adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015MNRAS.453.2480W (acknowledgments)
SAW and ACF acknowledge support from ERC Advanced Grant FEEDBACK. This work is based on observations obtained with the Chandra observatory, a NASA mission. It is also based on observations with XMM–Newton , an ESA science mission with instruments and contributions directly funded by ESA Member States and NASA.
Paper: 2016A&A...596A..20V (acknowledgments)
The authors thank the helpful referee for constructive and important comments. B.V. also thanks E. van Groningen for helpful comments, Brad Peterson for showing the AGN black hole mass database and A. Magnard, F. Poulenc, G. von Rivia and J. Pianist for inspiring discussions. She also acknowledges A. Barth, H. Netzer and M. Elitzur for help with the intermediate line region. B.V. was funded and supported by the Centre of Interdisciplinary Mathematics (Uppsala Universitet) and Erik and Märta Holmbergs donation from Kungliga Fysiografiska Sällskapet. This research also heavily relies on the Sloan Digital Sky Survey (SDSS). Funding for SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the Japanese Monbukagakusho, and the Max Planck Society.
Paper: 2015A&A...579A..56B (acknowledgments)
E.B. thanks the New York University at Abu Dhabi for the kind hospitality during part of this work and Milvia Capalbi for her precious support during the analysis of some XRT observations. We thank Phil Evans for useful discussions. A.P. is supported by a Juan de la Cierva fellowship, and acknowledges grants AYA2012-39303, SGR2009-811, and iLINK2011-0303. P.R. acknowledges contract ASI-INAF I/004/11/0. We thank N. Schartel and the XMM-Newton team for having promptly performed the ToO observation analyzed in this paper. We are indebted to the Swift PI and operations team for the continuous support during the monitoring campaign of X-ray transients.
Paper: 2019ApJ...882..108W (acknowledgments)
We thank the anonymous referee for helpful comments. This work is supported by the National Natural Science Foundation of China (grant No. U1831207).
Paper: 2016A&A...595A..38D (acknowledgments)
This research was financed by the Swiss National Science Foundation project 200021_149865. V.d.F. and M.F. acknowledge the Department of Physics at the University of Basel and especially Friedrich-K. Thielemann. We also thank the International Space Science Institute in Bern for their support. V.d.F. is grateful to the International Space Science Institute in Beijing for the hospitality to carry out part of this work. L.S. acknowledges partial support under contract ASI INAF I/004/11/1.
Paper: 2017A&A...607A..11G (acknowledgments)
The authors thank the referee for the many useful comments and suggestions which helped to improve this work. 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. This work has made use of the Vizier database, operated at CDS, Strasbourg, France, the cross-match service provided by CDS, Strasbourg, and M. Skarka’s BlaSGalF online list of Blazhko effect stars ( http://www.physics.muni.cz/~blasgalf/ ).
Paper: 2018A&A...610A..40R (acknowledgments)
Acknowledgments This work was supported by Fundação para a Ciência e a Tecnologia (FCT) through national funds (UID/FIS/04434/2013) and by FEDER through COMPETE2020 (POCI-01-0145-FEDER-007672). A.C.S.R. acknowledges the support of an IA fellowship: CIAAUP-17/2015-BI in the context of the project (UID/FIS/04434/2013 POCI-01-0145-FEDER-007672). P.P.P. acknowledges the visitor’s programme grant from Instituto de Astrofisica e Ciências do Espaço, Portugal. This work has made use of the VALD database, operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna.
Paper: 2015ApJ...814...57M (acknowledgments)
I thank A. Hamers for providing data from his TPI code that was used in constraining the functional forms of the anomalous diffusion coefficients in Section 2 . This work was supported by the National Science Foundation under grant no. AST 1211602 and by the National Aeronautics and Space Administration under grant no. NNX13AG92G.
Paper: 2017A&A...602A..97R (acknowledgments)
We thank the anonymous referee for the careful reading and helpful suggestions that improved the paper. We would like to thank Louis Ho, Zhao-Yu Li, and the CGS team for kindly providing the , , , luminosity profiles derived form the Carnegie-Irvine Galaxy Survey. Paola Mazzei and Roberto Rampazzo acknowledge support from INAF through grant PRIN-2014-14 “Star formation and evolution in galactic nuclei”. We acknowledge the usage of the HyperLeda database ( http://leda.univ-lyon1.fr ).
Paper: 2017ApJ...843...45K (acknowledgments)
The authors acknowledge support by Allegro, the European ALMA Regional Center node in the Netherlands, and expert advice from Yanett Contreras in particular. This work was supported by the Momentum grant of the MTA CSFK Lendület Disk Research Group. E.V. acknowledges support from the Austrian Science Fund (FWF) under research grant I2549-N27. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00870.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. Facility: ALMA.
Paper: 2019MNRAS.486..320L (acknowledgments)
ACKNOWLEDGEMENTS The authors wish to thank Bernard Delabre and Johan Kosmalski for useful discussions and suggestions.
Paper: 2016MNRAS.461.2025E (acknowledgments)
WE and MJH acknowledge support from the UK's Science and Technology Facilities Council [grant numbers ST/M503514/1 and ST/M001008/1]. This work has made use of the University of Hertfordshire Science and Technology Research Institute high-performance computing facility. This work was supported by funding from Deutsche Forschungsgemeinschaft under DFG project number PR 569/10-1 in the context of the Priority Program 1573 ‘Physics of the Interstellar Medium’. We also thank an anonymous referee for useful and constructive comments that helped improve this paper.
Paper: 2016MNRAS.456.1881L (acknowledgments)
We are grateful to Professor Perivolaropoulos L. for useful comments and suggestions. This work has been funded by the National Natural Science Fund of China under grants Nos. 11375203, 11305181, 11322545, 11335012 and 11575271.
Paper: 2017MNRAS.472.1413A (acknowledgments)
Acknowledgements The authors would like to thank Eric Linder for useful comments and Tamara Davis for many discussions on the content as well as useful comments. The Dark Cosmology Centre was funded by the Danish National Research Foundation.
Paper: 2015MNRAS.453.1371M (acknowledgments)
AVM and CP acknowledge support from the Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (subproject A2) of the German Research Foundation (DFG). We acknowledge the computational support from the THEO and HYDRA clusters of the Max-Planck-Institut für Astronomie at the Rechenzentrum in Garching. SAB thanks the C.I.F.S. (Consorzio Interuniversitario per la Fisica Spaziale) for its financial support.
Paper: 2017ApJ...846..118A (acknowledgments)
The author thanks Hitoshi Miura, Taishi Nakamoto, Satoshi Okuzumi, and Hidekazu Tanaka for valuable comments. The author is also thankful to the anonymous reviewer for constructive comments. This work is supported by the Grant-in-Aid for JSPS Research Fellow (17J06861).
Paper: 2017ApJ...839...93P (acknowledgments)
We thank the anonymous referee for a prompt and constructive report that has improved the paper. Support for HST program GO-12922 was provided by NASA through a grant from the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. D.P. acknowledges support through the EACOA Fellowship from the East Asian Core Observatories Association, which consists of the National Astronomical Observatories, Chinese Academy of Science (NAOC), National Astronomical Observatory of Japan (NAOJ), Korean Astronomy and Space Science Institute (KASI), and Academia Sinica Institute of Astronomy and Astrophysics (ASIAA). Research by A.J.B. is supported in part by National Science Foundation (NSF) grant AST-1412693. JHW acknowledges support by the National Research Foundation of Korea grant funded by the Korean government (No. 2010-0027910 and No. 2016R1A2B3011457). T.T. acknowledges support by the Packard Foundation through a Packard Research Fellowship and by the NSF through grant AST-1412315. V.N.B. gratefully acknowledges assistance from NSF Research at Undergraduate Institutions (RUI) grant AST-1312296. Note that the findings and conclusions do not necessarily represent the views of the NSF. R.J.A. was supported by FONDECYT grant number 1151408. We thank Jonelle L. Walsh for help with the STIS data reduction.
Paper: 2018MNRAS.480L..63S (acknowledgments)
ACKNOWLEDGEMENTS The author thanks the observations provided by the Solar Dynamic Observatory , and the referee’s valuable suggestions and comments that highly improved the quality of the paper. This work is supported by the Natural Science Foundation of China (11773068, 11633008, 11403097, and 11533009), the Yunnan Science Foundation (2015FB191 and 2017FB006), the Specialized Research Fund for State Key Laboratories, and the Youth Innovation Promotion Association (2014047) of Chinese Academy of Sciences.
Paper: 2019ApJ...880..144S (acknowledgments)
We thank the referee for their insightful comments that improved the paper quality. We thank Maïca Clavel for useful discussions about the X-ray data analysis. J.S. and I.O. acknowledge financial support from the Czech Science Foundation project No.17-06217Y. I.O. is grateful to Université Grenoble Alpes IPAG for their hospitality during the paper preparation. We have made use of the SDSS, ADS, and NED databases.
Paper: 2019A&A...629A.109S (acknowledgments)
Acknowledgement We wish to thank L. Fletcher for providing us with the data of HD 189733 b. We acknowledge the support of the DFG priority program SPP-1992 “Exploring the Diversity of ExtrasolarPlanets” (DFG PR 3624 602/41 and RE 1664/16-1). This work made use of the GWDG IT infrastructure. The GWDG is a shared corporate facility of the Georg-August-University Göttingen and the nonprofit Max-Planck Society (Max-Planck Gesellschaft zur Förderung der Wissenschaften e. V.). We also acknowledge the use of electronic databases SIMBAD and NASA’s ADS.
Paper: 2015ApJ...805..182G (acknowledgments)
J.Z.G. and R.P.K. acknowledge support by the National Science Foundation under grant AST-1108906 and the hospitality of the Munich University Observatory where part of this work was carried out. B.D. is supported by a fellowship from the Royal Astronomical Society. B.P. is supported in part by the Programme National de Physique Stellaire of the INSU CNRS. S.J.W. and A.Z.B. acknowledge funding by the European Union (European Social Fund) and National Resources under the ARISTEIA action of the Operational Programme Education and Lifelong Learning in Greece.
Paper: 2017A&A...602A.103W (acknowledgments)
Based on observations made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 60.A-9328 and 091.D-0823. We thank the referee for constructive and pertinent suggestions that helped to improve this paper. N.W., M.C., O.G., D.B., A.G., A.D., and M.M. acknowledge the Centre National d’Etudes Spatiales (CNES) for their support.
Paper: 2017MNRAS.467..290A (acknowledgments)
Acknowledgments MAP was funded by the International Research Fellowship programme of the Japan Society for the Promotion of Science (PE15024). MAP and TMD acknowledge the hospitality of the Kyoto University, where part of this work was carried out. MAP acknowledge the hospitality on her visit to RIKEN, and thanks the valuable discussion with K. Makishima, T. Mihara and the other members of the MAXI team. MAPs research is funded under the Juan de la Cierva Fellowship Programme of the Ministry of Science and Innovation (MINECO) of Spain. MAP and TMD acknowledge support by the Spanish MINECO grant AYA2013-42627. MS acknowledges support by the Special Postdoctoral Researchers Program at RIKEN. This research has made use of data obtained from the Suzaku satellite, a collaborative mission between the space agencies of Japan (JAXA) and the USA (NASA).
Paper: 2017ApJ...843...39A (acknowledgments)
We acknowledge support from the U.S. National Science Foundation (NSF); the U.S. Department of Energy Office of High-Energy Physics; the Laboratory Directed Research and Development (LDRD) program of Los Alamos National Laboratory; Consejo Nacional de Ciencia y Tecnología (CONACyT), México (grants 271051, 232656, 260378, 179588, 239762, 254964, 271737, 258865, 243290, 132197), Laboratorio Nacional HAWC de rayos gamma; L’OREAL Fellowship for Women in Science 2014; Red HAWC, México; DGAPA-UNAM (grants IG100317, IN111315, IN111716-3, IA102715, 109916, IA102917); VIEP-BUAP; PIFI 2012, 2013, PROFOCIE 2014, 2015; the University of Wisconsin Alumni Research Foundation; the Institute of Geophysics, Planetary Physics, and Signatures at Los Alamos National Laboratory; Polish Science Centre grant DEC-2014/13/B/ST9/945; and Coordinación de la Investigación Científica de la Universidad Michoacana. Thanks to Luciano Díaz and Eduardo Murrieta for technical support.
Paper: 2016ApJ...827..113N (acknowledgments)
We are grateful to Dr. Itsuki Sakon, Dr. Chris Packham, Dr. Hiroshi Shibai, Dr. Takao Nakagawa, Dr. Satoshi Okuzumi, and Dr. Inga Kamp for useful comments. We thank the referee for many important suggestions and comments. The numerical calculations in this study were carried out on SR16000 at Yukawa Institute for Theoretical Physics (YITP) and computer systems at Kwasan and Hida Observatory (KIPS) in Kyoto University. This work is supported by Grants-in-Aid for Scientific Research, 23103005, 25108004, 25400229, and 16J06887. S.N. is grateful for the support from the educational program organized by Unit of Synergetic Studies for Space, Kyoto University. C.W. acknowledges support from the Netherlands Organization for Scientific Research (NWO, program number 639.041.335). Astrophysics at Queen’s University Belfast is supported by a grant from the STFC.
Paper: 2016ApJ...823..114N (acknowledgments)
It is a pleasure to thank Maria Bergemann (MPIA) John Bochanski (Rider), Morgan Fouesneau (MPIA), Ricardo Schiavon (Liverpool John Moores University), Dan Foreman-Mackey (UW), Amelia Stutz (MPIA), and Ben Weiner (Arizona State) for valuable discussions and contributions. This project made use of the NASA Astrophysics Data System and open-source code in the numpy and scipy packages. The research has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP 7) ERC Grant Agreement n. [321035]. We thank the Kavali Institute Theoretical Physics Galactic Archeology Program: this research was supported in part by the National Science Foundation under Grant No. NSF PHY11-25915. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the participating institutions, the National Science Foundation, and the U.S. 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, the 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, the University of Portsmouth, Princeton University, the Spanish Participation Group, the University of Tokyo, the University of Utah, Vanderbilt University, the University of Virginia, the University of Washington, and Yale University.
Paper: 2015MNRAS.451.3145Z (acknowledgments)
We would like to thank the anonymous referee for instructive comments. This work is partially supported by the National Natural Science Foundation of China (NSFC 11433004, 11103016, 11173020), the Doctoral Fund of the Ministry of Education of China (RFDP 20115301110005), the Key Project of the Chinese Ministry of Education (212160), the Top Talents Programme of Yunnan Province, the Applied Basic Research Project of Yunnan Province (2011FB012) and the Light of the Western Talent Training Project (W8090303).
Paper: 2015ApJ...815..134H (acknowledgments)
We would like to acknowledge the helpful comments of the anonymous referee, as these greatly helped to improve the manuscript. This work has been supported by NASA EPSCoR grant NNX13AD28A.
Paper: 2017MNRAS.464..794G (acknowledgments)
SG thanks the Science and Technology Facilities Council (STFC) for the award of a studentship. The research leading to these results has received funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement no. 308024 .
Paper: 2018A&A...618A..74U (acknowledgments)
The authors thank the anonymous referee for constructive comments and suggestions. The authors also thank Dr. R. Kale for providing the VLA radio data. I.U. thanks H. Martínez-Rodríguez for his support in the initial stage of this work. H.A. acknowledges the support of NWO via Veni grant. T.O. and Y.I. acknowledge support by JSPS KAKENHI Grant Numbers 26220703 and 15H03642. SRON is supported financially by NWO, the Netherlands Organization for Scientific Research. This work is based on observations obtained with XMM-Newton, an ESA science mission with instruments and contributions directly funded by ESA member states and the USA (NASA).
Paper: 2017ApJ...844...26F (acknowledgments)
I thank the anonymous referee for helpful comments that improved the paper. I also thank Feng Chen and Sarah Gibson for reading the paper and for helpful comments. This work is supported in part by the Air Force Office of Scientific Research grant FA9550-15-1-0030 to NCAR. NCAR is sponsored by the National Science Foundation. The numerical simulations were carried out on the Cheyenne supercomputer at NWSC under the NCAR Strategic capability project NHAO0011 and also on the DOD supercomputers Thunder at AFRL and Topaz at ERDC under the project AFOSR4033B701.
Paper: 2016ApJ...832..133S (acknowledgments)
We acknowledge Susan Agrain, Tim Bedding, Karsten Brogaard, Hans Kjeldsen, Daniel Huber, Marc Pionsonneault, and Jie Yu for fruitful discussions and helpful comments. Funding for the Stellar Astrophysics Centre is provided by The Danish National Research Foundation (Grant DNRF106). The research was supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler ) funded by the European Research Council (Grant agreement No. 267864). D.S. acknowledges support from the Australian Research Council. A.V. is supported by the NSF Graduate Research Fellowship, Grant No. DGE 1144152. V.S.A. acknowledges support from VILLUM FONDEN (research grant 10118).
Paper: 2016MNRAS.456..192Z (acknowledgments)
We thank the US Air Force Research Laboratory, Agence Nationale de la Recherche (ANR-OS-BLAN-0033-01), Conseil des Programmes Scientifiques et Technologiques (CPST) for their great support. We would also like to thank the Polar Institut Paul Emile Victor (IPEV) for the precious infrastructure and friendly help. M. Chadid is indebted to all the people who participated in the Antarctica expeditions within the PAIX framework.
Paper: 2019MNRAS.487.4884I (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank J. Granot, H. Hamidani, K. Hotokezaka, K. Kashiyama, T. Kinugawa, S. Kisaka, K. Kyutoku, G. P. Lamb, A. Levinson, T. Matsumoto, T. Piran, G. Ryan, M. Shibata, K. Takahashi, and R. Yamazaki for useful discussions. This work is partly supported by JSPS KAKENHI nos. 18H01215, 17H06357, 17H06362, 17H06131, 26287051 (KI), and 15H02087 (TN). Discussions during the YITP workshop YITP-W-18-11 on ‘Jet and Shock Breakouts in Cosmic Transients’ and the workshop at Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1607611, were also useful to complete this work.
Paper: 2015A&A...579A.105O (acknowledgments)
This presented work is funded through the DFG grant: WO 857/10-1. Special thanks go to Yaroslav Pavlyuchenkov for his comments and advice, which were very helpful in the early development phase of Mol3D . We also want to acknowledge Peter Scicluna and Tommy Breslein for language editing and Jan Philipp Ruge for the helpful advice, especially regarding the use of the CASA simulator.
Paper: 2017A&A...608A..82F (acknowledgments)
Support for this work was provided by the French space agency CNES. M.P. acknowledges funding from the European Unions Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No. 664931. Support for this work was also provided by NASA ( Herschel OT funding) through an award issued by JPL/Caltech. This paper makes use of Herschel /HIFI data. Herschel is an ESA space observatory with science instruments provided by European-led principal Investigator consortia and with important participation from NASA. 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 U.S. 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 Arcetri-INAF; Netherlands: SRON, TUD; Poland: CAMK, CBK; Spain: Observatorio Astronómico Nacional (IGN), Centro de Astrobiología (CSIC-INTA); Sweden: Chalmers University of Technology-MC2, RSS and GARD, Onsala Space Observatory, Swedish National Space Board, Stockholm Observatory; Switzerland: ETH Zurich, FHNW; USA: Caltech, JPL, NHSC. Finally, we thank the anonymous referee for helpful comments and suggestions.