adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015ApJ...805..151Z (acknowledgments)
This paper was based on observations made with the NASA/ESA Hubble Space Telescope associated with program 13481; support for this program was provided by NASA through a grant from the Space Telescope Science Institute. EML is additionally supported by NASA through Hubble Fellowship grant number HST -HF-51324.01 A from the Space Telescope Science Institute. The Space Telescope Science Institute is operated by the Association of Universities for Research in Astronomy, Incorporated, under NASA contract NAS5-26555.
Paper: 2017A&A...605A..33B (acknowledgments)
We thank Axel Brandenburg for comments and useful discussions. F.D.S. acknowledges the Swedish Research Council International Postdoc fellowship for support, Giuseppe Jacopo Guidi for discussions, and the INAF Astrophysical observatory of Catania for the warm hospitality that allowed this work to be carried out.
Paper: 2016ApJ...816...52H (acknowledgments)
Support for this work was provided by the National Aeronautics and Space Administration through Chandra awards GO2–13091X and AR3-14017X issued by the Chandra X-ray Observatory Center, which is operated by the Smithsonian Astrophysical Observatory for and on behalf of the National Aeronautics Space Administration under contract NAS8–03060. E.S. acknowledges support from The Science Academy (Bilim Akademisi, Turkey) under the BAGEP program. We would like to thank the anonymous referee for carefully reading the paper and providing useful comments.
Paper: 2016A&A...585A..81M (acknowledgments)
This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. We have also used UKIDSS data from the UKIDSSDR8plus database. The UKIDSS project is defined in Lawrence et al. (2007) . UKIDSS uses the UKIRT Wide Field Camera (WFCAM; Casali et al. 2007 ) and a photometric system described in Hewett et al. (2006) . We thank R. M. Humphreys for her comments on an early version of the paper and N. L. J. Cox for his advice on DIBs.
Paper: 2016ApJ...826..159S (acknowledgments)
We thank Jarle Brinchmann, J. J. Eldridge, Elizabeth Stanway, Eric Pellegrini, Selma de Mink, Evan Kirby, Jim Fuller, Phil Hopkins, and Maryam Shirazi for very informative conversations. We benefited significantly from talks, discussions, and conversations during the First Carnegie Symposium in Honor of Leonard Searle, “Understanding Nebular Emission in High-Redshift Galaxies,” held at the Carnegie Observatories in Pasadena, 2015 July 13–17. T. Bensby, C. Esteban, and D. Erb kindly provided machine-readable data from their published work. This work has been supported in part by the US National Science Foundation through grants AST-0908805 and AST-1313472 (C.C.S., A.L.S., R.F.T.), as well as by an NSF Graduate Student Research Fellowship (A.L.S.). Finally, we wish to extend thanks to those of Hawaiian ancestry on whose sacred mountain we are privileged to be guests.
Paper: 2016A&A...585A.129S (acknowledgments)
The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen’s University Belfast, the Harvard-Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics and Space Administration under Grant No. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under Grant No. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE) and the Los Alamos National Laboratory. We thank the anonymous referee for very beneficial comments. T.S. thanks Andrea Merloni, Phil Uttley, Brandon Kelly, Jason Dexter, Simone Scaringi and Barbara De Marco for many helpful discussions and comments.
Paper: 2016A&A...585A..75D (acknowledgments)
L.D.F. acknowledges support through the ESO Studentship Programme, CAPES Programme and CNPq fellowship Programme (166880/2014-0). L.P. acknowledges the Visiting Researcher program of CNPq Brazilian Agency, at the Fed. Univ. of Rio Grande do Norte, Brazil. Support for C.C. is provided by the Ministry for the Economy, Development and Tourism’s Programa Iniciativa Científica do Milênio through grant IC20009, awarded to the Millennium Institute of Astrophysics (MAS). G.F.P.M. acknowledges financial support by CNPq grant 476909/2006-6, FAPERJ grant APQ1/26/170.687/2004 and ESO, for financial support for a trip to Garching, which enabled participation in this work. We thank Dr. Martin Asplund and Dr. Maria Bergemann for their contribution with the line lists used in this work. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France, of NASA’s Astrophysics Data System, of the WEBDA database, operated at the Department of Theoretical Physics and Astrophysics of the Masaryk University, and 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: 2015MNRAS.450.2615S (acknowledgments)
We would like to thank Ezequiel Treister and the anonymous referee for helpful discussions regarding the interpretations of our results. We would also like to thank Scott Chapman for providing radio images of the SSA22 field. CS acknowledges support from CONICYT-Chile (FONDECYT 3120198, Becas Chile 74140006, and the Anillo ACT1101). FEB acknowledges support from CONICYT-Chile (Basal-CATA PFB-06/2007, FONDECYT 1141218, Gemini-CONICYT 32120003, ‘EMBIGGEN”Anillo ACT1101), and Project IC120009 ‘Millennium Institute of Astrophysics (MAS)’ funded by the Iniciativa Científica Milenio del Ministerio de Economía, Fomento y Turismo. The work of DS was carried out at Jet Propulsion Laboratory, California Institute of Technology, under a contract with NASA. JEG thanks the Royal Society. Based on observations made with ESO Telescopes at the Paranal Observatory under programme IDs 085.A-0616 and 089.A-0405. 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 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: 2017A&A...604A..64M (acknowledgments)
Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 60.A-9379. The asteroid diameters and albedos based on NEOWISE observations were obtained from the Planetary Data System (PDS). 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. This research has made use of the Keck Observatory Archive (KOA), which is operated by the W. M. Keck Observatory and the NASA Exoplanet Science Institute (NExScI), under contract with the National Aeronautics and Space Administration. 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. This research used the MPC service developed, maintained, and hosted at the Lagrange laboratory, Observatoire de la Côte d’Azur ( Delbo et al. 2017 ). Photometry of 6 Hebe was identified and extracted from WASP data with the help of Neil Parley (Open University, now IEA Reading). The WASP project is currently funded and operated by Warwick University and Keele University, and was originally set up by Queen’s University Belfast, the Universities of Keele, St. Andrews and Leicester, the Open University, the Isaac Newton Group, the Instituto de Astrofisica de Canarias, the South African Astronomical Observatory and by STFC. The WASP project is currently funded and operated by Warwick University and Keele University, and was originally set up by Queen’s University Belfast, the Universities of Keele, St. Andrews and Leicester, the Open University, the Isaac Newton Group, the Instituto de Astrofisica de Canarias, the South African Astronomical Observatory and by STFC. TRAPPIST-South is a project funded by the Belgian Funds (National) de la Recherche Scientifique (F.R.S.-FNRS) under grant FRFC 2.5.594.09.F, with the participation of the Swiss National Science Foundation (FNS/SNSF). E.J. and M.G. are F.R.S.-FNRS research associates. Based on observations with ISO, an ESA project with instruments funded by ESA Member States and with the participation of ISAS and NASA. Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. Herschel fluxes of Hebe where extracted by Csaba Kiss (Konkoly Observatory, Research Centre for Astronomy and Earth Sciences, Hungarian Academy of Sciences, H-1121 Budapest, Konkoly Thege Miklós út 15–17, Hungary). TM received funding from the European Union’s Horizon 2020 Research and Innovation Programme, under Grant Agreement No. 687378.
Paper: 2015ApJ...799..100D (acknowledgments)
We thank the anonymous referee for his/her useful comments and suggestions to improve the results of this investigation. We are very grateful to Yasuo Fukui and his collaborators for kindly providing to us the fits images related to their investigation ( F14 ). We also thank the Hi-Gal Consortium team and in particular Sergio Molinari for the long-term collaboration and for providing to us the calibration maps. The Herschel data used in this paper belong to the fields Field290_ 0 (Obs-ID: 1342203081, 1342203082) and Field292_ 0 (ObsID: 1342203064, 1342203065), acquired during observing days 458 and 459, respectively. Herschel data are available at the following Web site: http://www.asdc.asi.it/mmia/index.php?mission=herschel . The Herschel spacecraft was designed, built, tested, and launched under a contract to ESA managed by the Herschel /Planck Project team by an industrial consortium under the overall responsibility of the prime contractor Thales Alenia Space (Cannes), and including Astrium (Friedrichshafen), responsible for the payload module and for system testing at the spacecraft level, Thales Alenia Space (Turin), responsible for the service module, and Astrium (Toulouse), responsible for the telescope, with an excess of one hundred subcontractors. This research made use of data products from the Midcourse Space Experiment . Processing of the data was funded by the Ballistic Missile Defense Organization with additional support from the NASA Office of Space Science. This research has also made use of 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. 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.
Paper: 2015ApJ...803...17Z (acknowledgments)
We acknowledge support from the Research Council of Lithuania under the grant No. MIP-85/2012. The European Union FP7-PEOPLE-2010-IRSES program is acknowledged for funding exchange visits in the framework of the project POSTAGBinGALAXIES (grant agreement No. 269193). L. Z. thanks Drs. T. Kipper, M. R. Schmidt, U. G. Jørgensen, and A. Barzdis for assistance during the first iterations of abundance analysis and valuable discussions. This research has made use of the Simbad database operated at CDS (Strasbourg, France) and the VALD database operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna. The publication charge was paid by the Research Council of Lithuania.
Paper: 2018ApJ...860...41L (acknowledgments)
We are grateful to the referee, Prof. Michael Shull, for his thorough reading and for useful comments and suggestions that have significantly improved the clarity of the paper. E.L. thanks G. Calderone for having modified the code QSFit to handle low-resolution WFC3 spectra and for feedback and suggestions on the fitting procedure. E.L. is supported by a European Union COFUND/Durham Junior Research Fellowship (under EU grant agreement 609412). M.F. acknowledges support by the Science and Technology Facilities Council (grant ST/P000541/1). This project has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement 757535). Support for HST Program GO-14127 was provided by NASA through grants from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS526555. M.R. acknowledges support by HST-GO-14127.011 and a NASA Keck PI Data Award, administered by the NASA Exoplanet Science Institute. Some of the data presented herein were obtained at the W.M. Keck Observatory from telescope time allocated to the National Aeronautics and Space Administration through the agency’s scientific partnership with the California Institute of Technology and the University of California. 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. Facilities: HST (WFC3) , Keck:II (ESI). Software: astropy (Astropy Collaboration et al. 2013 ), corner (Foreman-Mackey 2016 ), matplotlib (Hunter 2007 ), emcee (Foreman-Mackey et al. 2013 ), QSFit (Calderone et al. 2017 ).
Paper: 2018MNRAS.480.2449P (acknowledgments)
ACKNOWLEDGEMENTS We acknowledge valuable input from M. Aumer, J. Bland-Hawthorn, C. Dobbs, R. Genzel, K. Masters, M. Miville-Deschenes, E. Ostriker, S. Ragan, and D. Soderblom. We also thank the referee for a careful reading of the original manuscript and for numerous suggestions that improved the clarity and organization of the paper. The research of CFM is supported in part by NASA ATP grant NNX13AB84G.
Paper: 2018A&A...609A.122B (acknowledgments)
This work has been partly funded by a PRIN-INAF 2014 grant, the PRIN INAF SKA-CTA grant and a PRIN MIUR 2015. We acknowledge the CINECA award under the ISCRA initiative, for the availability of high-performance computing resources.
Paper: 2020MNRAS.491.3343G (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for useful comments. R.G. and J.G. are supported by the Israeli Science Foundation under grant No. 719/14 and by the ISF-NSFC joint research program (grant No. 3296/19). We thank Merlin Kole for organizing and the hospitality at the conference Shedding new light on Gamma-Ray Bursts with polarization data in Geneva where part of this work was completed.
Paper: 2020ApJ...889..143D (acknowledgments)
The STEREO /SEPT, Chandra /EPHIN, and SOHO /EPHIN project is supported under grant 50OC1702 by the Federal Ministry of Economics and Technology on the basis of a decision by the German Bundestag. R.G.H. acknowledges the Spanish MICIU/FEDER/AEI for the financial support under project ESP2017-88436-R. I.G.R. acknowledges support from NASA programs NNH17ZDA001N and NH14ZDA001N-LWS, and from the STEREO mission. F.E. and N.D. acknowledge support from NASA grant NNX17AK25G. Additional support from an Alexander von Humboldt group linkage program is appreciated. We thank the International Space Science Institute (ISSI) for hosting our team on “Solar flare acceleration signatures and their connection to solar energetic particles.” Financial support by the Deutsche Forschungsgemeinschaft (DFG) via project GI 1352/1-1 is acknowledged. We thank Dr. R. D. Strauss, Dr. E. Kontar, and Dr. A. Warmuth for helpful discussions.
Paper: 2019ApJ...885...45G (acknowledgments)
We thank the anonymous referee for thoughtful comments and suggestions that improved this paper. We are grateful to D. Koester for sharing his grid of white dwarf atmosphere models. We thank J. J. Hermes for his insightful comments on the appropriate mass ranges for the WD fits. This paper is based on observations made with the NASA/ESA Hubble Space Telescope , obtained at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These observations are associated with program #13354 and R.D.M. has been supported by NASA HST-GO-13354.001-A and NSF AST- 1714506. E.M.L. is funded by a National Science Foundation Astronomy and Astrophysics Postdoctoral Fellowship under award No. AST-1801937. Facility: HST (COS). Software: MESA (Paxton et al. 2015 ), numpy (van der Walt et al. 2011 ), astropy (Astropy Collaboration et al. 2013 ; Price-Whelan et al. 2018 ), emcee (Foreman-Mackey et al. 2013 ), seaborn (Waskom et al. 2018 ), matplotlib (Hunter 2007 ), scipy (Jones et al. 2001 ), ipython (Pérez Granger 2007 ).
Paper: 2015MNRAS.452.1233H (acknowledgments)
We would like to thank Mélanie Habouzit, Yohan Dubois, Joseph Silk, Gary Mamon, Stéphane Colombi, Rebekka Bieri, Andrea Negri, Mitch Begelman, Bhaskar Agarwal, Britton Smith, Mei Sasaki, and Paul Clark for valuable discussions and helpful contributions. We also thank the referee for insightful comments. We are very grateful for the free availability of the code music . We acknowledge funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013) via the ERC Grant ‘BLACK’ under the project number 614199 (TH, MAL, MV) and via the ERC Advanced Grant ‘STARLIGHT: Formation of the First Stars’ under the project number 339177 (RSK, SCOG). SCOG and RSK acknowledges support from the DFG via SFB 881, ‘The Milky Way System’ (subprojects B1, B2 and B8) as well as via SPP 1573 ‘Physics of the Interstellar Medium’. The simulations described in this paper were performed at the Jülich Supercomputing Centre.
Paper: 2016A&A...585A..45G (acknowledgments)
We thank an anonymous referee and M. Walmsley for comments that helped to improve this paper. We thank the SOFIA operations and the GREAT instrument teams, whose support has been essential for the GREAT accomplishments, and the DSI telescope engineering team. Based (in part) on observations made with the NASA/DLR Stratospheric Observatory for Infrared Astronomy. SOFIA Science Mission Operations are conducted jointly by the Universities Space Research Association, Inc., under NASA contract NAS2-97001, and the Deutsches SOFIA Institut, under DLR contract 50 OK 0901. We thank N. Cunningham for providing us with the spectacular image of the region. This work was partly funded by grant ANR-09- BLAN-0231-01 from the French Agence Nationale de la Recherche as part of the SCHISM project. It was also partly supported by the CNRS programme “Physique et Chimie du Milieu Interstellaire”.
Paper: 2015ApJ...815...27K (acknowledgments)
We acknowledge a helpful report from an anonymous referee. J.B.-P. and L.H. acknowledge UNAM-PAPIIT grant number IN103012. Numerical simulations were performed either at Miztli, a 4096-core cluster at DGTIC-UNAM, or at the University of Michigan HPC center, partially supported by UNAM-PAPIIT grant number IN103012 to J.B.-P. A.K. would like to acknowledge funding by the Rackham Graduate School at the University of Michigan.
Paper: 2017MNRAS.469.4675M (acknowledgments)
Acknowledgments We thank the Wyoming NASA Space Grant Consortium who funded this work through the National Aeronautics and Space Administration Grant #NNX15AI08H. ADM was partially supported by National Science Foundation grant 1515404.
Paper: 2015ApJ...813...30S (acknowledgments)
The authors thank Paul Kuin for the UVOTPY software used in extracting the UVOT spectra, Rollin Thomas for the SYN++ and SYNAPPS spectra synthesis packages, and Chris Burns for the SNooPy light-curve analysis program. We also thank the George P. and Cynthia Woods Mitchell Institute for Fundamental Physics Astronomy at Texas AM and the Carnegie Supernova Project. M.S. is supported partially by the NASA Swift Guest Investigator grant NNX15AR51G. P.J.B. and the Swift Optical/Ultraviolet Supernova Archive are supported by NASA’s Astrophysics Data Analysis Program through grant NNX13AF35G. We acknowledge the support of the staff of the Li-Jiang 2.4-m telescope (LJT), and Tsinghua-NAOC 80-cm telescope (TNT). Funding for the LJT has been provided by Chinese academy of science (CAS) and the People’s Government of Yunnan Province. The TNT is owned by Tsinghua University and operated by the National Astronomical Observatory of the Chinese Academy of Sciences (NAOC). J.J.Z. is supported by the National Natural Science Foundation of China (NSFC, grant 11403096). The work of X.F.W. is supported by the Major State Basic Research Development Program (2013CB834903), the NSFC (grants 11073013, 11178003, 11325313), Tsinghua University Initiative Scientific Research Program, and the Strategic Priority Research Program “The Emergence of Cosmological Structures” of the Chinese Academy of Sciences (grant No. XDB09000000). 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.
Paper: 2015ApJ...806..202M (acknowledgments)
This work was supported in part by the DeutscheForschungsgemeinschaft (DFG) via SFB 956. It was also partly supported by fruitful discussions with members of the Czech Science Foundation DFG collaboration (No. 13-00070J) and with members of the European Union Seventh Framework Program (FP7/2007-2013) under grant agreement no 312789; Strong gravity: Probing Strong Gravity by Black Holes Across the Range of Masses.
Paper: 2015ApJ...798..114S (acknowledgments)
We thank the anonymous referee and R. Ulrich for constructive comments. We are grateful to X. Zhao for the spherical harmonic decomposition code, and A. A. Norton and B. McClintock for bringing the DPD catalog to our attention. This work is supported by NASA contract NAS5-02139 (HMI). The HMI data are courtesy of NASA and the SDO /HMI team. The SSN records are courtesy of WDC-SILSO, Royal Observatory of Belgium, Brussels. Facility: SDO
Paper: 2019MNRAS.489.3836A (acknowledgments)
ACKNOWLEDGEMENTS RAB was supported by grant #2017/12828-4, So Paulo Research Foundation (FAPESP). The work of AS was supported by the Russian Science Foundation under grant no.19-71-10018, carried out at the Immanuel Kant Baltic Federal University. EMGDP was partially supported by FAPESP grant #2013/10559-5 and National Council for Scientific and Technological Development (CNPq) grant 306598/2009-4. The simulations were run at the cluster GAPAE of the group of Plasmas and High-Energy Astrophysics from the Institute of Astronomy, Geophysics and Atmospheric Sciences at the University of So Paulo (IAG-USP) (FAPESP grant #2013/10559-5).