adsabs/WIESP2022-NER huggingface dataset:
Paper: 2016ApJ...828...12V (acknowledgments)
SDO is a mission of NASA’s Living With a Star Program. We thank the referee for the suggestions, which helped to improve the paper. P.V. is supported by an INSPIRE grant of AORC scheme under the Department of Science and Technology. W.M. is funded by Chinese Academy of Sciences President’s International Fellowship Initiative Grant No. 2015PE015 and NSFC Grant Nos. 41131065, 41574165, and 41421063. C.M. and T.R. thank the Austrian Science Fund (FWF): [P26174-N27]. The presented work has received funding from the European Union Seventh Framework Programme (FP7/2007-2013) under grant agreement No. 606692 [HELCATS]. C.J.F. was partially funded by STEREO FARSIDE grant to UNH and NASA STEREO grant NNX15AU01G (decline of cycle 24). We thank the ACE SWEPAM and MAG instrument teams and the ACE Science Center for providing the ACE data.
Paper: 2018ApJ...869...61A (acknowledgments)
Results in this paper are based on observations made with the NASA/DLR Stratospheric Observatory for Infrared Astronomy (SOFIA). SOFIA is jointly operated by the Universities Space Research Association, Inc. (USRA), under NASA contract NAS2-97001, and the Deutsches SOFIA Institut (DSI) under DLR contract 50-OK-0901 to the University of Stuttgart. Financial support for this work was provided by NASA through awards SOF-04-0205 and SOF-05-0014, issued by USRA. The authors wish to thank an anonymous referee for very useful comments. Parts of the observations described in this paper were obtained at the Hale Telescope, Palomar Observatory, as part of a continuing collaboration between the California Institute of Technology, NASA/JPL, Yale University, and the National Astronomical Observatories of China. The authors wish to thank Chris Martin, the CWI team, and the staff of the Palomar observatory for permission to use, and assistance with, the semi-private PCWI instrument. The authors also thank S. Laine (Caltech/IPAC) and M. Krause (MPIFR) for permission to use the radio continuum, CO 1–0, and processed IRAC images used in this paper. This work was initiated, in part, at the Aspen Center for Physics, which is supported by NSF grant PHY-1607611. T.D.-S. acknowledges support from ALMA-CONICYT project 31130005 and FONDE-CYT regular project 1151239.
Paper: 2016ApJ...820..104H (acknowledgments)
R. Hounsell acknowledges support from the Space Telescope Science Institute and the University of Illinois at Urbana–Champaign. The USAF/NASA SMEI is a joint project of the University of California San Diego, Boston College, the University of Birmingham (UK), and the Air Force Research Laboratory. P.P.H., A.B., B.V.J., and J.M.C. acknowledge support from NSF grant ATM-0852246 and NASA grant NNX08AJ11G. A.W.S. acknowledges support from NSF grant AST-1009566. S.S. acknowledges partial support from NASA and NSF grants to ASU. We would like to thank Dr. Zach Cano (Centre for Astrophysics and Cosmology at the University of Iceland) for his thoughtful ideas and help during this project. Finally, we would like to thank the referee for their helpful comments and guidance.
Paper: 2016A&A...586A.130S (acknowledgments)
The authors would like to thank the institutional support of the Faculty of Philosophy and Science of the Silesian University in Opava, and the Albert Einstein Centre for Gravitation and Astrophysics supported by the Czech Science Foundation Grant No. 14-37086G.
Paper: 2019MNRAS.488.4816W (acknowledgments)
ACKNOWLEDGEMENTS We are grateful for constructive remarks and suggestions from the referee. We also thank Richard Saxton for sharing the Swift data of XMMSL1 J0740, and Suvi Gezari for sharing some of the data in Fig. 10 . TW is funded in part by European Research Council grant 320360 and by European Commission grant 730980. GL was supported by a research grant (19054) from VILLUM FONDEN. JCAM-J is the recipient of an Australian Research Council Future Fellowship (FT 140101082). PGJ and ZKR acknowledge support from European Research Council Consolidator Grant 647208. MG is supported by the Polish NCN MAESTRO grant 2014/14/A/ST9/00121. KM acknowledges support from STFC (ST/M005348/1) and from H2020 through an ERC Starting Grant (758638). MN acknowledges support from a Royal Astronomical Society Research Fellowship. FO acknowledges support of the H2020 Hemera program, grant agreement No 730970. Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 199.D-0143. We acknowledge the use of public data from the Swift data archive. The Australia Telescope Compact Array is part of the Australia Telescope National Facility which is funded by the Australian Government for operation as a National Facility managed by CSIRO. 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. We also acknowledge the Gaia Photometric Science Alerts Team ( http://gsaweb.ast.cam.ac.uk/alerts ).
Paper: 2018MNRAS.474.2452B (acknowledgments)
Acknowledgements We would like to thank our colleagues Ernesto Vieira Neto, Helton da Silva Gaspar, Luiz Augusto Guimarães Boldrin, Rafael Ribeiro de Sousa and Rodolfo José Bueno Rogerio for valuable discussions. This research was supported by the Brazilian agencies Coordenação de Aperfeiçoamento de Pessoal de Nível Superior - CAPES, Conselho Nacional de Desenvolvimento Científico e Tecnológico - CNPq and Fundação de Amparo à Pesquisa do Estado de São Paulo - FAPESP (proc. 2016/24561-0).
Paper: 2018ApJ...857...58E (acknowledgments)
This research is based on observations made by the Chandra X-ray Observatory and has made use of software provided by the Chandra X-ray Center (CXC) in the application packages CIAO, ChIPS, and Sherpa. P.E. and N.R. acknowledge funding in the framework of the NWO Vidi award A.2320.0076. M.M. is supported by an STFC Ernest Rutherford fellowship (ST/L003597/1). R.P. was partly supported by NSF award AST-1616157. We thank the anonymous referee for many valuable comments. P.E. is grateful to Lia Corrales, Sandro Mereghetti, Elisa Costantini, and Mathieu Renzo for useful discussions. R.P. and P.E. are grateful to Richard McCray for relevant information. Facility: Chandra (ACIS, HRC). Software: ChaRT (Carter et al. 2003 ), CIAO (v4.8; Fruscione et al. 2006 ), FTOOLS (v6.21; Blackburn et al. 1995 ), MARX (v5.3; Davis et al. 2012 ), Sherpa (Freeman et al. 2001 ), XSPEC (v12.9.1; Arnaud et al. 1996 ).
Paper: 2018MNRAS.474.1225A (acknowledgments)
Acknowledgements We thank the anonymous referee for helpful comments that contributed to this paper. We acknowledge helpful conversations with Dave Alexander, Francesca Civano, Andy Fabian, Ryan Hickox, James Mullaney, Kirpal Nandra and Marta Volonteri. JA acknowledges support from ERC Advanced Grant FEEDBACK 340442. AG acknowledges the thales project 383549 that is jointly funded by the European Union and the Greek Government in the framework of the programme ‘Education and lifelong learning’. This work is based in part on observations taken by the CANDELS Multi-Cycle Treasury Program and the 3D-HST Treasury Program (GO 12177 and 12328) with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. The scientific results reported in this article are based to a significant degree on observations made by the Chandra X-ray Observatory.
Paper: 2015ApJ...801...40S (acknowledgments)
We thank Li Zeng for helpful discussions and an anonymous referee for a detailed review that greatly enhanced the quality of this paper.
Paper: 2016MNRAS.456..477G (acknowledgments)
The authors thank Steve Finkelstein for helpful discussions, and the anonymous referee for insightful comments on the manuscript. AGS was supported by an AGEP-GRS supplement to NSF grant AST-1009973. MBK acknowledges support provided by NASA through Hubble Space Telescope theory grants (programs AR-12836 and AR-13888) from the Space Telescope Institute (STScI), which is operated by the Association of Universities for Research in Astronomy (AURA), Inc., under NASA contract NAS5-26555. DRW is supported by NASA through Hubble Fellowship grant HST-HF-51331.01 awarded by the Space Telescope Science Institute. JSB was supported by HST AR-12836 and NSF AST-1009973.
Paper: 2018A&A...615A..33M (acknowledgments)
We thank Christine Wilson for making the Caltech Millimeter Array CO map available to us. We also thank the referee for valuable and supportive comments that have significantly helped us to improve the first submitted version of this paper. AMI acknowledges support from the Spanish MINECO through project AYA2015-68217-P. PMW received support through BMBF Verbundforschung (projects MUSE-AO, grant 05A14BAC, and MUSE-NFM, grant 05A17BAA). Based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programmes 095.B-0042, 096.B-0017, and 097.B-0346. 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 paper uses the plotting package jmaplot developed by Jesús Maíz-Apellániz 7 . We are also grateful to the communities who developed the many python packages used in this research, such MPDAF ( Piqueras et al. 2017 ), Astropy ( Astropy Collaboration et al. 2013 ), numpy ( Walt et al. 2011 ), scipy ( Jones et al. 2001 ) and matplotlib ( Hunter 2007 ).
Paper: 2020ApJ...890..152M (acknowledgments)
M.M.-P. acknowledges support by the KASI and UNAM-DGAPA postdoctoral fellowships. This work is partially supported by the KASI project 2019184100 and Conacyt project CB-2016-281948. O.G.-M. acknowledges support by the PAPIIT projects IA100516. A.A.-H. acknowledges support through grant PG C2018-094671-B-I00 (MCIU/AEI/FEDER,UE). Work by A.A.H. was done under project No. MDM-2017-0737 Unidad de Excelencia “María de Maeztu”- Centro de Astrobiología (INTA-CSIC). Y.K. acknowledges support from grant DGAPA-PAPIIT 106518, and from program DGAPA-PASPA. T.H. acknowledges the support from the National Research Foundation of Korea (NRF) grant funded by the Korea government (MSIT; 2019R1A2C1087045). C.R.A. acknowledges financial support from the Spanish Ministry of Science and Innovation (MICINN) through project PN AYA2013-47742- C4-2-P. C.R.A. also acknowledges the Ramon y Cajal Program of the Spanish Ministry of Economy and Competitiveness. This work is based on observations obtained with the Spitzer Space Observatory , which is operated by JPL, Caltech, under NASA contract 1407. This research has made use of the NASA/IPAC Extragalactic Database (NED), which is operated by JPL, Caltech, under contract with the National Aeronautics and Space Administration. CASSIS is a product of the Infrared Science Center at Cornell University, supported by NASA and JPL.
Paper: 2017ApJ...834..140R (acknowledgments)
This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. L.F.R. and L.L. are grateful to CONACyT, Mexico and DGAPA, UNAM for their financial support. S.L. acknowledges support from project DGAPA IN105815 and CONACytT 238631. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2012.1.00123.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ.
Paper: 2015MNRAS.447.2852K (acknowledgments)
We thank E. Barr, J-P. Macquart and an anonymous referee for extensive helpful comments which have hugely improved the quality of this manuscript. EFK and EP acknowledge the support of the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110 001 020.
Paper: 2017A&A...608A.120A (acknowledgments)
The authors would like to thank the anonymous referee for her or his valuable comments, which substantially helped to improve the quality of the paper. This research has made use of SIMBAD, 2MASS, the GCVS catalogue, and the AAVSO variable search index. D.A. acknowledges the USRA NASA postdoctoral programme and the support of the Center for Space and Habitability of the University of Bern. S.C. acknowledges the Hungarian OTKA Grant K113117. D.K. gratefully acknowledges the support of the Center for Space and Habitability of the University of Bern and the MERAC Foundation for partial financial assistance. This work has been carried out within the frame of the National Centre for Competence in Research PlanetS supported by the Swiss National Science Foundation. D.K. acknowledges the financial support of the SNSF. HIPO work at Lowell is supported by USRA subcontract 8500-98-003. FLITECAM work at UCLA is supported by USRA subcontract 08500-05, PI Ian McLean. M.G. acknowledges financial support by the Helmholtz association, PD-015, and the Technische Universität Berlin.
Paper: 2015A&A...576A..66H (acknowledgments)
Based on observations collected at the German-Spanish Astronomical Center, Calar Alto, jointly operated by the Max-Planck-Institut für Astronomie Heidelberg and the Instituto de Astrofísica de Andalucía (CSIC). Based on observations made with the Italian Telescopio Nazionale Galileo (TNG) operated on the island of La Palma by the Fundación Galileo Galilei of the INAF (Instituto Nazionale di Astrofisica); and with he Nordic Optical Telescope, operated on the island of La Palma jointly by Denmark, Finland, Iceland, Norway, and Sweden; and with the Mercator Telescope, operated on the island of La Palma by the Flemish Community (obtained with the HERMES spectrograph, which is supported by the Fund for Scientific Research of Flanders (FWO), Belgium , the Research Council of K.U.Leuven, Belgium, the Fonds National Recherches Scientific (FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Genève, Switzerland and the Thüringer Landessternwarte Tautenburg, Germany), all operated at the Spanish Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. This work was supported by the Spanish Ministerio de Educación y Ciencia (MEC) under grant AYA2005-02750, Ministerio de Ciencia e Innovación (MICINN) under grant AYA2008-06423-C03-03, AstroMadrid S2009/ESP-1496. M. Hernán-Obispo wants to especially thanks to P. Figueira and M. Marmier for their availability to help and for providing us with the CORALIE data used in the activity study and the information requested. M. C. Gálvez-Ortiz acknowledges financial support by the Spanish MICINN under the Consolider-Ingenio 2010 Program grant CSD2006-00070: first Science with the GTC ( http://www.iac.es/consolider-ingenio-gtc ). She also acknowledges the support of a JAE-Doc CSIC fellowship co-funded with the European Social Fund under the program “Junta para la Ampliación de Estudios” . Financial support was also provided by the Spanish Ministerio de Ciencia e Innovación and Ministerio de Economía y Competitividad under AyA2011- 30147-C03-03 grant. M. Tuomi, J. R. Barnes, M. C. Gálvez-Ortiz and D. J. Pinfield acknowledge support from RoPACS during this research, a Marie Curie Initial Training Network funded by the European Commissions Seventh Framework Programme. J. S. Jenkins acknowledges funding from CATA (PB06, Conicyt). We want also to thanks Saskia Prins for her help in Mercator observations and HERMES pipeline members (L. Dumortier, Y. Fremat, H. Hensberge, A. Jorissen, S. Van Eck, H. Van Wickel) for their help in the data reduction. M. Hernán-Obispo thanks Sito Recuero for his help improving the Fig. 18. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France. The authors are grateful to an anonymous referee for valuable comments and suggestions which have helped improve this paper.
Paper: 2017MNRAS.470.1593R (acknowledgments)
Acknowledgments This research was supported by the Department of Space, Government of India. The research has made use of the SIMBAD data base operated at CDS, Strasbourg, France; the NASA/IPAC Infrared Science Archive, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration, USA; and the 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. We acknowledge the dusty team for making their codes available for the astronomy community. We sincerely thank the anonymous referee for very useful comments, which improved the quality of the article.
Paper: 2018A&A...614A..95S (acknowledgments)
Acknowledgements MS and MJ acknowledge the support of the Academy of Finland Grant No. 285769. JMa acknowledges the support of ERC-2015-STG No. 679852 RADFEEDBACK.
Paper: 2015MNRAS.452..784P (acknowledgments)
ZH acknowledges support from NASA grant NNX11AE05G. JP and RJ acknowledge support from Mineco grant FPA2011-29678-C02-02. JP acknowledges support from Anillo de Ciencia y Tecnologia (Project ACT1101). JP also thanks Yohan Dubois for providing the tracer particle patch for the ramses code. REG was supported by Proyecto Financiamiento Basal PFB-06’Centro de Astronomia y Tecnologias Afines’ and Proyecto Comité Mixto ESO 3312-013-82. The Geryon cluster at the Centro de Astro-Ingenieria UC was extensively used for the analysis calculations performed in this paper. The Anillo ACT-86, FONDEQUIP AIC-57 and QUIMAL 130008 provided funding for several improvements to the Geryon cluster. Finally, we thank the anonymous referee for useful comments on the manuscript.
Paper: 2019MNRAS.484L..79G (acknowledgments)
ACKNOWLEDGEMENTS We thank Marat Gilfanov for helpful comments. O.G. is supported by an NSF Astronomy and Astrophysics Fellowship under award AST-1602595. This work is based on data obtained with the NASA/ESA Hubble Space Telescope , all of which was obtained from MAST. 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 NASA.
Paper: 2018MNRAS.478.1570B (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the Swedish National Space Board (SNSB) through grants 108/12, 112/13, and 96/15. We are indebted to the whole Rosetta mission team, Science Ground Segment, and Rosetta Mission Operation Control for their hard work making this mission possible.
Paper: 2016A&A...590A.128R (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. PQ 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. We thank Ralf Napiwotzki for putting the reduced ESO/VLT spectra at our disposal, Monica Raineri who sent us the electronic versions of the Kr iv ( Bredice et al. 2000 ) and Kr v ( Raineri et al. 2012 ) data, and Liang Liang who provided the Kr vii data ( Liang et al. 2013 ). This work used the profile-fitting procedure, OWENS, that was developed by M. Lemoine and the FUSE French Team. This research has made use of NASA’s Astrophysics Data System and the SIMBAD database, operated at CDS, Strasbourg, France. The TheoSSA service ( http://dc.g-vo.org/theossa ) used to retrieve theoretical spectra for this paper and the TOSS service ( http://dc.g-vo.org/TOSS ) that provides weighted oscillator strengths and transition probabilities were constructed as part of the activities of the German Astrophysical Virtual Observatory.
Paper: 2018ApJ...860...71D (acknowledgments)
The research leading to these results has received funding from the European Union’s Horizon 2020 research and innovation program under the Marie Sklodowska-Curie grant agreement No 745782. B.V. and M.D. acknowledge financial support by the Croatian Science Foundation under project 6212 “Solar and Stellar Variability.” M.T. acknowledges the support by the FFG/ASAP Programme under grant no. 859729 (SWAMI) and from the Austrian Science Fund (FWF) V195-N16.
Paper: 2017ApJ...836..215W (acknowledgments)
This work was sponsored by the Chief of Naval Research and NASA’s Hinode project. Hinode is a Japanese mission developed and launched by ISAS/JAXA, with NAOJ as domestic partner and NASA and STFC (UK) as international partners.
Paper: 2019ApJ...881..123W (acknowledgments)
G.M.W. acknowledges discussions with Frank Rieger, who pointed out the numerical error in the expression for the particle gyro-radius in Equation (99) of Webb et al. ( 2018a ). We thank the referee for a very thorough report and for pointing out inconsistencies and errors in the original manuscript. G.M.W. and G.L. were supported in part by NASA grant 80NSSC19K0075. P.M. acknowledges the support of a NASA Earth and Space Science Fellowship Grant 16-HELIO16F-0022. J.A.L.R. is supported in part by NASA grants NNX15A165G, 80NSSC19K0276, and NSF-DOE grant PHY-1707247. G.P.Z. has been supported in part by the NSF EPSCoR RII-Track-1 Cooperative Agreement OIA-1655280 and an NSF/DOE Partnership in Basic Plasma Science and Engineering via NSF grant PHY-1707247. A.F.B. acknowledges valuable insights and discussions with Prof. Peter Biermann on UHECR and candidate sources and radio galaxies.
Paper: 2015ApJ...807..159T (acknowledgments)
We thank Dr. Jin Matsumoto for fruitful discussions and comments. Shinsuke Takasao acknowledges support from the Research Fellowship of the Japan Society for the Promotion of Science (JSPS). This work was supported by the Grant-in-Aids from the Ministry of Education, Culture, Sports, Science and Technology of Japan (No. 25287039).
Paper: 2015ApJ...814..147P (acknowledgments)
The authors acknowledge the efforts of the Kepler Mission team in obtaining the light curve data used in this publication. These data were generated by the Kepler Mission science pipeline through the efforts of the Kepler Science Operations Center and Science Office. The Kepler Mission is lead by the project office at NASA Ames Research Center. Ball Aerospace built the Kepler photometer and spacecraft which is operated by the mission operations center at LASP. These data products are archived at the Mikulski Archive for Space Telescopes. The authors would thank the University at Albany Physics Department for its ongoing support in our exoplanet research. Daniel Angerhausen’s Research was supported by an appointment to the NASA Postdoctoral Program at the Goddard Space Flight Center, administered by Oak Ridge Associated Universities through a contract with NASA. The authors thank Em DeLarme, Jon Morse, William B. Rossow, and Barbara J. Thompson for discussions about this exciting extrasolar system.