adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015MNRAS.448..642E (acknowledgments)
We acknowledge the grants ASI n.I/023/12/0 ‘Attività relative alla fase B2/C per la missione Euclid’ and MIUR PRIN 2010-2011 ‘The dark Universe and the cosmic evolution of baryons: from current surveys to Euclid’. MB is supported by the Marie Curie Intra European Fellowship ‘SIDUN’ within the 7th Framework Programme of the European Commission. The numerical simulations presented in this work have been performed and analysed on the Hydra cluster at the RZG supercomputing centre in Garching, and on the BladeRunner cluster at the Bologna University, partly funded by the Marie Curie Intra European Fellowship ‘SIDUN’. We acknowledge financial support from PRIN INAF 2012 ‘The Universe in the box: multiscale simulations of cosmic structure.
Paper: 2016MNRAS.457.2391C (acknowledgments)
We would like to thank Gary Bernstein, Sarah Bridle, Jörg Dietrich, Mike Jarvis, Elisabeth Krause, Ravi Sheth, Yuanyuan Zhang, and especially Rachel Mandelbaum for helpful discussions and comments. We are very grateful to Erin Sheldon for the use of his SDSS shear catalogues and to Tomasz Kacprzak for related collaborative work. BJ and MT also thank the Aspen Center for Physics and NSF Grant #1066293, for their warm hospitality when part of this work was done. BJ and JC are partially supported by Department of Energy grant DE-SC0007901. MT is supported by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan, by the FIRST program ‘Subaru Measurements of Images and Redshifts (SuMIRe)’, CSTP, Japan, by Grant-in-Aid for Scientific Research from the JSPS Promotion of Science (No. 23340061 and 26610058), and by MEXT Grant-in-Aid for Scientific Research on Innovative Areas (No. 15H05893 and 15K21733). HM was supported in part by Japan Society for the Promotion of Science (JSPS) Research Fellowships for Young Scientists. HM was supported in part by the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.
Paper: 2019ApJ...874...80M (acknowledgments)
Kohta Murase thanks Poonam Chandra, Boaz Katz, Eran Ofek, Todd Thompson, and Eli Waxman for useful discussions. We also thank internal referees in the Fermi -LAT Collaboration, especially Regina Caputo, Seth Digel, Nicola Omodei, and Nicolas Renault-Tinacci for reviewing the manuscript. The work of Kohta Murase is supported by NSF grant No. PHY-1620777 and the Alfred P. Sloan Foundation. He also acknowledges the Hubble Fellowship through NASA and STScI during the early stages of this work. A.F. was supported by the Initiative and Networking Fund of the Helmholtz Association. Keiichi Maeda acknowledges support by JSPS KAKENHI grant Nos. 18H04585, 18H05223, 17H02864. J.F.B. is supported by NSF grant No. PHY-1714479. The preliminary estimates and results were presented at the PCTS workshop at Princeton University in 2015, the AMON workshop at Penn State University in 2015, and the supernova workshop at ISSI in 2016. The Fermi -LAT Collaboration acknowledges generous ongoing support from a number of agencies and institutes that have supported both the development and the operation of the LAT, as well as scientific data analysis. These include the National Aeronautics and Space Administration and the Department of Energy in the United States; the Commissariat à l’Energie Atomique and the Centre National de la Recherche Scientifique Institut National de Physique Nucléaire et de Physique des Particules in France; the Agenzia Spaziale Italiana and the Istituto Nazionale di Fisica Nucleare in Italy; the Ministry of Education, Culture, Sports, Science and Technology (MEXT), High Energy Accelerator Research Organization (KEK), and Japan Aerospace Exploration Agency (JAXA) in Japan; and the K. A. Wallenberg Foundation, the Swedish Research Council, and the Swedish National Space Board in Sweden. Additional support for science analysis during the operations phase is gratefully acknowledged from the Istituto Nazionale di Astrofisica in Italy and the Centre National d’Études Spatiales in France. This work was performed in part under DOE Contract DE-AC02-76SF00515.
Paper: 2017MNRAS.469.3670S (acknowledgments)
Acknowledgments The authors would like to thank the anonymous referee for their helpful comments. We would also like to thank R. Davies and K. Pimbblet for discussion and suggestions which greatly improved the clarity of this paper. This publication made extensive use of the Tool for Operations on Catalogues And Tables (TOPCAT; Taylor 2005 ) that can be found at http://www.star.bris.ac.uk/mbt/topcat/ and the open source Python module astroPy ; 9 Astropy Collaboration etal. ( 2013 ). This research has also made use of NASAs ADS service and Cornells ArXiv. RJS would like to acknowledge funding from both the Science and Technology Facilities Council, Grant Code ST/K502236/1, and from the Ogden Trust. SJK would like to acknowledge the funding from STFC Grant Code ST/MJ0371X/1. The development of Galaxy Zoo was supported in part by the Alfred P. Sloan Foundation and by The Leverhulme Trust. Based on observations made with the NASA Galaxy Evolution Explorer. GALEX is operated for NASA by the California Institute of Technology under NASA contract NAS5-98034. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. 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 Web Site 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: 2017MNRAS.470.2938F (acknowledgments)
Acknowledgements This research was supported in part by the US Department of Energy through grant GR523126, the National Science Foundation through grant GR506177 and the Space Telescope Science Institute through grant GR528562. AP would also like to acknowledge that partial salary support was provided by the Canadian Institute for Theoretical Astrophysics (CITA) National Fellowship.
Paper: 2016MNRAS.456L.109K (acknowledgments)
I thank Chris Nixon and Stuart Muldrew for discussions and help in preparing the Letter, and the referee for a very perceptive report. This paper was completed during a visit to the Institut d'Astrophysique, Paris, and I am grateful to them for support. I particularly thank Jean-Pierre Lasota for discussions of accretion disc stability during my stay. Theoretical astrophysics research in Leicester is supported by an STFC Consolidated Grant.
Paper: 2018A&A...616L...8S (acknowledgments)
We thank the referee, Sergei Nayakshin, for useful comments that improved the quality of the letter as well as D. Calderón, M. Habibi, and L. Oskinova for very useful comments and discussion. For the computations and analysis, we have made use of many open-source software packages, including R AMSES ( Teyssier 2002 ), yt ( Turk et al. 2011 ), NumPy, SciPy, matplotlib, hdf5, h4py. We thank everybody involved in the development of these for their contributions. MS acknowledges support by the Deutsche Forschungsgemeinschaft through grant no. BU 842/25-1. The computations were performed on the HPC system HYDRA of the Max Planck Computing and Data Facility.
Paper: 2018MNRAS.477.4228P (acknowledgments)
Acknowledgements We thank an anonymous referee for very useful comments and suggestions, and Valerie Connaughton for providing us with the details of the Fermi GBM follow ups to the BBH merger events in runs O1 and O2. RP was partly supported by NSF award AST-1616157. KB acknowledges support from the Polish National Science Center (NCN) grant: Sonata Bis 2 (DEC-2012/07/E/ST9/01360). AC acknowledges support from the NSF CAREER award #1455090 and also partial support from the Swift Cycle 12 GI programme (Grant No. NNX17AF93G).
Paper: 2016ApJ...822..104H (acknowledgments)
This study is based on observations obtained in the framework of the ESO Prg. 092.D-0209(A). A.K. thanks Saint Petersburg State University for grant 6.38.18.2014.
Paper: 2017MNRAS.469.3322G (acknowledgments)
Acknowledgments I am grateful to Shahram Abbassi for helpful comments on this paper. I also thank the referee for his/her thoughtful and constructive comments that greatly helped me to improve this paper.
Paper: 2018MNRAS.476.1111P (acknowledgments)
Acknowledgements This work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work has also made use of the Rainbow Cosmological Surveys data base, which is operated by the Universidad Complutense de Madrid (UCM), partnered with the University of California Observatories at Santa Cruz (UCO/Lick,UCSC) and used observations taken by the CANDELS Multi-Cycle Treasury Program with the NASA/ESA HST, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555.
Paper: 2019ApJ...870...34Z (acknowledgments)
We appreciate the MMS teams for the high-quality data and successful operation. This work is supported by the National Natural Science Foundation of China (NSFC) under grants 41522405, 41774154, and 41331070. The data used in this study was obtained from the MMS Science Data Center ( https://lasp.colorado.edu/mms/sdc/public/ ).
Paper: 2019ApJ...883...65S (acknowledgments)
The authors thank W. Dziembowski for his contribution to the theoretical predictions for activity-related frequency shifts in Metcalfe et al. ( 2007 ). The authors thank D. Bossini for providing the evolutionary tracks shown in this paper. A.R.G.S. acknowledges the support from National Aeronautics and Space Administration under grant NNX17AF27G. T.L.C. acknowledges support from the European Unions Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 792848 and from grant CIAAUP-12/2018-BPD. W.J.C., G.R.D., R.H., and Y.E. acknowledge the support of the UK Science and Technology Facilities Council (STFC). M.S.C acknowledges support from FCT—Fundação para a Ciência e a Tecnologia—through national funds and by FEDER through COMPETE2020—Programa Operacional Competitividade e Internacionalização—through the grants: UID/FIS/04434/2019; PTDC/FIS-AST/30389/2017 POCI-01-0145-FEDER-030389. C.K. is supported by the Villum Foundation. Funding for the Stellar Astrophysics Centre is provided by the Danish National Research Foundation (grant agreement No.: DNRF106). T.S.M. acknowledges support from a Visiting Fellowship at the Max Planck Institute for Solar System Research. S.M. acknowledges the support from the Ramon y Cajal fellowship number RYC-2015-17697. R.A.G. acknowledges the support from PLATO and GOLF CNES grants. M.N.L. acknowledges the support of The Danish Council for Independent Research—Natural Science (grant DFF-4181-00415). R.K. acknowledges the support of the STFC consolidated grant ST/P000320/1. V.S.A. acknowledges support from the Independent Research Fund Denmark (Research grant 7027-00096B). Software: SciPy (Jones et al. 2001 ), NumPy (van der Walt et al. 2011 ), Matplotlib (Hunter 2007 ), scikit-learn (Pedregosa et al. 2011 ), MESA (Paxton et al. 2011 , 2013 , 2015 , 2018 ).
Paper: 2017ApJ...843..109G (acknowledgments)
We thank the authors of K16 , especially M. Kadler and F. Krauss for providing the data on PKS B1424-418. S.G. and M.P. acknowledge support by the Helmholtz Alliance for Astroparticle Physics (HAP) funded by the Initiative and Networking Fund of the Helmholtz Association. W.W. acknowledges funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (Grant No. 646623).
Paper: 2016MNRAS.460.3052C (acknowledgments)
We thank the anonymous referee for very useful comments and suggestion to improve this work. We acknowledge support from CONICYT-Chile grants, Basal-CATA PFB-06/2007 (DC, FEB, SS), FONDECYT 1141218 (FEB), PCCI 130074 (FEB), ALMA-CONICYT 31100004 (FEB), Gemini-CONICYT 32120003 (FEB), ‘EMBIGGEN’ Anillo ACT1101 (DC, FEB), the Ministry of Economy, Development, Tourism's Millennium Science Initiative through grant IC120009 awarded to The Millennium Institute of Astrophysics, MAS (FEB, SS), CONICYT-Chile through PCHA/Doctorado Nacional (2015-21151574) (DC), and by NASA through Herschel contracts 1427277 and 1454738 (SV). Optical observations were obtained with the Magellan/Baade as part of the program CN–2015A–129. We acknowledge NASA and Mikulski Archive for Space Telescopes (MAST) for the use of data retrieved from MAST.
Paper: 2016ApJ...826..217L (acknowledgments)
This work was supported by the National Natural Science Foundation of China (NSFC) under the grant Nos. 10878002, 11025314, 10673004, 10610099a, and 11533005, as well as NKBRSF under the grants 2011CB811402 and 2014CB744203. W.C. acknowledges the support of the US NSF (AGS-0847126 and AGS-1250818) and NASA (NNX13AG14G).
Paper: 2017MNRAS.471.2812B (acknowledgments)
Acknowledgements We would like to kindly thank Michael Marks for useful discussions and suggestions. We would also like to thank an anonymous referee for numerous comments and suggestions. DB was supported by the CAPES foundation, Brazilian Ministry of Education through the grant BEX 13514/13-0 and by the National Science Centre, Poland, through the grant UMO-2016/21/N/ST9/02938. AA would like to acknowledge support from the National Science Centre, Poland, through the grant UMO-2015/17/N/ST9/02573 and partial support from Nicolaus Copernicus Astronomical Centre's grant for young researchers.
Paper: 2019ApJ...886....3L (acknowledgments)
The work was supported in part by the project NNX17AB74G of NASA’s HGI Program.
Paper: 2019ApJ...882...10N (acknowledgments)
We would like to thank the referee for constructive comments that helped clarify the paper. This paper makes use of the following ALMA data: ADS/JAO.ALMA #2015.1.01115.S, #2016.1.00544.S, and #2017.1.01301.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. M.N., F.W., B.V., and Ml.N. acknowledge support from ERC Advanced grant 740246 (Cosmic_Gas). D.R. acknowledges support from the National Science Foundation under grant No. AST-1614213.
Paper: 2016MNRAS.458.3808R (acknowledgments)
We thanks the anonymous referee for his/her comments and suggestions. This research has been funded by MINECO grant AYA2014-59084-P, by the AGAUR, by the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement no. 320964 (WDTracer), by Milenium Science Initiative, Chilean Ministry of Economy, Nucleus P10-022-F, by Fondecyt (1141269, 3140585) and by the National Key Basic Research Programme of China (2014CB845700). 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 web site 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.
Paper: 2015ApJ...814..106C (acknowledgments)
This work is partially supported by the Spanish Ministry of Science through projects AYA2010-18029, AYA2011-24808, and AYA2014-55078-P. This work contributes to the deliverables identified in FP7 European Research Council grant agreement 277829, “Magnetic connectivity through the Solar Partially Ionized Atmosphere.”
Paper: 2018A&A...612A..75B (acknowledgments)
Acknowledgement We would like to thank Ivan Minchev for a very opportune question while we recently met at the Gaia meeting in Nice, and Benoit Famaey and Christian Boily for pertinent remarks.
Paper: 2016MNRAS.463.1332S (acknowledgments)
This work has been supported by the Polish Ministry of Science and Higher Education through the program ‘Ideas Plus’ award No. IdP2012 000162. The OGLE project has received funding from the Polish National Science Centre grant MAESTRO no. 2014/14/A/ST9/00121. RS acknowledges support from the Polish National Science Centre grants no. DEC-2012/05/B/ST9/03932 and DEC-2015/17/B/ST9/03421.
Paper: 2020MNRAS.493L..87H (acknowledgments)
ACKNOWLEDGEMENTS The authors thank the anonymous referee for their helpful comments that improved the presentation of this work. The authors thank Connor Bottrell, Greg Bryan, John Forbes, Shy Genel, Li-Hwai Lin, Nic Loewen, Ari Maller, Hsi-An Pan, David Patton, Rachel Somerville, Mallory Thorp, and Joanna Woo for their insightful comments and helpful discussions. MHH acknowledges the receipt of a Vanier Canada Graduate Scholarship. SLE acknowledges the receipt of an NSERC Discovery Grant. The data used in this work were, in part, hosted on facilities supported by the Scientific Computing Core at the Flatiron Institute, a division of the Simons Foundation.
Paper: 2016ApJ...818...73T (acknowledgments)
We thank the anonymous referee for constructive suggestions that improved the quality of the manuscript. The authors wish to thank I.(K.) Lee, A. Stutz, B. Reipurth, J. Jorgensen, A. Kraus, and L. Tychoniec for useful discussions regarding this work. J.J.T. is currently supported by grant 639.041.439 from the Netherlands Organisation for Scientific Research (NWO). J.J.T. acknowledges past support provided by NASA through Hubble Fellowship grant #HST-HF-51300.01-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 NAS 5-26555. L.W.L. acknowledges support from the Laboratory for Astronomical Imaging at the University of Illinois and the NSF under grant AST-07-09206. Z.Y.L. is supported in part by NSF1313083 and NASA NNX14AB38G. C.M. acknowledges financial support from the U.S. National Science Foundation through award AST-1313428. M.M.D. acknowledges support from the Submillimeter Array through an SMA postdoctoral fellowship. This research made use of Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration, 2013, http://www.astropy.org ). This research made use of APLpy, an open-source plotting package for Python hosted at http://aplpy.github.com . This research has made use of NASA's Astrophysics Data System. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. Facility: VLA
Paper: 2016MNRAS.457..903P (acknowledgments)
We thank Nicolas Bouché, Max Pettini and Crystal Martin for inputs on the work presented here. We also thank the anonymous referee for many suggestions that have improved the paper. We would like to thank the Paranal and Garching staff at ESO for performing the observations in service mode and the instrument team for making a reliable instrument. CP thanks the ESO science visitor programme for support. SQ thanks CNRS and CNES (Centre National d'Etudes Spatiales) for support for his PhD. VPK acknowledges partial support from the US National Science Foundation grant AST/1108830 and NASA grant NNX14AG74G. Additional support from a NASA/STScI grant for programme 13733 is gratefully acknowledged. This work has been carried out thanks to the support of the OCEVU Labex (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the ‘Investissements d'Avenir’ French government programme managed by the ANR. L. A. S. acknowledges support from ERC Grant agreement 278594-GasAroundGalaxies.
Paper: 2018ApJ...862..165T (acknowledgments)
We thank K. S. Cheng, C. W. Ng, K. L. Li, J. Takata, and A. K. H. Kong for valuable discussion. We acknowledge the use of data and software facilities from the FSSC, managed by the HEASARC at the Goddard Space Flight Center. This work is supported by the National Natural Science Foundation of China (NSFC) through grants 11633007, 11661161010, and U1731136.
Paper: 2015A&A...581A..69C (acknowledgments)
Financial support from the Academy of Finland Centre of Excellence ReSoLVE No. 272157 (MJK) and from the Vilho, Yrjö and Kalle Väisälä Foundation (EC) is gratefully acknowledged.
Paper: 2015MNRAS.448.2617M (acknowledgments)
This publication is supported by NPRP grant no. 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 authors. Based on observations obtained with the 1.52-m Cassini telescope at the OAB Observatory in Loiano (Italy), and with the 1.23-m and 2.2-m telescopes at the Centro Astronòmico Hispano Alemàn (CAHA) at Calar Alto (Spain), jointly operated by the Max-Planck Institut for Astronomy and the Instituto de Astrofìsica de Andalucìa (CSIC). We thank to TÜBİTAK for the partial support in using T100 telescope with project number 12CT100-378. OB acknowledges the support by the research fund of Ankara University (BAP) through the project 13B4240006.
Paper: 2018A&A...609A..80F (acknowledgments)
Support comes from the ERC Synergy Grant “BlackHoleCam – Imaging the Event Horizon of Black Holes” (Grant 610058). M.P. acknowledges support by the Spanish “Ministerio de Economía y Competitividad” grants AYA2013-48226-C3-2-P and AYA2015-66899-P. Z.Y. acknowledges support from an Alexander von Humboldt Fellowship. E.R. acknowledges support from the grants AYA-2012-38491-C02-01, AYA2015-63939-C2-2-P, and PROMETEOII/2014/057. C.M.F. wants to thank Walter Alef and Helge Rottmann for support during the computation on the MPIfR cluster and Mariafelicia De Laurentis and Hector Olivares for fruitful discussion and helpful comments to the manuscript.
Paper: 2019ApJ...876...83A (acknowledgments)
The authors thank the anonymous referee for their helpful comments that improved the data analysis and strengthened the conclusions. The authors further thank A. Strugarek and J. Varela for the use of their data, as well as S. Mathis for extensive discussions and helpful advice. The authors also thank S. Tobias for his helpful comments. K.C.A. acknowledges support from the ERC SPIRE 647383 grant. A.S.B. acknowledges funding by ERC WHOLESUN 810218 grant, INSU/PNST, and CNES Solar Orbiter. J.T. was partly supported by NASA through grants NNX14AB56G and NNX17AG22G.