adsabs/WIESP2022-NER huggingface dataset:
Paper: 2016MNRAS.459.3025P (acknowledgments)
This research was supported by the Victorian Life Sciences Computation Initiative (VLSCI), grant ref. UOM0005, on its Peak Computing Facility hosted at the University of Melbourne, an initiative of the Victorian Government, Australia. Part of this work was performed on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Governments Education Investment Fund. This research programme is funded by the Australian Research Council through the ARC Laureate Fellowship FL110100072 awarded to JSBW. CP acknowledges support of ARC DP130100117 and DP140100198, and ARC Future Fellowship FT130100041. AM acknowledges support from the European Research Council (ERC) under the European Unions Horizon 2020 research and innovation programme (grant agreement no. 638809 AIDA). We thank Volker Springel for making his gadget-2 and subfind codes available to us and Peter Behroozi for making his rockstar code available. We also thank N. Gnedin for several very useful comments on our manuscript.
Paper: 2015ApJ...810....5C (acknowledgments)
We thank the McDonald Observatory staff in West Texas for their hospitality during the observing runs for this research. P. W. C. especially thanks David Doss for his help, without which the collection of some of this data would not have been possible. P. W. C. would also like to acknowledge Pat Hartigan for his comments and discussion throughout this project. We thank the referee for their helpful comments which improved the quality of this manuscript. This research has made use of the SIMBAD database and the NASA Astrophysics Data System. We acknowledge partial support for this research from the NSF through grant 1212122, from NASA Astrophysics Data Analysis Program through grant NNX13AF09G, and from Space Telescope Science Institute through grant HST-60-12996.001, all made to Rice University.
Paper: 2016A&A...595A..32B (acknowledgments)
The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. We like to thank Juan Pablo Perez-Beaupuits for providing the ionized, atomic, and molecular data of M17 presented in Fig. 13 . H.B. acknowledges support from the European Research Council under the Horizon 2020 Framework Program via the ERC Consolidator Grant CSF-648505. R.S.K. and S.C.O.G. acknowledge support from the European Research Council via the ERC Advanced Grant STARLIGHT (project number 339177). R.S.K. and S.C.O.G. furthermore thank for financial help from the DFG via SFB 881 “The Milky Way System” (subprojects B1, B2, and B8) and SPP 1573 “Physics of the Interstellar Medium”.
Paper: 2019MNRAS.483..664M (acknowledgments)
ACKNOWLEDGEMENTS We thank Javier Román and Raúl Infante for providing the extended SDSS r -band PSF, and Sebastién Comerón for a number of useful suggestions. We acknowledge support from the Spanish Ministry of Economy and Competitiveness (MINECO) under grant numbers AYA2013-41243-P, AYA2016-76219-P and AYA2016-77237-C3-1-P. J.H.K. and I.T.C. acknowledge financial support from the European Union’s Horizon 2020 research and innovation programme under Marie Skłodowska-Curie grant agreement No. 721463 to the SUNDIAL ITN network and from the Fundación BBVA under its 2017 programme of assistance to scientific research groups, for the project ‘Using machine-learning techniques to drag galaxies from the noise in deep imaging’. J.H.K. thanks the Leverhulme Foundation for the award of a Visiting Professorship at Liverpool John Moores University. 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. 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, University of Cambridge, 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, 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. This work is based on archival data from the Spitzer Space Telescope available in 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. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non- HST data is provided by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts.This research has made use of different Python packages and of NASA’s Astrophysics Data (NED) System Bibliographic Services, which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautic and Space Administration. We acknowledge constructive remarks by an anonymous referee.
Paper: 2017MNRAS.472.1226D (acknowledgments)
Acknowledgements I thank David M. Hernandez for a critical reading and Scott Tremaine for useful conversations on symplecticity and time symmetry. WD is partly supported by STFC grant ST/N000757/1.
Paper: 2019MNRAS.487..253D (acknowledgments)
ACKNOWLEDGEMENTS We greatly appreciate valuable comments from Christopher M. Hirata and Patrick Mcdonald. We also thank Tim Eifler for providing the source galaxy redshift information for the PWL-Stage III and IV surveys adopted in this work. ZD, DC, and H-JS are supported by the U.S. Department of Energy, Office of Science,Office of High Energy Physics under Award Number DE-SC0014329. SS was supported in part by JSPS KAKENHI Grant Number JP15H05896 and by World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan. This research used the DESI allocation resources of the National Energy Research Scientific Computing Center (NERSC), a U.S. Department of Energy Office of Science User Facility operated under Contract No. DE-AC02-05CH11231.
Paper: 2017ApJ...837...14A (acknowledgments)
This work was supported by grant GO6-17005X from the Smithsonian Astrophysical Observatory, based on observations from the Chandra X-ray Observatory, collected and processed at the Chandra X-ray Center, operated by SAO under contract to NASA; and grants GO-14349 ( α Per) and GO-12278 (Advanced Spectral Library [ASTRAL]: Cool Stars) from the Space Telescope Science Institute, based on observations from Hubble Space Telescope collected at STScI, operated by the Associated Universities for Research in Astronomy, also under contract to NASA. Ground-based observations were obtained with the Apache Point Observatory 3.5 m telescope, operated by the Astrophysical Research Corporation. Dr. Carol Grady guided the APO/GIFS imaging, and generously contributed time for the project out of her engineering allocation. This study also made use of public databases hosted by SIMBAD, maintained by CDS, Strasbourg, France; the Mikulski Archive for Space Telescopes at STScI in Baltimore, Maryland; and the High Energy Astrophysics Science and Research Center at the NASA Goddard Space Flight Center, in Greenbelt, Maryland. Additionally, this work has made use of data from the European Space Agency (ESA) mission Gaia ( http://www.cosmos.esa.int/gaia ), processed by the Gaia Data Processing and Analysis Consortium (DPAC, http://www.cosmos.esa.int/web/gaia/dpac/consortium ). Funding for the DPAC has been provided by national institutions, in particular those participating in the Gaia Multilateral Agreement.
Paper: 2019MNRAS.485.4625B (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for her/his comments and suggestions that improved the quality of the paper. We thank Karin Lind and Henrique Reggiani for helpful discussions on this work. Our work has been supported by The Scientific and Technological Research Council of Turkey (TÜBİTAK, project No. 116F407), by the US National Science Foundation (NSF, grant AST 16-16040), and by the University of Texas Rex G. Baker, Jr. Centennial Research Endowment. This work used the Immersion Grating Infrared Spectrometer (IGRINS) that was developed under a collaboration between the University of Texas at Austin and the Korea Astronomy and Space Science Institute (KASI) with the financial support of the US National Science Foundation under grant AST-1229522, of the University of Texas at Austin, and of the Korean GMT Project of KASI. 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. This research has made use of NASA’s Astrophysics Data System Bibliographic Services; the SIMBAD database and the VizieR service, both operated at CDS, Strasbourg, France. This research has made use of the WEBDA database, operated at the Department of Theoretical Physics and Astrophysics of the Masaryk University, and the VALD database, operated at Uppsala University, the Institute of Astronomy RAS in Moscow, and the University of Vienna. This paper includes data taken at The McDonald Observatory of The University of Texas at Austin.
Paper: 2017MNRAS.469S.238L (acknowledgments)
Acknowledgements Optical, Spectroscopic and Infrared Remote Imaging System (OSIRIS) was built by a consortium of the Max-Planck-Institut für Sonnensystemforschung, in Göttingen, Germany, CISAS-University of Padova, Italy, the Laboratoire d’Astrophysique de Marseille, France, the Instituto de Astrofisica de Andalucia, CSIC, Granada, Spain, the Research and Scientific Support Department of the European Space Agency, Noordwijk, the Netherlands, the Instituto Nacional de Tecnica Aeroespacial, Madrid, Spain, the Universidad Politechnica de Madrid, Spain, the Department of Physics and Astronomy of Uppsala University, Sweden and the Institut für Datentechnik und Kommunikationsnetze der Technischen Universität Braunschweig, Germany. The support of the national funding agencies of Germany (DLR), Italy (ASI), France (CNES), Spain (MEC), Sweden (SNSB) and the ESA Technical Directorate is gratefully acknowledged. We thank the ESA teams at ESAC, ESOC and ESTEC for their work in support of the Rosetta mission. We made use of the arcgis 10.2 software together with idl and matlab software to perform the presented analysis.
Paper: 2018MNRAS.477.2164P (acknowledgments)
ACKNOWLEDGEMENTS This publication 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. We thank the referee for his/her thorough reading of the manuscript and timely suggestions to improve it.
Paper: 2019MNRAS.487.5272J (acknowledgments)
ACKNOWLEDGEMENTS We acknowledge stimulating discussions with Frank van den Bosch, Adi Nusser, Shany Danieli, Yuval Birnboim, Elad Zinger, and Nicolas Cornuault. We thank the editor and the anonymous referee for helping to make the paper more rounded. This work was partly supported by the grants ISF 124/12, I-CORE Program of the PBC/ISF 1829/12, BSF 2014-273, PICS 2015-18, and NSF AST-1405962. FJ is partly supported by the PBC Fellowship. AJR was supported by National Science Foundation (NSF) grant AST-1616710, and as a Research Corporation for Science Advancement Cottrell Scholar. ADC acknowledges financial support from a Marie-Skłodowska-Curie Individual Fellowship grant, H2020-MSCA-IF-2016 Grant agreement 748213 DIGESTIVO. The simulations were performed on the High Performance Computing resources at New York University Abu Dhabi; on the THEO cluster of the Max Planck Institute fr Astronomie and on the HYDRA clusters at the Rechenzentrum in Garching.
Paper: 2015A&A...577A..99N (acknowledgments)
We warmly thank A. K. Vivas for useful discussions and information regarding her team’s variability search around Cen. We also thank the anonymous referee for useful comments that helped improve the presentation of our results. Support for this project is provided by the Ministry for the Economy, Development, and Tourism’s Programa Iniciativa Científica Milenio through grant IC 120009, awarded to the Millennium Institute of Astrophysics (MAS); by Proyecto Basal PFB-06/2007; and by FONDECYT grants #1141141 (C.N., F.G., M.C.), #1130196 (F.G., D.M.), #3130320 (R.C.R.), and #3130552 (J.A.-G.). C.N. and F.G. acknowledge additional support from CONICYT-PCHA/Magíster Nacional (grants 2012-22121934 and 2014-22141509, respectively).
Paper: 2015ApJ...804...69Y (acknowledgments)
The authors thank the anonymous referee for helpful comments on the manuscript. Hinode is a Japanese mission developed and launched by ISAS/JAXA, with NAOJ as domestic partner and NASA and STFC (UK) as international partners. It is operated by these agencies in co-operation with ESA and NSC (Norway). L.-M. Yan thanks H. Peter, Y. Chen, B. Li, L.-P. Yang, and L. Zhang for helpful discussion. The group from Shandong University was supported by grants NSBRSF 2012CB825601 and NNSFC 41274178. The group from Peking University was supported by NNSFC under 41174148, 40890162, and 40931055.
Paper: 2016MNRAS.455.4295G (acknowledgments)
This project has received funding from the European Research Council (ERC) under the European Union's Horizon 2020 research and innovation programme (grant agreement No 638809 – AIDA). J.C.P. is supported by an NSF Astronomy and Astrophysics Fellowship under award AST-1302774.
Paper: 2019MNRAS.485.4330K (acknowledgments)
ACKNOWLEDGEMENTS This paper uses observations made at the South African Astronomical Observatory; is based partly upon work supported financially by the University of the Western Cape and the National Research Foundation of South Africa; and has made use of the SIMBAD data base operated at the Centre de Données astronomiques de Strasbourg (CDS) in Strasbourg, France. We are grateful to the referee, Prof. M.D. Reed, for comments which have enabled the authors to improve this paper.
Paper: 2018A&A...614A..53R (acknowledgments)
Acknowledgements This research has made use of the high performance computing cluster at the Abdus Salam Centre for Physics, Pakistan and the supercomputer Leftraru, Chile. The first author (R.R.) gratefully acknowledges support from the Department of Astronomy, University of Concepcion, Chile. The first author R.R. and third author D.R.G.S. are thankful for funding through the “Concurso Proyectos Internacionales de Investigación, Convocatoria 2015” (project code PII20150171). D.R.G.S. is further thankful for funding via Fondecyt regular (project code 1161247) and via the Chilean BASAL Centro de Excelencia en Astrofísica yTecnologías Afines (CATA) grant PFB-06/2007, and ALMA-Conicyt project (proyecto code 31160001). The second author (S.V.) developed the computer code that has been used in this work on the HPC system Thinking at KU Leuven, which is part of the infrastructure of the FSC (Flemish Supercomputing Center). We thank the KU leuven support team for helping with the use of this system. The second author also gratefully acknowledges the support of Prof. Dr. Stefaan Poedts and Prof. Dr. Rony Keppens for having provided both access and funding, which made the use of the KU Leuven HPC infrastructure possible.
Paper: 2015ApJ...798...78C (acknowledgments)
We thank Vicky Kaspi and Sterl Phinney for helpful comments on the manuscript. This work was supported in part by NSF grant AST-1312034.
Paper: 2019ApJ...885...76P (acknowledgments)
We thank I. Liodakis and A. Marsher for helpful discussions of jet polarization physics. This work was supported in part by NASA grant NNM17AA26C.
Paper: 2015MNRAS.454.3366Z (acknowledgments)
AZ acknowledges funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement no. 617001. NDK acknowledges partial support by the ‘RoboPol’ project, which is implemented under the ‘ARISTEIA’ Action of the ‘Operational Program Education and Lifelong Learning’ and is co-funded by the European Social Fund (ESF) and National Resources. This research has made use of NASA's Astrophysics Data System. This research has made use of data and/or software provided by the High Energy Astrophysics Science Archive Research Center (HEASARC), which is a service of the Astrophysics Science Division at NASA/GSFC and the High Energy Astrophysics Division of the Smithsonian Astrophysical Observatory.
Paper: 2020A&A...633A.127F (acknowledgments)
The authors acknowledge the referee for his/her useful comments that helped to improve the manuscript. JAFO acknowledges financial support by the Agenzia Spaziale Italiana (ASI) under the research contract 2018-31-HH.0. JAFO and KMD acknowledge financial support by the Hellenic Foundation for Research and Innovation (HFRI), under the first call for the creation of research groups by postdoctoral researchers that was launched by the General Secretariat For Research and Technology (project number 1882). MPS acknowledges support from the Comunidad de Madrid, Spain, through Atracción de Talento Investigador Grant 2018-T1/TIC-11035 and STFC through grants ST/N000919/1 and ST/N002717/1. CR acknowledges support from the CONICYT+PAI, Convocatoria Nacional subvención a instalación en la academia, convocatoria año 2017 PAI77170080. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2017.1.00236.S. ALMA is a partnership of ESO (representing its member states), NSF (USA) and NINS (Japan), together with NRC (Canada), MOST 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 National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2018A&A...617A..90L (acknowledgments)
I sincerely thank Pavel Naselsky, Sebastian von Hausegger and James Creswell for valuable discussions and suggestions, as well as the anonymous referee for carefully reading the article and giving very helpful comments. This research has made use of data/product from the WMAP (The WMAP data release 2013) and Planck (The Planck data release 2015) collaborations. Some of the results in this paper are derived using the HEALPix ( Górski et al. 2005 ) package. This work was partially funded by the Danish National Research Foundation (DNRF) through establishment of the Discovery Center and the Villum Fonden through the Deep Space project. Hao Liu is also supported by the Youth Innovation Promotion Association, CAS.
Paper: 2015ApJ...810...81T (acknowledgments)
The material is based upon work supported by the National Aeronautics and Space Administration under Prime Contract Number NAS2-03144 awarded to the University of California, Santa Cruz, University Affiliated Research Center. This work was supported in part by the National Aeronautics and Space Administration's Ames Research Center under a center investment fund. It was carried out at the NASA Ames Research Center. Any opinions, findings, and conclusions or recommendations expressed in this article are those of the authors and do not necessarily reflect the views of the National Aeronautics and Space Administration.
Paper: 2018ApJ...859...34O (acknowledgments)
The authors thank the anonymous referee for insightful comments that greatly improved this paper. We also thank Peter Gao and Diana Powell for providing paper manuscripts, and Shigeru Ida, Hidekazu Tanaka, Xi Zhang, Chris Ormel, Ryo Tazaki, Yamira Miguel, Masahiro Ogihara, Yuichi Ito, and Yui Kawashima for helpful comments. This work was supported by JSPS Grants-in-Aid for Scientific Research (#15H02065, 16H04081, 16K17661, 18J14557) and the Foundation for Promotion of Astronomy.
Paper: 2016ApJ...829...24V (acknowledgments)
SDO is a mission of NASA's Living With a Star Program. This work used the DAVE4VM code, written and developed by P.W. Schuck at the Naval Research Laboratory. 3D rendering is due to VAPOR ( www.vapor.ucar.edu ) software. The authors sincerely thank Dr. T. Wiegelmann for providing NLFFF code. We acknowledge an extensive usage of the multi-node, multi-processor high performance computing facility at IIA. PV is supported by an INSPIRE grant of AORC scheme under the Department of Science and Technology. XC is supported by NSFC under grants 11303016. We thank the referee for constructive comments and suggestions that greatly helped to improve the manuscript.
Paper: 2016MNRAS.455.3136M (acknowledgments)
We are grateful to the S 3 -SAX and HIPASS collaborations. SAM wishes to thank Stefan Westerlund, Laura Hoppmann, Jacinta Delhaize, Matthew Pearce, Rebecca Lange and Angus Wright for coding assistance and Taylem Frost for editorial work. We acknowledge use of the topcat software package ( http://www.star.bristol.ac.uk/∼mbt/topcat/ ) and miriad (Sault 1995 ) for data reduction. This research was conducted by the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020.
Paper: 2015MNRAS.449.2472B (acknowledgments)
The JCMT is operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the UK, the National Research Council of Canada and (until 2013 March 31) the Netherlands Organisation for Scientific Research. Additional funds for the construction of SCUBA-2 were provided by the Canada Foundation for Innovation. DJ is supported by the National Research Council of Canada and by a Natural Sciences and Engineering Research Council of Canada (NSERC) Discovery Grant. This publication 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.
Paper: 2016ApJ...826..197F (acknowledgments)
The research of V.F. and J.H. was supported by NASA grants NNX12AH44G, NNX13AF99G, NNX14AF43G, NNX14AJ53G, and NNX14AP24G, and by NSF grant AGS-0955700. Resources supporting this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center. The work of J.N. was supported by Narodowe Centrum Nauki through research project DEC-2013/10/E/ST9/00662. The authors thank P.A. Isenberg, K.-I. Nishikawa, G.P. Zank, and E.J. Summerlin for helpful discussions.
Paper: 2016ApJ...821...41L (acknowledgments)
H.B.L. is grateful for support from ASIAA. We are extremely grateful to our referee Charles Hull,for the very useful comments. H.B.L. thanks Dr. Steve Myers for the information about polarization calibration sources, and thanks Drs. Akimasa Kataoka, Francisca Kemper, Hiroyuki Hirashita, and Michihiro Takami for useful suggestions. N.H. is supported by the MoST grant 104-2119-M-001-016. J.M.G. acknowledges support from the MICINN (Spain) AYA2014-57369-C3-1-P grant and the MECD (Spain) PRX15/00435 travel grant. C.C.-G. acknowledges support by UNAM-DGAPA-PAPIIT, grant number IA101214. Y.H. is currently supported by JPL/Caltech. Facilities: EVLA , SMA .