adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019A&A...622A..81M (acknowledgments)
E.H. acknowledges support by the Spanish Ministry of Economy and Competitiveness (MINECO) and the Fondo Europeo de Desarrollo Regional (FEDER) through grant ESP2016-80435-C2-1-R, as well as the support of the Generalitat de Catalunya/CERCA program. D. D. acknowledges support provided by NASA through Hubble Fellowship grant HST-HF2-51372.001-A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS5-26555. E.S. acknowledges support by the Russian Science Foundation grant No. 14-50-00043 for conducting international photometric observing campaign. I.S. acknowledges support by the Russian Foundation for Basic Research (project No. 17-02-00542). R.B. acknowledges support from FONDECYT Post-doctoral Fellowship Project No. 3180246. M.L. acknowledges support from the Austrian Research Promotion Agency (FFG) under project 859724 “GRAPPA”. S.-H.G. acknowledges the financial support from the National Natural Science Foundation of China (No.U1531121). L.C. recognizes funding from DLR – 50OR1804. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant agreement no.: DNRF106). We thank the staff at the various participating observatories STELLA, CASLEO, Calar Alto, TJO, and others for their support. Partly based on data obtained with the STELLA robotic telescopes in Tenerife, an AIP facility jointly operated by AIP and IAC, on data acquired at Complejo Astronómico El Leoncito, operated under agreement between the Consejo Nacional de Investigaciones Científicas y Técnicas de la República Argentina and the National Universities of La Plata, Córdoba and San Juan, on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC), and on data obtained with the Joan Oró Telescope (TJO) of the Montsec Astronomical Observatory (OAdM), owned by the Generalitat de Catalunya and operated by the Institute for Space Studies of Catalonia (IEEC). This research has made use of the SIMBAD data base and VizieR catalog access tool, operated at CDS, Strasbourg, France, and of the NASA Astrophysics Data System (ADS).
Paper: 2016ApJ...832..177S (acknowledgments)
This research has made use of data and software obtained from the High Energy Astrophysics Science Archive Research Center (HEASARC), provided by NASA’s Goddard Space Flight Center. We acknowledge the use of Fermi -LAT data and analysis tools from Fermi Science Support Center. We thank Dr. David Paneque for providing published multiwaveband campaign data of Mrk 501.
Paper: 2017ApJ...845...59V (acknowledgments)
SDO is a mission of NASA’s Living With a Star Program. SOHO is a project of international cooperation between ESA and NASA. This work used the DAVE4VM code written and developed by P. W. Schuck at the Naval Research Laboratory. I thank the referee, Prof. P. Démoulin, and Prof. B. Ravindra for useful comments and suggestions. P.V. is supported by an INSPIRE grant of AORC scheme under the Department of Science and Technology.
Paper: 2018MNRAS.481.4698F (acknowledgments)
ACKNOWLEDGEMENTS We acknowledge partial financial support from the Center for Space and Habitability (CSH), the PlanetS National Center of Competence in Research (NCCR), the Swiss National Science Foundation, a European Research Council (ERC) Consolidator Grant, and the Swiss-based MERAC Foundation. CF acknowledges partial financial support from a University of Bern International 2021 Ph.D. Fellowship. We thank Simon Grimm, Daniel Kitzmann, Maria Oreshenko, Shami Tsai, and Matej Malik for constructive conversations.
Paper: 2017ApJ...850..194F (acknowledgments)
H.F. and G.Z. are supported by the National Natural Science Foundation of China under grant nos. 11390371, 11233004, and 11603033. D.G.Y. was supported by NSF grant AST-1009603, D.E.W. by NSF grant AST-1238926, J.A.D. by NSF grant AST-1008424, T.P.S. by NSF grant AST-1009929, and B.L.R. by NSF grant AST-1008801. Based in part on data obtained from the ESO Science Archive Facility by user “zihaoj.” Facilities: APO (ARCES) , ESO/Max Planck: 2.2 m (FEROS) , Magellan : Clay (MIKE) .
Paper: 2016MNRAS.462.3386S (acknowledgments)
This work is based upon research supported by the Science Faculty at University of Cape Town (UCT), the South African National Research Foundation and the Department of Science and Technology . Part of this research was conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020 . WLW acknowledges support from the UK Science and Technology Facilities Council [ST/M001008/1]. We thank Dr Tom Mutabazi and Hiroki Onozato for running some of the observations. We also thank Dr Yasushi Nakajima, Dr Takahiro Nagayama and Dr Ihab Riad for many discussions regarding the reduction pipeline. We are very grateful to Dr Christina Magoulas for her careful reading and comments on the paper. We are grateful to Dr Anja Schroeder for making the 2MASX bright galaxy ZOA list available prior to publication.
Paper: 2017A&A...600A...4C (acknowledgments)
This paper makes use of the following ALMA data: ADS/JAO.ALMA2013.0.00458.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), NSC and ASIAA (Taiwan), and KASI (Republic of Korea), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO and NAOJ. The data presented here were first reduced by CASA (ALMA default calibration software), but a second iteration in the data reduction and later analysis for presentation was made by using the MAPPING package available in the GILDAS software ( http://www.iram.fr/IRAMFR/GILDAS ). Also, Fig. 5 was obtained from few 30 m-IRAM telescope acquisitions and data from the APEX telescope data archive. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain). APEX is a collaboration between the Max-Planck-Institut fur Radioastronomie, the European Southern Observatory, and the Onsala Space Observatory. This work has also been supported by the Spanish MINECO, grants AYA2016-78994-P and FIS2012-32096, and by the European Research Council (ERC) Grant 610256: NANOCOSMOS.
Paper: 2018ApJ...855..128W (acknowledgments)
P.E.H. acknowledges support from NSF awards AST-0506666 and AST-0908010 and NASA/ATP awards NNX08AG83G and NNX12AH06G to the University of Alabama. This work made use of the Swinburne University of Technology software correlator, developed as part of the Australian Major National Research Facilities Programme and operated under license. Earth Orientation and Ionospheric data hosted on the Crustal Dynamics Data Information System (CDDIS) at the NASA Goddard Space Flight Center were used in this project. This study makes use of 43 GHz VLBA data from the VLBA-BU Blazar Monitoring Program (VLBA-BU-BLAZAR; http://www.bu.edu/blazars/VLBAproject.html ), funded by NASA through the Fermi Guest Investigator Program. C.L. and F.B.D. were summer students at the NRAO when they became involved in this project.
Paper: 2018MNRAS.473.5334R (acknowledgments)
Acknowledgements This paper is based on observations obtained at the Gemini Observatory, which is operated by the Association of Universities for Research in Astronomy, Inc., under a cooperative agreement with the NSF on behalf of the Gemini partnership: the National Science Foundation (United States), the National Research Council (Canada), CONICYT (Chile), the Australian Research Council (Australia), Ministério da Ciência, Tecnologia e Inovação (Brazil) and Ministerio de Ciencia, Tecnología e Innovación Productiva (Argentina) and also on observations collected at the European Organisation for Astronomical Research in the Southern hemisphere under ESO programmes 079.C-0328(A) and 079.C-0328(B). This research has also made use of the NED, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. Some of the data presented in this paper were based on observations made with the NASA/ESA HST, obtained from the data archive at the Space Telescope Institute. STScI is operated by the association of Universities for Research in Astronomy, Inc. under the NASA contract NAS 5-26555. This publication also 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. TVRacknowledges CNPq for the financial support under the grant 304321/2016-8. JES acknowledges FAPESP for the financial support under the grant 2011/51680-6. DM acknowledges CNPq for the financial support under the grant 312987/2016-1. The optical data were obtained under grant support from Instituto do Milênio, MEGALIT (AGR). RBM acknowledges CAPES (Coordenação de Aperfeiçoamento de Pessoal de Nível Superior). Finally, we thank Roberto Cid Fernandes for carefully reading the manuscript, which improved a lot the quality of this work, and also Juliana Cristina Motter, for English revision. We also thank the anonymous referee for valuable insights that also enriched this paper.
Paper: 2019MNRAS.486..112K (acknowledgments)
ACKNOWLEDGEMENTS JK acknowledges the financial support of the Polish National Science Centre during the period 2015–2019 (grant 2015/17/B/ST9/03397) and the grant UMO-2017/25/B/ST9/01524 for the period 2018–2021. GAG, JK, and GGV acknowledge the Chilean fund CONICYT grant REDES180136 for financial support of their international collaboration. This paper includes data gathered with the VLT (UVES) ESO telescope and the 3.6 m (ESpADoNs) CFH telescope. 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..
Paper: 2017A&A...600A.112I (acknowledgments)
This paper is based on observations made with ESO telescopes at the La Silla Paranal Observatory under program ID 092.B-0104(A). We have made extensive use of the SIMBAD Database at CDS (Centre de Données astronomiques) Strasbourg, the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, CalTech, under contract with NASA, and of the VizieR catalog access tool, CDS, Strasbourg, France. Support for J.B., D.M., J.C.B., R.K., M.H. is provided by the Ministry of Economy, Development, and Tourism’s Millennium Science Initiative through grant IC120009, awarded to The Millennium Institute of Astrophysics, MAS. Support for R.K. is provided from Fondecyt Reg. No. 1130140. R.K.S. acknowledges support from CNPq/Brazil through project 310636/2013-2. We are grateful to the anonymous referee for useful suggestions that helped to improve the paper.
Paper: 2017ApJ...835..124E (acknowledgments)
Work performed by F.E., F.R.d.C. and V.P. was supported by NASA grants NNX13AF79G and NNX14AG03G. M.O. was supported by NASA grants NNX08AO83G at UC Berkeley and NNH16AC60I at Los Alamos National Laboratory (LANL). W.L. was supported by NASA HGI grant NNX16AF78G. L.G. was supported by an NSF Faculty Development Grant (AGS-1429512) to the University of Minnesota. Work performed by F.R.d.C. and W.L. is part of the team effort under the title of “Diagnosing heating mechanisms in solar flares through spectroscopic observations of flare ribbons” at the International Space Science Institute (ISSI). M.O. and F.E. are part of the ISSI team “Particle Acceleration in Solar Flares and Terrestrial Substorms.”
Paper: 2017ApJ...846....5L (acknowledgments)
We thank the anonymous referee for a careful reading of our manuscript and for constructive comments and suggestions, which improved the paper. HIFI has been designed and built by a consortium of institutes and university departments from across Europe, Canada, and the United States under the leadership of SRON Netherlands Institute for Space Research, Groningen, The Netherlands, and with major contributions from Germany, France, and the US. Consortium members are: Canada: CSA, U.Waterloo; France: CESR, LAB, LERMA, IRAM; Germany: KOSMA, MPIfR, MPS; Ireland: NUI Maynooth; Italy: ASI, IFSI-INAF, Osservatorio Astrofisico di ArcetriINAF; Netherlands: SRON, TUD; Poland: CAMK, CBK; Spain: Observatorio Astronmico Nacional (IGN), Centro de Astrobiologia (CSIC-INTA); Sweden: Chalmers University of Technology MC2, RSS GARD, Onsala Space Observatory, Swedish National Space Board, Stockholm University Stockholm Observatory; Switzerland: ETH Zurich, FHNW; USA: Caltech, JPL, NHSC. L.J. and Y.G. acknowledge support by NSFC grant nos. 11311130491 and 11420101002 and CAS Key Research Program of Frontier Sciences B program no. XDB09000000.
Paper: 2016MNRAS.457.1888S (acknowledgments)
We thank the anonymous referee for their detailed comments, which have improved the clarity of this paper. JPS, AMS, RGB, CMH and IRS acknowledge support from STFC (ST/I001573/1 and ST/L00075X/1). JPS also gratefully acknowledges support from a Hintze Research Fellowship. IRS acknowledges support from an ERC Advanced Investigator programme DUSTYGAL 321334 and a Royal Society/Wolfson Merit Award. AJB gratefully acknowledges the hospitality of the Research School of Astronomy Astrophysics at the Australian National University, Mount Stromlo, Canberra where some of this work was done under the Distinguished Visitor scheme. DS acknowledges financial support from the Netherlands Organisation for Scientific research (NWO) through a Veni fellowship and from FCT through an FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010). PNB is grateful for support from STFC (ST/M001229/1). We thank Holly Elbert, Timothy Green and Laura Prichard for their observations and Alex Karim for providing main-sequence fits. We also thank Matthieu Schaller for discussions on the EAGLE simulation quantities and Omar Almaini for discussions on the UDS. Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under the programme IDs 60.A-9460, 092.B-0538, 093.B-0106, 094.B-0061 and 095.B-0035. This research uses data from the VIMOS VLT Deep Survey, obtained from the VVDS data base operated by Cesam, Laboratoire d'Astrophysique de Marseille, France. This paper uses data from the VIMOS Public Extragalactic Redshift Survey (VIPERS). VIPERS has been performed using the ESO VLT, under the ‘Large Programme’ 182.A-0886. The participating institutions and funding agencies are listed at http://vipers.inaf.it . This paper uses data from zCOSMOS which is based on observations made with ESO Telescopes at the La Silla or Paranal Observatories under programme ID 175.A-0839. We acknowledge the Virgo Consortium for making their simulation data available. The EAGLE simulations were performed using the DiRAC-2 facility at Durham, managed by the ICC, and the PRACE facility Curie based in France at TGCC, CEA, Bruyres-le-Chtel. This work is based in part on data obtained as part of the UKIRT Infrared Deep Sky Survey.
Paper: 2017ApJ...835...18G (acknowledgments)
I am very grateful to the anonymous referee for their very valuable comments and suggestions, which greatly improved the quality of this work. I thank Professor Richard V. E. Lovelace for his constructive comments in the initial version of this manuscript. Also, I would like to thank Dr. M. Nejad-Asghar and Dr. H. Ebadi for their fruitful discussions, which were helpful for revising the manuscript. This work has been supported financially by Research Institute for Astronomy Astrophysics of Maragha (RIAAM) under research project No. 1/4717-65.
Paper: 2015MNRAS.450..592R (acknowledgments)
The authors wish to thank the anonymous referee for comments that helped improved the presentation of this work. We thank August Evrard for comments on an early draft of this manuscript. We also thank Nabila Aghanim for help with accessing the full Planck cluster catalogue and validation table. This work was supported in part by the US Department of Energy contract to SLAC no. DE-AC02-76SF00515. JGB gratefully acknowledges support from the Institut Universitaire de France . A portion of the research described in this paper was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Paper: 2019A&A...627A..90V (acknowledgments)
M.V. acknowledges support from Grant 17-06065S by the Grant Agency of the Czech Republic and from the AV ČR Grant RVO:67985815.
Paper: 2018ApJ...863...80X (acknowledgments)
We acknowledge NASA contract NAS5-02099 for use of data from the THEMIS Mission. Specifically, we thank C. W. Carlson and J. P. McFadden for the use of ESA data; K. H. Glassmeier, U. Auster, and W. Baumjohann for the use of FGM data; and D. Larson and R. P. Lin for the use of SST data. We also thank SILSO ( http://www.sidc.be/silso/datafiles ) for providing the sunspot numbers and the World Data Center ( http://wdc.kugi.kyoto-u.ac.jp/aeasy/index.html ) for providing the AE indices. This work is supported by the Science and Technology Development Fund of Macao SAR (008/2016/A1 and 119/2017/A3) and National Natural Science Foundation of China (NSFC) under grants 41564007 and 41374174.
Paper: 2015MNRAS.450.4277V (acknowledgments)
The figure production made use of the pgplot software at the NRC Canada in Victoria.
Paper: 2019ApJ...880..101Y (acknowledgments)
This research was carried out using data obtained from the Data Archive and Transmission System (DARTS), provided by the Center for Science-satellite Operation and Data Archive (C-SODA) at ISAS/JAXA. This work was partially supported by a MEXT-Supported Program for the Strategic Research Foundation at Private Universities, 2014–2018 (S1411024).
Paper: 2015MNRAS.449..559S (acknowledgments)
We thank the referee for an insightful report which helped to improve our paper. GS, NVA and RCF acknowledge the support from the CAPES–COFECUB project 30007ZD. LS acknowledges the support from CAPES and FAPESP. MVCD thanks FAPESP and CAPES/PDSE–BEX 8509/11-5 scholarships that allowed him to develop this project. He also acknowledges the hospitality of the LUTH, at Observatoire de Paris for a long-term visit. NVA acknowledges the support and hospitality of the LUTH, at Observatoire de Paris, for short term visits. This work has made use of the computing facilities of the Laboratory of Astroinformatics (IAG/USP, NAT/Unicsul), whose purchase was made possible by the Brazilian agency FAPESP (grant 2009/54006-4) and the INCT-A. All the authors wish to thank the team of the SDSS for their dedication to a project which has made this work possible. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS website is http://www.sdss.org/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington.
Paper: 2015ApJ...801...85S (acknowledgments)
This work was supported by NSF AAG grant 1211329. J.R.M and K.M.M. were supported under contract with the California Institute of Technology (Caltech) funded by NASA through the Sagan Fellowship Program. This material is based upon work supported by the National Science Foundation Graduate Research Fellowship under Grant No. DGE-1143953. Any opinion, findings, and conclusions or recommendations expressed in this material are those of the authors(s) and do not necessarily reflect the views of the National Science Foundation.
Paper: 2018MNRAS.480L.106O (acknowledgments)
ACKNOWLEDGEMENTS GO acknowledges the constructive comments from the referees helped to greatly improve this Letter and thanks Oliver Hahn and Frank van den Bosch for careful reading of the draft. GO was supported by funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research andinnovation programme (grant agreement No. 679145, project ‘COSMO-SIMS’).
Paper: 2017ApJ...842...87M (acknowledgments)
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. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the participating institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III website is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration, including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, University of Florida, the French Participation Group, the German Participation Group, Harvard University, the Instituto de Astrofisica de Canarias, the Michigan State/Notre Dame/JINA Participation Group, Johns Hopkins University, Lawrence Berkeley National Laboratory, Max Planck Institute for Astrophysics, Max Planck Institute for Extraterrestrial Physics, New Mexico State University, New York University, Ohio State University, Pennsylvania State University, University of Portsmouth, Princeton University, the Spanish Participation Group, University of Tokyo, University of Utah, Vanderbilt University, University of Virginia, University of Washington, and Yale University. Part of this work is based on archival data, software, or online services provided by the ASI Science Data Center. The NASA/IPAC Extragalactic Database (NED) is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration. TOPCAT 14 14 http://www.star.bris.ac.uk/mbt/topcat/ (Taylor 2005 ) was used for the preparation and manipulation of the tabular data and the images. F. M. gratefully acknowledges the financial support of the Programma Giovani Ricercatori—Rita Levi Montalcini—Rientro dei Cervelli (2012) awarded by the Italian Ministry of Education, Universities and Research (MIUR).
Paper: 2016ApJ...833..106Y (acknowledgments)
The author acknowledges NSF grant AGS1550566 to the University of Maryland, and the BK21 plus program from the National Research Foundation (NRF), Korea, to Kyung Hee University. He also acknowledges the Science Award Grant from GFT Inc. to the University of Maryland.