adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015ApJ...810..148C (acknowledgments)
We thank Angela Bragaglia for valuable help and discussions and Alessio Mucciarelli for providing his results for potassium. This publication makes use of data products from the 2MASS, 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. This research has been funded by PRIN MIUR 2010-2011, project “The Chemical and Dynamical Evolution of the Milky Way and Local Group Galaxies” (PI F. Matteucci) . This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France and of NASA’s Astrophysical Data System.
Paper: 2018A&A...612L...3M (acknowledgments)
Acknowledgements We thank an anonymous referee for a helpful review, as well as other anonymous referees, who commented on earlier versions of this manuscript. This work has been carried out in part within the frame of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation. MRM and SPQ are pleased to acknowledge this financial support of the SNSF. M.R. acknowledges funding from the European Research Council Under the European Union’s Seventh Framework Program (ERC Grant Agreement No. 337569) and from the French Community of Belgium through an ARC grant for Concerted Research Action.
Paper: 2016MNRAS.457.1711C (acknowledgments)
AC acknowledges support from the University of Oxford. SAB acknowledges support from the Royal Society in the form of a Wolfson Research Merit Award. We would like to thank the anonymous referee for carefully reading our manuscript and giving in-depth comments which substantially helped improving the quality of the paper.
Paper: 2018MNRAS.480.5352K (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for critical comments that have improved this paper. RK acknowledges support through the DST-INSPIRE Faculty Award by the Government of India. We thank the staff of the GMRT that made these observations possible. 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. This research made use of Astropy, a community-developed core python package for Astronomy (Astropy Collaboration, 2018). The scientific results reported in this article are based in part on data obtained from the Chandra Data Archive.
Paper: 2016ApJ...831..142M (acknowledgments)
The Fermi -LAT Collaboration acknowledges support for LAT development, operation and data analysis from NASA and DOE (United States), CEA/Irfu and IN2P3/CNRS (France), ASI and INFN (Italy), MEXT, KEK, and JAXA (Japan), and the K.A. Wallenberg Foundation, the Swedish Research Council and the National Space Board (Sweden). Science analysis support in the operations phase from INAF (Italy) and CNES (France) is also gratefully acknowledged. This work was partially supported under the NASA contract No. NNG08FD60C, and made use of observations from the NuSTAR mission, a project led by California Institute of Technology, managed by the Jet Propulsion Laboratory, and funded by NASA. We thank the NuSTAR Operations, Software, and Calibration teams for support in the execution and analysis of these observations. This research has made use of the NuSTAR Data Analysis Software (NuSTARDAS) jointly developed by the ASI Science Data Center (ASDC, Italy) and the California Institute of Technology (USA). K.N. was supported by NASA through Einstein Postdoctoral Fellowship grant number PF3-140130 awarded by the Chandra X-ray Center, and by the Polish National Science Centre grant 2015/18/E/ST9/00580. M.B. acknowledges support from NASA under the NASA Earth and Space Science Fellowship Program, grant NNX14AQ07H.
Paper: 2019MNRAS.488.5788C (acknowledgments)
ACKNOWLEDGEMENTS We thank Phil Hopkins for providing us with the current version of gizmo , and are grateful to Alar Toomre and Scott Tremaine for illuminating discussions. This work has been partially supported by the Hubble Space Telescopr /STScI Theory grant AR-14584, and by JSPS KAKENHI grant number 16H02163 (to IS). IS is grateful for support from International Joint Research Promotion Program at Osaka University. The STScI is operated by the AURA, Inc., under NASA contract NAS5-26555. Simulations have been performed on the University of Kentucky DLX Cluster.
Paper: 2018ApJ...868...87B (acknowledgments)
A.E.B., P.T., and M.S. receive financial support from the Perimeter Institute for Theoretical Physics and the Natural Sciences and Engineering Research Council of Canada through a Discovery Grant and through the Alexander Graham Bell scholarship (P.T.). Research at the Perimeter Institute is supported by the Government of Canada through Industry Canada and by the Province of Ontario through the Ministry of Research and Innovation. A.E.B. thanks the Delaney family for their generous financial support via the Delaney Family John A. Wheeler Chair at Perimeter Institute. C.P., M.S., and M.W. acknowledge support by the European Research Council under ERC-CoG grant CRAGSMAN-646955. P.C. gratefully acknowledges support from NSF grant AST-1255469. A.L. receives financial support from an Alfred P. Sloan Research Fellowship, NASA ATP grant NNX14AH35G, and NSF Collaborative Research Grant 411920 and CAREER grant 1455342. E.P. acknowledges support by the Kavli Foundation.
Paper: 2015ApJ...798...49W (acknowledgments)
P.R.W. acknowledges support from contracts from the Los Alamos (LANL) and Sandia National Laboratories and NSF PRAC grant OCI-0832618. The development of the PPB scheme for multifluid fractional volume advection was supported by PRW's LANL contract and DoE grant DEFG02-03ER25569. F.H. acknowledges NSERC Discovery Grant funding. The hydrodynamics simulations were performed on the LCSE workstation cluster, supported by NSF CRI grant CNS-0708822, on NSF's Kraken supercomputer at the National Institute for Computational Sciences (NICS), on the Itasca machine at the Minnesota Supercomputing Institute (MSI), and the Canadian WestGrid Lattice and Orcinus high-performance computers.
Paper: 2019A&A...625A..32B (acknowledgments)
We thank Ivana Ebrová, Benedikt Diemer, and the anonymous referee for their valuable comments. SS acknowledges the support from the Ministry of Education, Science and Technological Development of the Republic of Serbia through project no. 176021 “Visible and Invisible Matter in Nearby Galaxies: Theory and Observations”. FR acknowledges support from the Knut and Alice Wallenberg Foundation. We acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ). This research has made use of “Aladin sky atlas” developed at CDS, Strasbourg Observatory, France. The Digitized Sky Surveys were produced at the Space Telescope Science Institute under US Government grant NAG W-2166. The images of these surveys are based on photographic data obtained using the Oschin Schmidt Telescope on Palomar Mountain and the UK Schmidt Telescope. The plates were processed into the present compressed digital form with the permission of these institutions. We acknowledge support provided by the European Commission through project BELISSIMA (BELgrade Initiative for Space Science, Instrumentation and Modelling in Astrophysics, call FP7-REGPOT-2010-5, contract no. 256772) in the early stage of this project.
Paper: 2018MNRAS.481L..79F (acknowledgments)
ACKNOWLEDGEMENTS We thank the IRAM 30-m staff for precious help during the observations. We thank the anonymous referee for his/her constructive comments. VMR and MP acknowledge the financial support received from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 664931. LC acknowledges support from the Italian Ministero dell’Istruzione, Università e Ricerca through the grant Progetti Premiali 2012 - iALMA (CUP C52I13000140001). PC acknowledges support from the European Research Council (ERC project PALs 320620).
Paper: 2016A&A...595A.121P (acknowledgments)
The authors extend their thanks to the referee for important comments and suggestions. This research has been partly co-financed by the European Union (European Social Fund -ESF) and Greek national funds through the Operational Program “Education and Lifelong Learning” of the National Strategic Reference Framework (NSRF) – Research Funding Program: “Thales. Investing in knowledge society through the European Social Fund”. S.P. acknowledges support from an FP7 Marie Curie Grant (FP7-PEOPLE-2010-RG/268288). M.K.G. wishes to acknowledge support from the EU’s Seventh Framework Programme under grant agreement no PIRG07-GA-2010-268245. The authors acknowledge the Variability of the Sun and Its Terrestrial Impact (VarSITI) international program.
Paper: 2018MNRAS.473.4306A (acknowledgments)
Acknowledgements The author would like to thank Pedro Ferreira, Alan Heavens, Boris Leistedt, Jason McEwen, Anže Slosar and David Spergel for useful comments and discussions, and the Center for Computational Astrophysics, part of the Simons Foundation, for their hospitality. He also acknowledges support from the Science and Technology Facilities Council and the Leverhume and Beecroft Trusts.
Paper: 2019MNRAS.488.4149C (acknowledgments)
ACKNOWLEDGEMENTS In this study, we make use of the numpy, scipy (Jones et al. 2001 ), and Astropy (Astropy Collaboration 2013 ) for python . The figures in this paper were produced using matplotlib (Hunter 2007 ) and inkscape ( https://inkscape.org ). CK and NCS acknowledge support by the Science and Technology Facilities Council (STFC), and from STFC grant ST/M001326/1. MK is funded by a Newton International Fellowship from the Royal Society. PS acknowledges support by the National Science Foundation (NSF) grant AST-1514737.
Paper: 2017MNRAS.465...45C (acknowledgments)
The results reported in this article are based in part on data obtained from the Chandra X-ray Observatory (NASA) Data Archive and from the Data Archive of XMM–Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA. EC, IK, RS acknowledge partial support by grant No. 14-22-00271 from the Russian Scientific Foundation. GP acknowledges support by the German BMWI/DLR (FKZ 50 OR 1408 and FKZ 50 OR 1604) and the Max Planck Society.
Paper: 2016A&A...588A.118M (acknowledgments)
GAPS acknowledges support from INAF through the “Progetti Premiali” funding scheme of the Italian Ministry of Education, University, and Research. L.M. acknowledges the financial support provided by the European Union Seventh Framework Programme (FP7/2007-2013) under Grant agreement number 313014 (ETAEARTH). V.N. acknowledges partial support from INAF-OAPd through the grant “Analysis of HARPS-N data in the framework of GAPS project” (#19/2013) and “Studio preparatorio per le osservazioni della missione ESA/CHEOPS” (#42/2013). J.I.G.H. acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) under the 2013 Ramón y Cajal program MINECO RYC-2013-14875, and the Spanish ministry project MINECO AYA2014-56359-P. We made use of the SIMBAD database and VizieR catalogue access tool, operated at the CDS, Strasbourg, France. We wish to thank the anonymous referee for the valuable comments and suggestions.
Paper: 2016MNRAS.457.3975S (acknowledgments)
AS and LFSR acknowledge useful discussions with the members of the International Team 323 of the International Space Science Institute in Bern. Useful comments of Diego Harari are gratefully acknowledged. APS would like to thank David Ruffolo and Wirin Sonsrettee for useful discussions. APS is grateful to the School of Mathematics and Statistics in Newcastle for hospitality. This work was supported by the Leverhulme Trust (Grant RPG-2014-427) and the STFC (Grant ST/L005549/1).
Paper: 2015MNRAS.453.3386J (acknowledgments)
We are grateful to Bernhard Müller for helpful discussions about various neutrino-transport issues, to Lorenz Hüdepohl for providing his vertex-prometheus data used for the test in Section 4.3.1 , to Bruno Peres for useful comments, and to the anonymous referee for helping to improve the clarity of the manuscript. We acknowledge support by the Max-Planck/Princeton Center for Plasma Physics (MPPC), by the Deutsche Forschungsgemeinschaft through the Transregional Collaborative Research Center SFB/TR 7 ‘Gravitational Wave Astronomy’, by the Computational Center for Particle and Astrophysics (C2PAP) as part of the Cluster of Excellence EXC 153 ‘Origin and Structure of the Universe’, by the European Research Council through ERC-AdG no. 341157-COCO2CASA at Garching and grant CAMAP-259276 at Valencia, and by the Spanish Ministerio de Ciencia e Innovación through grant AYA2013-40979-P Astrofísica Relativista Computacional at Valencia. The computations were performed at the Rechenzentrum Garching, the Leibniz-Rechenzentrum, and at the cluster Lluisvives of the University of Valencia.
Paper: 2019A&A...622A.155Y (acknowledgments)
Acknowledgements We are very grateful to the anonymous referee for his/her helpful comments and suggestions. This paper has made use of information from the APEX Telescope Large Area Survey of the Galaxy. The ATLASGAL project is a collaboration between the Max-Planck-Gesellschaft, the European Southern Observatory (ESO) and the Universidad de Chile. This research made use of data products from the Millimeter Astronomy Legacy Team 90 GHz (MALT90) survey. The Mopra telescope is part of the Australia Telescope and is funded by the Commonwealth of Australia for operation as National Facility managed by CSIRO. This paper is supported by National Natural Science Foundation of China under grants of 11503037.
Paper: 2018ApJ...852..132B (acknowledgments)
We would like to thank the anonymous referee for his or her helpful contributions to the final paper. This work was supported by NASA grant number NNX15AV32G. We thank the NuSTAR Galactic Binaries Science Team for comments and contributions. This research made use of NuSTARDAS, developed by ASDC (Italy) and Caltech (USA).
Paper: 2019ApJ...877...46W (acknowledgments)
The authors acknowledge their sincere thanks to Jordan M. Stone and Thayne Currie for their insightful comments on an earlier version of this manuscript. The results reported herein benefited from collaborations and/or information exchange within NASA’s Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA’s Science Mission Directorate. K.R.W. is supported by the National Science Foundation Graduate Research Fellowship Program under grant No. 2015209499. This research has made use of the NASA Exoplanet Archive, which is operated by the California Institute of Technology, under contract with the National Aeronautics and Space Administration under the Exoplanet Exploration Program.
Paper: 2020A&A...635A..36G (acknowledgments)
We acknowledge M. Salvato and G. Hasinger and entire zCOSMOS, DEIMOS, VUDS, MOSFIRE, FORS2, FMOS, MOIRCS, LEGA-C, and the COSMOS teams for their effort in the COSMOS spectroscopic observations and their willingness to share the spectroscopic redshift catalogues. We wish to thank Kenneth P. K. Quek for his useful comments. The author acknowledges the usage of the following python packages, in alphabetical order: astropy ( Astropy Collaboration 2013 , 2018 ), chainConsumer ( Hinton 2019 ), emcee ( Foreman-Mackey et al. 2019 ), matplotlib ( Hunter 2007 ), numpy ( Oliphant 2006 ; van der Walt et al. 2011 ), and scipy ( Virtanen et al. 2019 ).
Paper: 2019A&A...623A..91T (acknowledgments)
We want to thank the anonymous referee for constructive and useful comments. We acknowledge support by the Spanish Ministerio de Economía y Competitividad (MINECO/FEDER, UE) under grants AYA2013-47447-C3-1-P, AYA2016-76012-C3-1-P, with partial support by the European Regional Development Fund (ERDF/FEDER), MDM-2014-0369 of ICCUB (Unidad de Excelencia “María de Maeztu”), and the Catalan DEC grant 2017 SGR 643. N.T-A. acknowledges support from MINECO through FPU14/04887 grant.
Paper: 2019A&A...627A.133A (acknowledgments)
We wish to thank our colleagues from the Observatoire de Paris-Meudon and the NRH staff for providing the original visibility data. The authors are grateful to the other members of the ARTEMIS group, C. Caroubalos, P. Preka-Papadema, X. Moussas, A. Kontogeorgos and P. Tsitsipis, for their support work. We also wish to thank A. Nindos and S. Patsourakos for useful discussions and comments. Data from TRACE, GOES, the RSTN network, MTI/HXRS and HXT were obtained from the respective data bases; we are grateful to all those who contributed to the operation of these instruments and made the data available to the community.
Paper: 2019MNRAS.490.4175H (acknowledgments)
ACKNOWLEDGEMENTS I thank Jun Makino, Scott Tremaine, Matt Payne, Jack Wisdom, and the anonymous referees for comments that improved this work.
Paper: 2019A&A...623A.100N (acknowledgments)
Acknowledgements We thank the Swiss National Science Foundation (SNSF) and the Geneva University for their continuous support to our planet search programs. This work has been in particular carried out in the frame of the National Centre for Competencein Research “PlanetS” supported by the Swiss National Science Foundation (SNSF). This publication makes use of The Data Analysis Center for Exoplanets (DACE), which is a facility based at the University of Geneva (CH) dedicated to extrasolar planets data visualisation, exchange and analysis. DACE is a platform of the Swiss National Centre of Competence in Research (NCCR) PlanetS, federating the Swiss expertise in Exoplanet research. The DACE platform is available at https://dace.unige.ch . We acknowledge the use of TESS Alert data, which is currently in a beta test phase, from the TESS Science Office and at the TESS Science Processing Operations Center. Funding for the TESS mission is provided by NASA’s Science Mission directorate. 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 study was in part based on observations collected at the European Southern Observatory under ESO programme 0102.C-0503(A). MINERVA-Australis is supported by Australian Research Council LIEF Grant LE160100001, Discovery Grant DP180100972, Mount Cuba Astronomical Foundation, and institutional partners University of Southern Queensland, MIT, Nanjing University, George Mason University, University of Louisville, University of California Riverside, University of Florida, and University of Texas at Austin.
Paper: 2015MNRAS.446L..36F (acknowledgments)
Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center and by the High Performance Computing resources at New York University Abu Dhabi. We acknowledge support from NASA grant NNX11AE05G (to ZH and AM). We are grateful to Daniel D'Orazio, Andrei Gruzinov, and Aleksey Generozov for helpful comments and discussions.
Paper: 2017MNRAS.468.3166P (acknowledgments)
Acknowledgments The first author would like to thanks Iran Science Elites Federation.
Paper: 2017ApJ...844...82N (acknowledgments)
We wish to thank the anonymous referee for reading the original manuscript and providing useful suggestions. Financial support for this work was provided by NSF through AST-1313319 for H.N. and A.C. The UCI group also acknowledges support from HST -GO-14083.002-A, HST -GO-13718.002-A, and NASA NNX16AF38G grants. M.N. has received funding from the European Unions Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 707601. D.R. acknowledges support from the National Science Foundation under grant number AST-1614213 to Cornell University. G.D.Z. acknowledges financial support from ASI/INAF agreement n. 2014-024-R.0. H.D. acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) under the 2014 Ramón y Cajal program MINECO RYC-2014-15686. I.O. and R.J.I. acknowledge support from the European Research Council in the form of the Advanced Investigator Programme, 321302, cosmicism . J.L.W. is supported by a European Union COFUND/Durham Junior Research Fellowship under EU grant agreement number 267209, and acknowledges additional support from STFC (ST/L00075X/1). Some of the data presented herein were obtained at the W.M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W.M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Data presented herein were obtained using the UCI Remote Observing Facility, made possible by a generous gift from John and Ruth Ann Evans. Support for CARMA construction was derived from the Gordon and Betty Moore Foundation, the Kenneth T. and Eileen L. Norris Foundation, the James S. McDonnell Foundation, the Associates of the California Institute of Technology, the University of Chicago, the states of California, Illinois, and Maryland, and the National Science Foundation. Ongoing CARMA development and operations are supported by NSF grant ATI-0838178 to CARMA, and by the CARMA partner universities. The Submillimeter Array is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica.
Paper: 2017MNRAS.465L..79C (acknowledgments)
The simulations in this Letter were run on the COSMOS Shared Memory system at DAMTP, University of Cambridge operated on behalf of the STFC DiRAC HPC Facility. This equipment is funded by BIS National E-infrastructure capital grant ST/J005673/1 and STFC grants ST/H008586/1, ST/K00333X/1. VPD is supported by STFC Consolidated grant #ST/M000877/1.
Paper: 2017MNRAS.470..755H (acknowledgments)
Acknowledgments TH was supported by STFC grant ST/M503812/1 during the course of this work. VW, JM-A, MP and KR acknowledge support from the European Research Council Starting Grant SEDmorph (P.I. V. Wild). The table manipulation software, topcat , was extremely useful at various points in this project (Taylor 2005 ). This research made use of astropy , a community-developed core python package for Astronomy (Astropy-Collaboration 2013 ). The authors thank the anonymous referee for their enormously constructive comments.
Paper: 2019ApJ...871....4H (acknowledgments)
The authors are grateful to the anonymous referee for valuable suggestions. The data are used courtesy of the SDO and IRIS science teams. SDO is a mission of NASA’s Living With a Star Program. 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 ESA and the Norwegian Space Centre. This work is supported by the National Natural Science Foundations of China (11533008, 11790304, 11773039, 11673035, 11673034, 11873059, and 11790300), the Youth Innovation Promotion Association of CAS (2017078 and 2014043), and Key Programs of the Chinese Academy of Sciences (QYZDJ-SSW-SLH050).