adsabs/WIESP2022-NER huggingface dataset:
Paper: 2018A&A...617A.134B (acknowledgments)
Acknowledgements We thank the referee for their interesting and useful comments that helped improve the clarity of the paper. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory. F.B. acknowledges financial support from INAF through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research and through the ASI-INAF contract 2015-019-R.O. A.Z. acknowledges support from Prof. Giuseppe Lodato during his Master thesis work.
Paper: 2015ApJ...806..253M (acknowledgments)
We thank Alberto Sesana for illuminating discussions when starting this project, Phil Armitage for very useful comments on an earlier version of this paper, and Christoph Mordasini for fruitful discussions. We also thank students Gabriel Torrealba and Matías Gárate for their help in developing analysis and visualization tools for Fargo simulations. Financial support was provided by Millennium Nucleus RC130007 (Chilean Ministry of Economy). M.M. acknowledges support from FONDECYT grant No. 3120101 and CONICYT-Gemini grant No. 32130007, J.C. acknowledges support from CONICYTChile through FONDECYT (1141175), Basal (PFB0609), Anillo (ACT1101), and DRI-Intercambio (PCCI130064) grant, S.P. acknowledges financial support provided by FONDECYT grant 3140601, and S.C. acknowledges support from FONDECYT grant 1130949. The authors also thank the referee for suggestions that have improved the presentation of this paper.
Paper: 2019A&A...628A..20D (acknowledgments)
Acknowledgements We would like to thank Leonardo Testi, Hauyu Baobab Liu, Jonathan Williams, Peter Abraham, Agnes Kospal, Klaus Pontoppidan, Giovanni Rosotti, Thomas Haworth, Colin McNally, Willy Kley, Antonella Natta, Nienke van der Marel, Ewine van Dishoeck, Ralf Klessen, Philipp Girichidis, Patrick Hennebelle, Mario van den Ancker, Monika Petr-Gotzens, Adriana Pohl, Carsten Dominik, for useful discussions, and Daniel Thun for help with the Binac Cluster. The authors acknowledgesupport by the High Performance and Cloud Computing Group at the Zentrum für Datenverarbeitung of the University of Tübingen, the state of Baden-Württemberg through bwHPC and the German Research Foundation (DFG) through grant no INST 37/935-1 FUGG. This research was supported by the Munich Institute for Astro- and Particle Physics (MIAPP) of the DFG cluster of excellence “Origin and Structure of the Universe”, in particular the MIAPP workshop “Protoplanetary Disks and Planet Formation” in June 2017 where many of the above discussions took place which considerably helped to improve the argumentation. Part of this work was also funded by the DFG Forschergruppe FOR 2634 “Planet Formation Witnesses and Probes: Transition Disks” under grant DU 414/23-1. F.G. acknowledges support from DFG Schwerpunktprogramm SPP 1992 “Diversity of Extrasolar Planets” grant DU 414/21-1. The research of M.K. is supported by a research grant of the Independent Research Foundation Denmark (IRFD) (international postdoctoral fellow, project number: 8028-00025B). The hydrodynamics models were done with the PLUTO code ( http://plutocode.ph.unito.it ). Some supporting models (not shown in this paper) were performed with the AREPO code ( https://wwwmpa.mpa-garching.mpg.de/~volker/arepo/ ). Finally, we would like to thank the anonymous referee for his/her patience and useful suggestions to improve the paper.
Paper: 2017ApJ...841..111M (acknowledgments)
The authors thank the referee, Marcin Sawicki, for a helpful report that improved this paper. D.M. would like to thank Giuseppe Longo, Audrey Galametz, Sotiria Fotopoulou, and George Helou for helpful conversations. D.M., P.C., D.S., and J.R. acknowledge support by NASA ROSES grant 12-EUCLID12-0004. J.R. and D.S. are supported by JPL, run by Caltech for NASA. F.C. acknowledges support by MINECO grant ESP2015-88861. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Mauna Kea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain.
Paper: 2020MNRAS.491.6102B (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank James Willis for his help with the velociraptor halo finder, and Aaron Ludlow, Cedric Lacey, Richard Bower, Shy Genel, Greg Bryan, and Rob Crain for helpful discussions that contributed significantly to this work. They would also like to thank the anonymous reviewer, who provided many useful suggestions that helped clarify our explanations. This work was initiated as a project for the Kavli Summer Program in Astrophysics held at the Center for Computational Astrophysics of the Flatiron Institute in 2018. The program was co-funded by the Kavli Foundation and the Simons Foundation. We thank them for their generous support. This work was supported by collaborative visits funded by the Cosmology and Astroparticle Student and Postdoc Exchange Network (CASPEN). JB is supported by Science and Technology Facilities Council (STFC) studentship ST/R504725/1. DAA is supported by the Flatiron Institute, which is supported by the Simons Foundation. This work used the ARCHER UK National Supercomputing Service. This work used the DiRAC@Durham facility managed by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). The equipment was funded by BEIS capital funding via STFC capital grants ST/K00042X/1, ST/P002293/1, ST/R002371/1, and ST/S002502/1, Durham University, and STFC operations grant ST/R000832/1. DiRAC is part of the National e-Infrastructure. We would like to extend our thanks specifically to Alastair Basden and his team for managing the DiRAC Memory Intensive service. Software citations This paper made use of the following software packages: GIZMO (Hopkins 2017 ) gadget (Springel 2005 ) swift (Schaller et al. 2016 ) python (Rossum 1995 ), with the following libraries: numpy (Oliphant 2006 ) scipy (Jones et al. 2001 ) py-sphviewer (Benitez-Llambay 2015 ) caesar (Thompson 2018 ) yt (Turk et al. 2011 ) velociraptor (Elahi et al. 2019 ) The AHF (Gill et al. 2004 ; Knollmann Knebe 2009 ).
Paper: 2019A&A...632A..62C (acknowledgments)
The authors thank an anonymous referee for the constructive and helpful comments. A. C. acknowledges funding from the Swiss National Science Foundation under grant P2GEP2_184492.
Paper: 2016MNRAS.459..657B (acknowledgments)
We acknowledge partial financial support from the Spanish Ministerio de Economía y Competitividad Project AYA2012-39475-C02-01 and Consolider-Ingenio 2010 CSD2010-00064. The authors thank Enrique Martínez-González for useful discussions and Francesco Paci for providing an apodisation code. The healp ix package (Górski et al. 2005 ) was used throughout the data analysis.
Paper: 2018ApJ...857...79J (acknowledgments)
We thank the referee for constructive comments that helped to improve the original manuscript. Y.J.-T. would like to thank Dr. Marc Postman for his support, help, and encouragement during her stay at the STScI, which made this work possible. We gratefully acknowledge the computational support of Dr. Fernando Roig. Y.J.-T. also acknowledges financial support from the Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ; fellowship Nota 10, PDR-10) through grant E-26/202.835/2016 and the Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES; Science without Borders program, Young Talent Fellowship, BJT) through grant A062/2013. R.A.D. acknowledges support from the Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq) through BP grant 312307/2015-2 and the Financiadora de Estudos e Projetos (FINEP) grant REF. 1217/13-01.13.0279.00. Both Y.J.-T. and R.A.D. also acknowledge support from the Spanish National Research Council (CSIC; I-COOP+2016 program) through grant COOPB20263 and the Spanish Ministry of Economy, Industry, and Competitiveness (MINECO) through grants AYA2013-48623-C2-1-P and AYA2016-81065-C2-1-P. K.U. acknowledges support from the Ministry of Science and Technology of Taiwan (grant MOST 103-2628-M-001-003-MY3) and from the Academia Sinica Investigator Award. M.M. acknowledges support from the Italian Ministry of Foreign Affairs and International Cooperation, Directorate General for Country Promotion.
Paper: 2016MNRAS.462.4067P (acknowledgments)
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 website is http://www.sdss.org/ . The results described in this paper are based on observations obtained with Herschel , an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. SPIRE has been developed by a consortium of institutes led by Cardiff Univ. (UK) and including: Univ. Lethbridge (Canada); NAOC (China); CEA, LAM (France); IFSI, Univ. Padua (Italy); IAC (Spain); Stockholm Observatory (Sweden); Imperial College London, RAL, UCL-MSSL, UKATC, Univ. Sussex (UK); and Caltech, JPL, NHSC, Univ. Colorado (USA). This development has been supported by national funding agencies: CSA (Canada); NAOC (China); CEA, CNES, CNRS (France); ASI (Italy); MCINN (Spain); SNSB (Sweden); STFC, UKSA (UK); and NASA (USA). This research has made use of data from the HerMES project ( http://hermes.sussex.ac.uk/ ). HerMES is a Herschel Key Programme utilizing Guaranteed Time from the SPIRE instrument team, ESAC scientists, and a mission scientist. HerMES is described in Oliver et al. ( 2012 ). The HerMES data presented in this paper are available through the Herschel Database in Marseille ( http://hedam.lam.fr/HerMES/ ). AF acknowledges support from the ERC via an Advanced Grant under grant agreement no. 321323 NEOGAL. This work makes extensive use of TOPCAT (Taylor 2005 ).
Paper: 2018MNRAS.475.2185C (acknowledgments)
Acknowledgements This work is partially supported by the National Natural Science Foundation of China (NSFC 11433004, U1738211, 11363006, and 11403019), the Applied Basic Research Projects Foundation of Yunnan Province (2014FD001) and Top Talents Program of Yunnan Province.
Paper: 2017ApJ...846...48D (acknowledgments)
This project is funded by DFG grant KE 1897/1-1, SPP 1681 grant WE2623/7-2, and FOR 1509 grant WE2623/13. We also thank the referee for a constructive review of the paper.
Paper: 2019MNRAS.488..213F (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the Science and Technology Funding Council (UK) (ST/P000541/1) and (ST/PN002660/1). OJDF acknowledges the support of STFC (ST/N50404X/1). Horizon 2020: This project has received funding from the European Union’s Horizon 2020 research and innovation programme under grant agreement No 730890. This material reflects only the author's views and the Commission is not liable for any use that may be made of the information contained therein. CC received support from A*MIDEX (project no. ANR-11- IDEX-0001- 02) funded by the ‘Investissements d’Avenir’ French Government program, managed by the French National Research Agency (ANR). This work was supported by the Action Spécifique Haute Résolution Angulaire (ASHRA) of CNRS/INSU co-funded by CNES. This research made use of python including Numpy and Scipy (van der Walt, Colbert Varoquaux 2011 ), matplotlib (Hunter 2007 ) and A stropy , a community-developed core Python package for Astronomy (Robitaille et al. 2013 ). We also made use of the Python AO utility library AOtools ( https://github. com/AOtools/aotools ).
Paper: 2016ApJ...829...19V (acknowledgments)
We thank B. Ochsendorf and K. Tchernyshyov for useful discussions. We thank the referee for the useful comments. 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. SvV is supported by NASA through a Hubble Fellowship (HST-HF2-51350).
Paper: 2018A&A...613A...7Y (acknowledgments)
Acknowledgements This work was supported by the European Research Council Advanced Grant HotMol (ERC-2011-AdG291659).
Paper: 2018ApJ...860...68E (acknowledgments)
N.E.-R. thanks Avet Harutyunyan for his help and acknowledges the hospitality of the Institut de Ciències de l’Espai at the Autonomous University of Barcelona’s Campus, where much of this work was written. Support for this work was provided by NASA/ HST through grants GO-11575, GO-13684, GO-14668, and AR-14295 from the Space Telescope Science Institute (STScI), which is operated by AURA, Inc., under National Aeronautics and Space Administration (NASA) contract NAS5-26555. S.B. and M.T. acknowledge partial financial support by the PRIN-INAF 2017 (project “Towards the SKA and CTA Era: Discovery, Localization, and Physics of Transient Sources”). A.V.F. is grateful for generous financial assistance from the Christopher R. Redlich Fund, the TABASGO Foundation, the Miller Institute for Basic Research in Science (UC Berkeley), and US NSF grant AST-1211916. G.P. acknowledges support provided by the Millennium Institute of Astrophysics (MAS) through grant IC120009 of the Programa Iniciativa Cientíifica Milenio del Ministerio de Economía, Fomento y Turismo de Chile. L.G. was supported in part by NSF grant AST-1311862. N.S. was supported in part by NSF grants AST-1312221 and AST-1515559. This research is based in part on observations made with the NASA/ESA Hubble Space Telescope and obtained from the Hubble Legacy Archive, which is a collaboration between STScI/NASA, the Space Telescope European Coordinating Facility (ST-ECF/ESA), and the Canadian Astronomy Data Centre (CADC/NRC/CSA); the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA (support was provided by NASA through an award issued by JPL/Caltech); the SMARTS Consortium 1.3 m telescope located at Cerro Tololo Inter-American Observatory (CTIO), Chile; and the New Technology Telescope at the European Southern Observatory–La Silla Observatory. Data in this work have been taken in the framework of the European supernova collaboration involved in ESO-NTT large program 184.D-1140 led by Stefano Benetti. Many of the spectra used here for comparison were obtained from the Padova-Asiago Supernova Archive (ASA). This work 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 NASA, and 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 NASA and the NSF. Facilities: Swift , Spitzer , ING:Kapteyn (JAG) , CTIO:1.3m (ANDICAM) , HST (WFPC2) , ACS , WFC3 , ESO:3.6m (EFOSC2 , SOFI) , Magellan:Clay (LDSS-3) , VLT:Yepun (HAWK-I) . Software: IRAF (Tody 1986 , 1993 ), SNOoPy ( http://sngroup.oapd.inaf.it/snoopy.html ), SExtractor (Bertin Arnouts 1996 ), HOTPANTS (Becker 2015 ), Dolphot (Dolphin 2000 ), GELATO ( https://gelato.tng.iac.es ), MOPEX ( http://irsa.ipac.caltech.edu/data/SPITZER/docs/dataanalysistools/tools/mopex/ ).
Paper: 2017MNRAS.467.3122N (acknowledgments)
Acknowledgments J-SN and J-NF acknowledge the support from the Joint Fund of Astronomy of National Natural Science Foundation of China (NSFC) and Chinese Academy of Sciences through the grant U1231202, the NSFC grant 11673003, the National Basic Research Program of China (973 Program 2014CB845700 and 2013CB834900) and the LAMOST FELLOWSHIP supported by the Special Funding for Advanced Users, budgeted and administrated by the Center for Astronomical Mega-Science, Chinese Academy of Sciences (CAMS). J-SN thanks Nami Mowlavi for helpful discussions and useful advice.
Paper: 2020MNRAS.492.5102L (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for a constructive referee report which greatly improved this manuscript. The authors thank Glenn van de Ven, Morgan Fouesneau, Anna Lisa Varri, Gigi Leung, Diederik Kruijssen, Carme Gallart, and Matteo Monelli for useful discussions which improved the manuscript. Dedicated to BL. RL thanks AH. This work was made possible with funding from the Natural Sciences and Engineering Research Council of Canada PDF award and supported by Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (subproject A7 and A8) of the German Research Foundation (DFG), and Deutscher Akademischer Austauschdienst (DAAD) PPP project number 57316058 ‘Finding and exploiting accreted star clusters in the Milky Way’. TRL acknowledges support via grants AYA2014-56795-P and AYA2016-77237-C3-1-P from the Spanish Government. PB acknowledges financial support from a Canadian Institute for Theoretical Astrophysics (CITA) National Fellowship. MAB and JFB acknowledge support from grant AYA2016-77237-C3-1-P from the Spanish Ministry of Economy and Competitiveness (MINECO) and from the Severo Ochoa Excellence programme SEV-2015-0548.
Paper: 2016MNRAS.463..529H (acknowledgments)
We thank the referee for his/her thoughtful comments. The research leading to these results has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013 Grant Agreement no. 614199 , project ‘BLACK’). This work was granted access to the HPC resources of TGCC under the allocations x2014046955, x2015046955 and c2015047012 made by GENCI. We thank Stéphane Rouberoul for smoothly running the horizon cluster in IAP, where the post-processing of the simulations has been done.
Paper: 2019MNRAS.490..527C (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for a very helpful report. The authors would like to thank the Argus instrument team from the Stanford University, Caltech, JPL, University of Maryland, University of Miami, and the Green Bank Observatory for their efforts on the instrument and software that have made this work possible. The Argus instrument construction was funded by the National Science Foundation (NSF) ATI-1207825. Green Bank Observatory is a facility of the National Science Foundation and is operated by Associated Universities, Inc. CYC and ZYL acknowledge support from NSF AST-1815784. ZYL is supported in part by the National Aeronautics and Space Administration (NASA) 80NSSC18K1095 and NNX14AB38G and NSF AST-1716259. AIH and JL acknowledge support from NSF AST-1615647. This research made use of astropy , 7 a community-developed core python package for Astronomy (Astropy Collaboration 2013 , 2018 ).
Paper: 2019A&A...627A.125M (acknowledgments)
The authors are grateful to the anonymous referee for a thoughtful report that helped improve the results and the clarity of this work. The authors acknowledge financial contribution from the agreements ASI-INAF I/037/12/0 and n.2017-14-H.0. This work is partially supported by the HERMES Project, financed by the Italian Space Agency (ASI) Agreement n. 2016/13 U.O. AP acknowledges funding from the European Union’s Horizon 2020 Framework Programme for Research and Innovation under the Marie Sklodowska-Curie Individual Fellowship grant agreement 660657-TMSP-H2020-MSCAIF-2014. 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. AM acknowledges funding from FSE (Fondo Sociale Europeo) Sicilia 2020.
Paper: 2016A&A...589A..52V (acknowledgments)
This study has received financial support from the French State in the frame of the “Investments for the future” Programme IdEx Bordeaux, reference ANR-10-IDEX-03-02. Computer time for this study was provided in part by the computing facilities MCIA (Mésocentre de Calcul Intensif Aquitain) of the Université de Bordeaux and of the Université de Pau et des Pays de l’Adour. P.G. acknowledges support from the ERC Starting Grant (3DICE, grant agreement 336474). P.G.’s postdoctoral position is funded by INSU/CNRS. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. 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. This research has made use of the Exoplanet Orbit Database and the Exoplanet Data Explorer at exoplanets.org.
Paper: 2019A&A...627A.156H (acknowledgments)
We thank Jos de Boer for the TYC 5259-446-1 dataset.
Paper: 2015MNRAS.452.4128M (acknowledgments)
The authors thank F. Israel for comments on the manuscript. The authors are indebted to F. Müller-Sánchez for providing the SINFONI H 2 gas emission map of NGC 1068, O. González-Martín for the Chandra data, J. Wang for the Chandra image of NGC 1068, L. Burtscher for the SINFONI data cubes, F. Combes for the ALMA image of NGC 1566, D. Espada for the ALMA image of CenA, and S. García Burillo for the ALMA image of NGC 1068. MM acknowledges financial support from AYA2011-25527 and NASA Chandra grant G05-16099X. The research leading to the results has received funding from the European Community's Seventh Framework Programme under grant agreement 312430. Research by JAFO was supported by Canary Islands CIE: Tricontinental Atlantic Campus. This research is based on ESO VLT programmes P71.B-0632A, 74.B-0722B and 86.B-0484. The 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.
Paper: 2016ApJ...833..131L (acknowledgments)
I acknowledge the NSF grant AST 1212096, NASA grant NNX14AJ53G and the NSF Center for Magnetic Self Organization (CMSO) as well as a distinguished visitor PVE/CAPES appointment at the Physics Graduate Program of the Federal University of Rio Grande do Norte, the INCT INEspao, and Physics Graduate Program/UFRN. Productive and stimulating discussions with Jungyeon Cho and Gianfranco Brunetti as well as helpful comments of the anonymous referee are acknowledged.
Paper: 2018ApJ...853....8P (acknowledgments)
We would like to thank Atul Chhotray, Hirotaka Ito, and Hiro Nagataki for useful discussions. This work was supported in part by NASA Swift GI grant NNX15AG96G and ATP grant NNX17AK42G.
Paper: 2018ApJ...864...55Z (acknowledgments)
Support for this work was provided by NASA through grants associated with projects GO-13476 and GO-14343 from the STScI, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. This work has made use of data from the European Space Agency 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. S.K. acknowledges the financial support of the Polish National Science Center through the grants OPUS 2014/15/B/ST9/00093 and MAESTRO 2014/14/A/ST9/00121.