphase ISM. Finally, the referee must be thanked for a careful reading of the paper and for the pertinent comments. This paper is supported by the Deutsche Forschungsgemeinschaft (DFG) priority programme 1573 ISM-SPP.
Paper: 2015MNRAS.453..287M (acknowledgments)
The author acknowledges fruitful exchange with H. Andressen, A. Burrows, Th. Foglizzo, A. Heger, W.R. Hix, H.-Th. Janka, Y. Levin, T. Plewa, and T. Waters. He has been supported by the Australian Research Council through a Discovery Early Career Researcher Award (grant DE150101145) and by the Alexander von Humboldt Foundation through a Feodor Lynen fellowship. The computations were performed on Raijin at the NCI National Facility (project fh6) using computer time contingents obtained through NCMAS, ASTAC, and a Monash LIEF top-up grant, on the Monash eGrid Cluster, and on the IBM iDataPlex system hydra at the Rechenzentrum of the Max-Planck Society (RZG).