adsabs/WIESP2022-NER huggingface dataset:
Paper: 2018A&A...611A..72K (acknowledgments)
Acknowledgements We thank Andrew Fletcher and Aritra Basu for fruitful discussions, and Aritra Basu also for helpful comments on the manuscript. We acknowledge a helpful suggestion of the anonymous referee. 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. RAMW acknowledges support from the National Science Foundation through grant AST-1615594.
Paper: 2019MNRAS.482..321G (acknowledgments)
ACKNOWLEDGEMENTS The authors are very grateful to Bruce Draine and Joseph Weingartner for their valuable and rapid answers to questions regarding their work on the silicate–graphite–PAH dust model. We also thank Simone Bianchi and Andrea Ferrara for their insightful comments on the manuscript. Finally, we would like express our gratitude to the anonymous referee for reading the manuscript with great care and for providing challenging comments that resulted in a constructive discussion and substantial improvements.
Paper: 2016ApJ...827..115S (acknowledgments)
This work was supported by a Postdoctoral Fellowship from Mahidol University, Basic Research Grant BRG5880009 from the Thailand Research Fund, the US National Science Foundation Solar Terrestrial program grant AGS-1063439, and NASA grants NNX14AI63G (Heliospheric Grand Challenge Research) and NNX15AB88G (Living with a Star Program). A.P.S. would like to thank Korn Pattanaseri for assistance with computer simulations.
Paper: 2019A&A...628A..94A (acknowledgments)
The authors thank Benoît Mosser (Paris), Lola Balaguer (Barcelona), Ralf-Dieter Scholz (Potsdam), and the careful referee for valuable comments on the manuscript. We also thank Eleonora Zari (Leiden) for testing a preliminary version of the database. During the preparation of the data for the StarHorse run, we have frequently used the Gaia archive at ESAC ( Salgado et al. 2017 ) as well as its mirrors at AIP and ARI. FA warmly thanks Alcione Mora and Juan González-Núñez (ESAC) for support with the Gaia archive in a critical moment. During the analysis, we have made extensive use of the astronomical java software TOPCAT and STILTS ( Taylor 2005 ), as well as the python packages numpy and scipy ( Oliphant 2007 ), astropy ( Astropy Collaboration 2013 ), dask ( Dask Development Team 2016 ), HoloViews , and matplotlib ( Hunter 2007 ). Figures 3 and B.1 through B.3 were created using the corner package ( Foreman-Mackey 2016 ). For Fig. 9 we used galpy.util.bovy_coords ( Bovy 2015 ) to transform the proper motions to the Galactic frame. This research has made use of the SVO Filter Profile Service ( http://svo2.cab.inta-csic.es/theory/fps/ ; Rodrigo et al. 2012 ; Rodrigo Solano 2013 ) supported from the Spanish MINECO through grant AYA2017-84089. This work has made use of data from the European Space Agency (ESA) mission Gaia ( http://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://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 project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 800502 H2020-MSCA-IF-EF-2017. This work was partially supported by the MINECO (Spanish Ministry of Economy) through grant ESP2016-80079-C2-1-R (MINECO/FEDER, UE) and MDM-2014-0369 of ICCUB (Unidad de Excelencia María de Maeztu).
Paper: 2019ApJ...873...35S (acknowledgments)
We thank the Gemini Observatory staff for their help with our observing program and the anonymous referee for comments that improved the manuscript. J.W., L.J., L.C.H. and X.W. acknowledge support from the National Key RD Program of China (2016YFA0400702, 2016YFA0400703) and from the National Science Foundation of China (grant No. 11473002, 11533001, 11721303). Y.S. acknowledges support from an Alfred P. Sloan Research Fellowship and National Science Foundation grant No. AST-1715579. D.R. acknowledges support from the National Science Foundation under grant No. AST-1614213. M.V. gratefully acknowledges support from the Independent Research Fund Denmark via grant Nos. DFF 4002-00275 and 8021-00130.
Paper: 2018MNRAS.480.4912S (acknowledgments)
ACKNOWLEDGEMENTS JB acknowledges support from FONDECYT Postdoctorados grant 3160439 and the DFG cluster of excellence ‘Origin and Structure of the Universe’. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency.
Paper: 2017ApJ...851...78A (acknowledgments)
We are grateful to the referee for the constructive input which helped improve the paper. M.A. is grateful to Kim Tolbert and Richard Schwartz for useful discussions on uncertainty computation and general use of RHESSI data analysis tools. Thanks to Brian Dennis for his comments on making the best possible images with RHESSI and for numerous science discussions, and to Joel Allred for helpful discussions on the relative importance of energy loss mechanisms in solar plasmas. This work was supported by a NASA Heliophysics Guest Investigator grant and the RHESSI project.
Paper: 2019ApJ...881..132D (acknowledgments)
The authors would like to thank the data provided by the SDO , SOHO /LASCO, and Wind science teams; the anonymous referee’s valuable comments and suggestions that largely improved the quality of the paper; and the helpful discussions with Dr. Yu Liu and Junchao Hong from Yunnan Observatories, CAS, China. This work is supported by the Natural Science Foundation of China (11773068, 1163308, and 11363007), the Yunnan Science Foundation (2017FB006), and the West Light Foundation of Chinese Academy of Sciences. H.C.C. acknowledges the support by NSFC 11703084, 11633008, and 11873088.
Paper: 2016MNRAS.458.1660L (acknowledgments)
We are grateful to Antonia Rowlinson, Yuri Levin, Eric Thrane, Andrew Melatos, Eric Howell, and Pantelis Pnigouras for enlightening conversations and comments on the manuscript. We are also grateful to the anonymous referee for useful feedback that has improved the manuscript. PDL is supported by an Australian Research Council Discovery Project DP1410102578. KG is supported by the Ramón y Cajal Programme of the Spanish Ministerio de Ciencia e Innovación, by a Humboldt Foundation research visit grant at the University of Tübingen, and also acknowledges travel support from NewCompstar (a COST-funded Research Networking Programme).
Paper: 2020ApJ...889..167B (acknowledgments)
Special thanks goes to Pavol Bobik, Giuliano Boella, Karel Kudela, Marian Putis, and Mario Zannoni for their continuous support of the H el M od project and many useful suggestions. This work is supported by ASI (Agenzia Spaziale Italiana) through a contract ASI-INFN I/002/13/0 and by ESA (European Space Agency) through a contract 4000116146/16/NL/HK. Igor Moskalenko and Troy Porter acknowledge support from NASA grant No. NNX17AB48G. We thank the ACE CRIS instrument team and the ACE Science Center for providing the ACE data.
Paper: 2016A&A...592A..92L (acknowledgments)
This work is supported by the National Basic Research Program (“973” Program) of China under Grant No. 2014CB845800 and the National Natural Science Foundation of China (grant Nos. 11573014 and 11473008).
Paper: 2016ApJ...829..101M (acknowledgments)
AGILE is an ASI space mission developed with programmatic support by INAF and INFN. We acknowledge partial support through the ASI grant no. I/028/12/2. This research made use of Enrico, a community-developed Python package to simplify Fermi-LAT analysis (Sanchez Deil 2013 )
Paper: 2016ApJ...826..135L (acknowledgments)
We would like to thank the anonymous referee for important comments and suggestions that have enormously improved the manuscript. This research has made use of data obtained with the Global Millimeter VLBI Array (GMVA), which consists of telescopes operated by the MPIfR, IRAM, Onsala, Metsahovi, Yebes, and the VLBA. The data were correlated with the correlator at the MPIfR in Bonn, Germany. The VLBA is an instrument of the National Radio Astronomy Observatory, a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2018MNRAS.475.1073V (acknowledgments)
Acknowledgements We would like to thank F. La Barbera for a referee report that greatly improved this work, as well as for making available the Na-MILES models used in this paper. SPV would like to thank P. Alton for fruitful discussions on the effect of Na on stellar atmospheres and A. Ferré-Mateu for making her optical measurements of NGC 1277 available. This paper made use of the astropy python package (Astropy Collaboration et al. 2013 ), as well as the matplotlib (Hunter 2007 ) and seaborn plotting software (Waskom et al. 2017 ) and the scientific libraries numpy (Van Der Walt, Colbert Varoquaux 2011 ) and scipy (Jones et al. 2001 ). The Oxford SWIFT integral field spectrograph was supported by a Marie Curie Excellence Grant from the European Commission (MEXT-CT-2003-002792, Team Leader: N. Thatte). It was also supported by additional funds from the University of Oxford Physics Department and the John Fell OUP Research Fund. Additional funds to host and support SWIFT at the 200-inch Hale Telescope on Palomar were provided by Caltech Optical Observatories. This work was supported by the Astrophysics at Oxford grants (ST/H002456/1 and ST/K00106X/1) as well as visitors grant (ST/H504862/1) from the UK Science and Technology Facilities Council. SPV is supported by a doctoral studentship supported by STFC grant ST/N504233/1. RCWH was supported by the Science and Technology Facilities Council (STFC grant numbers ST/H002456/1, ST/K00106X/1 ST/J002216/1). RLD acknowledges travel and computer grants from Christ Church, Oxford, and support from the Oxford Hintze Centre for Astrophysical Surveys, which is funded through generous support from the Hintze Family Charitable Foundation.
Paper: 2017MNRAS.465.3759M (acknowledgments)
Acknowledgments We would like to thank the anonymous referee for a prompt and useful report. This publication was made possible by NPRP grant number X-019-1-006 from the Qatar National Research Fund (a member of Qatar Foundation). The statements made herein are solely the responsibility of the author.
Paper: 2019MNRAS.485..577M (acknowledgments)
ACKNOWLEDGEMENTS The authors are grateful to the Science and Engineering Research Board (SERB), Govt. of India for monetary support in the form of Ramanujan Fellowship (SB/S2/RJN-061/2015) and Early Career Research Award (ECR/2016/000161). RM and MI would also like to thank IISER Bhopal for providing all the research and infrastructure facilities.
Paper: 2019MNRAS.489.5742G (acknowledgments)
ACKNOWLEDGEMENTS We wish to thank David Campbell and Adrian Jenkins for generating the initial conditions and selecting the sample of the Auriga galaxies. IG acknowledges financial support from CONICYT Programa de Astronomía, Fondo ALMA-CONICYT 2017 31170048. AM acknowledges support from CONICYT FONDECYT Regular grant 1181797. FAG acknowledges support from CONICYT FONDECYT Regular grant 1181264. IG, AM, and FAG acknowledge funding from the Max Planck Society through a ‘Partner Group’ grant. FM acknowledges support through the program ‘Rita Levi Montalcini’ of the italian MIUR. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grant ST/H008519/1, and STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure.
Paper: 2017A&A...602A.115D (acknowledgments)
We wish to thank an anonymous referee for his/her helpful suggestions. I.P. acknowledges support by Chandra fund 16617814 contract GO2-13021X. The scientific results reported in this article are based on observations made by the Chandra and XMM-Newton X-ray Observatories. This paper also makes use of data obtained as part of the INT Photometric H Survey of the Northern Galactic Plane (IPHAS, www.iphas.org ) carried out at the Isaac Newton Telescope (INT). The INT is operated on the island of La Palma by the Isaac Newton Group in the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofisica de Canarias. All IPHAS data are processed by the Cambridge Astronomical Survey Unit, at the Institute of Astronomy in Cambridge. The bandmerged DR2 catalog was assembled at the Centre for Astrophysics Research, University of Hertfordshire, supported by STFC grant ST/J001333/1. This publication makes use of data products from the Wide-field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. This research makes use of the SIMBAD database, operated at CDS, Strasbourg, France. We also make heavy use of R: A language and environment for statistical computing. R Foundation for Statistical Computing, Vienna, Austria. ( http://www.R-project.org/ ).
Paper: 2019A&A...629A.115A (acknowledgments)
Acknowledgements This research is supported by the Agence Nationale de la Recherche (project BxB: ANR-17-CE31-0022). F.L. and F.B. acknowledge support from the European Research Council under the European Union’s Horizon 2020 Research Innovation Framework Programme (ERC grant agreement ERC-2016-ADG-742719). S.M. and S.Z. acknowledge support by the ERC InvariantClass 320959. This work was also supported by the Programme National “Physique et Chimie du Milieu Interstellaire” (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES. We gratefully acknowledge fruitful discussions with J.-F. Cardoso, K. Benabed, P. Lesaffre, B. Godard, A. Gusdorf, E. Falgarone, S. Prunet, and J. Neveu. We finally thank the anonymous referee, whose comments helped to significantly improve the manuscript.
Paper: 2017MNRAS.472.4587H (acknowledgments)
Acknowledgements We are grateful to the anonymous referee for useful comments. HH thanks the staff at LAM for their hospitality and financial and technical support during my stay. HH is supported by the Ministry of Science and Technology grant MOST 105-2112-M-001-027-MY3.
Paper: 2017A&A...598A...9B (acknowledgments)
This research was supported in part by the National French Program “Physique et Chimie du Milieu Interstellaire” (PCMI) and the French National Research Agency (ANR-13-BS05-0008-02 “IMOLABS”). The Laboratoire d’Excellence “Chemical and Physical Properties of the Atmosphere” (CaPPA) is also acknowledged. The CaPPA project is funded by the French National Research Agency under contract ANR-11-LABX-0005-01, by the Regional Council “Hauts de France” and by the European Regional Development Fund (ERDF). J. Cernicharo thanks the European Research Council and the Spanish Ministry of Science and Innovation through the NANOCOSMOS (SyG-610256) and ASTROMOL (CSD2009-00038) projects, respectively, and the Spanish Ministry of Economy and Competitiveness through the projects AYA2009-07304, and AYA2012-32032. The referee is also thanked for the valuable comments concerning the hyperfine structure.
Paper: 2016MNRAS.456.3494C (acknowledgments)
JC thanks Graca Rocha and especially Silvia Galli for discussions about the effect of variations of fundamental constants, which helped clarifying the comparison with the previous literature. JC is supported by the Royal Society as a Royal Society University Research Fellow at the University of Cambridge, UK. YAH is supported by NSF Grant No. 0244990, NASA NNX15AB18G, the John Templeton Foundation, and the Simons Foundation. Use of the GPC supercomputer at the SciNet HPC Consortium is acknowledged. SciNet is funded by: the Canada Foundation for Innovation under the auspices of Compute Canada; the Government of Ontario; Ontario Research Fund - Research Excellence; and the University of Toronto.
Paper: 2017MNRAS.468.4340P (acknowledgments)
Acknowledgments We thank the anonymous referee for their comments and suggestions, which have greatly improved the paper. We also thank Kevin Luhman for making his data available to us prior to publication, and for comments and suggestions on the original manuscript. We thank the authors of Parker etal. ( 2014 ) for providing the material for Section 3.1 . RJP acknowledges support from the Royal Society in the form of a Dorothy Hodgkin Fellowship.
Paper: 2018MNRAS.481.4960R (acknowledgments)
ACKNOWLEDGEMENTS This publication is based on data collected under the NGTS project at the ESO La Silla Paranal Observatory. The NGTS instrument and operations are funded by the consortium institutes and by the UK Science and Technology Facilities Council (STFC; project reference ST/M001962/1). LR is supported by an STFC studentship (1795021). The contributions at the University of Leicester by MRG and MRB have been supported by STFC through consolidated grant ST/N000757/1. SLC acknowledges support from LISEO at the University of Leicester. This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement no. 681601). The contributions at the University of Warwick by PJW, RGW, DJA, DP, and TL are supported by an STFC consolidated grant (ST/P000495/1). JSJ acknowledges support by FONDECYT grant 1161218 and partial support by CATA-Basal (PB06, CONICYT). MNG is supported by the UK STFC award reference 1490409 as well as the Isaac Newton Studentship. Contributions at the University of Geneva by FB, BC, LM, and SU were carried out within the framework of the National Centre for Competence in Research ‘PlanetS’ supported by the Swiss National Science Foundation (SNSF). CAW acknowledges support from the STFC grant ST/P000312/1. 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 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: 2019MNRAS.488.5437P (acknowledgments)
ACKNOWLEDGEMENTS FDP is supported by the Science and Technology Facilities Council. MJB acknowledges European Research Council funding by grant ERC-2015-AdG 694520 SNDUST.
Paper: 2018ApJ...866...55C (acknowledgments)
The authors would like to thank S. Sulis for useful discussions regarding colored noise and periodograms, and J. Löhner-Böttcher for sharing results from the LARS spectrograph. The authors also thank the anonymous referee for useful comments, which improved the clarity of this manuscript. H.M.C. acknowledges the financial support of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation (SNSF); S.S., H.M.C, and C.A.W acknowledge support from the Leverhulme Trust. W.J.C., G.R.D., and C.A.W. acknowledge support from the UK Science and Technology Facilities Council (STFC), including grants ST/I001123/1 and ST/P000312/1. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant agreement no.: DNRF106). S.H.S. was supported by NASA Heliophysics LWS grant NNX16AB79G, and M.L.P. was supported by the NSF-REU solar physics program at SAO, grant number AGS-1560313. Some of this work was performed under contract with the California Institute of Technology (Caltech)/Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute (R.D.H.). This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility; DiRAC is part of the National E-Infrastructure. This research has made use of NASA’s Astrophysics Data System Bibliographic Services, as well as the VALD database operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna. Software: MURaM (Vögler et al. 2005 ; Shelyag Przybylski 2014 ; Shelyag 2015 ); OPAL (Rogers et al. 1996 ; Rogers Nayfonov 2002 ); NICOLE (Socas-Navarro 2015 ; Socas-Navarro et al. 2015 ).
Paper: 2016MNRAS.461.3835M (acknowledgments)
We thank the anonymous referee for insightful comments on this manuscript and Jo Bovy for useful discussions. This work has been supported by a postdoctoral grant from the Centre National d'Etudes Spatiales (CNES) for GM. RG acknowledges support through the DFG Research Centre SFB-881 ‘The Milky Way System’ through project A1 .
Paper: 2017MNRAS.466.1839P (acknowledgments)
The authors thank an anonymous referee whose comments helped to improve the scientific content of this work. FP acknowledges support from a post-doctoral STFC fellowship and thanks Inga Cebotaru for carefully reading the manuscript and improve the style. RR acknowledges funding by the graduate college Astrophysics of cosmological probes of gravity by Landesgraduiertenakademie Baden-Wrttemberg.
Paper: 2018A&A...615A...2C (acknowledgments)
Acknowledgements We are very grateful to the staff of the Observatorio del Teide providing excellent support to the operation of the IAC80 and Carlos Sánchez telescopes, and in particular to Álex Oscoz for a generous allocation of time to this project that proved to be essential to its success. We are also equally thankful to the staff of Calar Alto observatory for their support during our AstraLux observing run. The constructive remarks by an anonymous referee helped to improve the presentation of our results. NS acknowledges support by the French ANR and the German DFG through the project “GENESIS” (ANR-16-CE92-0035-01/DFG1591/2-1). 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.
Paper: 2019MNRAS.484.1347H (acknowledgments)
ACKNOWLEDGEMENTS We are grateful to the referee Anita Cochran whose comments improved the quality and clarity of this manuscript. The WHT is 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. We gratefully thank the staff at the Isaac Newton Group for their support in the observations reported here. MGH acknowledges receipt of a Northern Ireland DEL studentship award. AF acknowledges support for this work from UK STFC grants ST/L000709/1 and ST/P0003094/1. CS acknowledges support from the STFC in the form of the Ernest Rutherford Fellowship.
Paper: 2015ApJ...806..172S (acknowledgments)
We thank the IRIS team for providing the data in the public domain. 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 (NSC, Norway) through an ESA PRODEX contract. H.T. is supported by contracts 8100002705 and SP02H1701R from Lockheed-Martin to SAO.