adsabs/WIESP2022-NER huggingface dataset:
Paper: 2017ApJ...849....8M (acknowledgments)
U.M. and H.B.P. acknowledge support from the Marie Curie FP7 career integration grant “GRAND,” the Research Cooperation Lower Saxony-Israel Niedersachsisches Vorab fund, the Minerva center for life under extreme planetary conditions and the ISF I-CORE grant 1829/12.
Paper: 2020MNRAS.491.4194L (acknowledgments)
ACKNOWLEDGEMENTS The authors are grateful to the anonymous referee whose comments and suggestions helped to significantly improve the manuscript.
Paper: 2020MNRAS.491.3523B (acknowledgments)
ACKNOWLEDGEMENTS This research is supported by the I-CORE program of the Planning and Budgeting Committee (grant 1937/12), and was performed in part at Aspen Center for Physics, which is supported by National Science Foundation grant PHY-1607611. We thank an anonymous referee for useful comments.
Paper: 2017ApJ...851...33P (acknowledgments)
We are thankful to the journal referee for constructive comments. We are also grateful to the Fermi -LAT Collaboration internal referee Rodrigo Nemmen for useful suggestions and Philippe Bruel, Elizabetta Cavazzutti, Sara Cutini, Seth Digel, Alberto Domínguez, Marcello Giroletti, and Dave Thompson for critical reading of the manuscript. 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 NASA and the Department of Energy in the United States, the Commissariat à l’Energie Atomique and Centre National de la Recherche Scientifique/Institut National de Physique Nucléaire et de Physique des Particules in France, the Agenzia Spaziale Italiana and 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, Swedish Research Council, and 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 performed in part under DOE Contract DE-AC02-76SF00515. This research has made use of data obtained through the High Energy Astrophysics Science Archive Research Center Online Service, provided by the NASA/Goddard Space Flight Center. Part of this work is based on archival data, software, or online services provided by the ASI Data Center (ASDC). This research has made use of the XRT Data Analysis Software (XRTDAS). 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 NASA. The scientific results reported in this article are based on data obtained from the Chandra Data Archive. This research has made use of software provided by the Chandra X-ray Center (CXC) in the application packages CIAO, ChIPS, and Sherpa. 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 NASA. Software: SAS (v15.0.0), fermiPy (Wood et al. 2017 ), XSPEC (Arnaud 1996 ), Swift-XRT data product generator (Evans et al. 2009 ), CIAO (v.4.9).
Paper: 2018A&A...609L...3S (acknowledgments)
Acknowledgements JDS acknowledges the support from the European Research Council (ERC) under the Horizon 2020 Framework Program via the Consolidator Grant CSF-648505. AB acknowledges the support from the ERC Advanced Grant ORISTARS under the European Union’s Seventh Framework Programme (Grant 291294). AP was partly funded by a Canadian Institute for Theoretical Astrophysics (CITA) National Fellowship. We thank the referee M. Alves for her constructive comments that have led to improvements in this presentation of our results. Thanks to M. Houde and S. Basu for their comments on the early versions of this work. We also thank the following people who helped with their encouragement and conversation: P. G. Martin, H. Beuther, C. Heiles, T. Robishaw, M.-A. Miville-Deschênes, and A. Roy. Special thanks go to Thomas Müller at the Haus der Astronomie for his assistance in the magnetic field visualization.
Paper: 2015A&A...575A..39M (acknowledgments)
Research at Armagh Observatory is a grant aided by the N. Ireland Department of Culture, Arts and Leisure. M.M. is funded by the Leverhulme trust. We thank Richard Harrison for important discussion and an anonymous referee for insightful comments. M.M. thanks Kamalam Vanninathan, Astrid Veronig and Zhenghua Huang for fruitful discussions on this manuscript. We are grateful to Vasyl Yurchyshyn for providing us with the BBSO images. We thank STFC for the support via ST/J001082/1.
Paper: 2017MNRAS.470..372O (acknowledgments)
Acknowledgments GDS and MO'D are partially supported by Department of Energy grant DE-SC0009946 to the particle astrophysics theory group at CWRU. MO'D is partially supported by the CAPES Foundation of the Ministry of Education of Brazil. Some of the results in this paper have been derived using the healpix (Górski et al. 2005 ) package. This work made use of the High Performance Computing Resource in the Core Facility for Advanced Research Computing at Case Western Reserve University.
Paper: 2016A&A...594A..28P (acknowledgments)
The Planck Collaboration acknowledges the support of: ESA; CNES and CNRS/INSU-IN2P3-INP (France); ASI, CNR, and INAF (Italy); NASA and DoE (USA); STFC and UKSA (UK); CSIC, MINECO, J.A., and RES (Spain); Tekes, AoF, and CSC (Finland); DLR and MPG (Germany); CSA (Canada); DTU Space (Denmark); SER/SSO (Switzerland); RCN (Norway); SFI (Ireland); FCT/MCTES (Portugal); ERC and PRACE (EU). A description of the Planck Collaboration and a list of its members, indicating which technical or scientific activities they have been involved in, can be found at http://www.cosmos.esa.int/web/planck/planck-collaboration
Paper: 2015MNRAS.451.2978C (acknowledgments)
We acknowledge valuable communications and discussions with F. Bouchet, C. Burigana, J. Dunkley, G. Efstathiou, K. Ganga, P. Naselsky, H. Peiris, C. Räth and D. Scott. GDS and CJC are supported by a grant from the US Department of Energy to the Particle Astrophysics Theory Group at CWRU. DH has been supported by the DOE, NSF, and the Michigan Center for Theoretical Physics. DJS is supported by the DFG grant RTG 1620 ‘Models of gravity’. DH thanks the Kavli Institute for Theoretical Physics and GDS thanks the Theory Unit at CERN for their respective hospitality. This work made extensive use of the healpix package (Górski et al. 2005 ). The numerical simulations were performed on the facilities provided by the Case ITS High Performance Computing Cluster. We acknowledge the use of the Legacy Archive for Microwave Background Data Analysis (LAMBDA), part of the High Energy Astrophysics Science Archive Center (HEASARC). HEASARC/LAMBDA is a service of the Astrophysics Science Division at the NASA Goddard Space Flight Center. This paper made use of observations obtained with Planck ( http://www.esa.int/Planck ), an ESA science mission with instruments and contributions directly funded by ESA Member States, NASA, and Canada.
Paper: 2018MNRAS.476.5548K (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by NASA Astrophysics Theory Program grant NNX13AG61G and the International Space Science Institute in Bern. SH was supported by Japan JSPS KAKENH 15K05040 and the joint research project of ILE, Osaka University. The radiation MHD simulation was partly carried out on the Cray XT4 at CfCA, National Astronomical Observatory of Japan, and on SR16000 at YITP in Kyoto University.
Paper: 2018ApJ...864...48C (acknowledgments)
E.W.C. thanks Karel Schrijver and Jürg Beer for organizing a series of stimulating ISSI Team meetings on extreme solar events, and Ian Richardson for sharing results in advance of publication. E.D. acknowledges support from the Belgian Federal Science Policy Office (BELSPO) through the ESA-PRODEX programme, grant No. 4000120800.
Paper: 2018MNRAS.477.2020C (acknowledgments)
ACKNOWLEDGEMENTS This publication makes use of vosa , developed under the Spanish Virtual Observatory project supported from the Spanish MICINN through grant AyA2011-24052. This research has made use of the SIMBAD data base and VizieR catalogue access tool, operated at CDS, Strasbourg, France. This is based on observations made with the CAOS operated by the Catania Astrophysical Observatory.
Paper: 2019MNRAS.490.3309M (acknowledgments)
ACKNOWLEDGEMENTS 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, Bruyg̀resle-Chåtel. We would like to thank Claudio Dalla Vecchia for the kind help with the data handling. We also thank Romeel Davé for providing the simba simulation data and for his help in interpreting them, and the CANDELS team for providing the latest available data.
Paper: 2017A&A...605A..39T (acknowledgments)
This work was supported by the Russian Science Foundation grant 14-12-01287 (S.S.T., A.A.L., A.A.M.), the Foundations’ Professor Pool, the Finnish Cultural Foundation and the Academy of Finland grant 268740 (J.P.). We also acknowledge the support from the COST Action MP1304.
Paper: 2018MNRAS.473.4523W (acknowledgments)
Acknowledgements We thank L. Dunne and S. Maddox for hosting the author and for initial advice at the University of Canterbury and subsequent helpful discussions. Stuart Weston is a recipient of a CSIRO Astronomy and Space Science, Australia Telescope National Facility Graduate Research Scholarship. Nicholas Seymour is the recipient of an Australian Research Council Future Fellowship. Mattia Vaccari acknowledges support from the European Commission Research Executive Agency (FP7-SPACE-2013-1 GA 607254), the South African Department of Science and Technology (DST/CON 0134/2014) and the Italian Ministry for Foreign Affairs and International Cooperation (PGR GA ZA14GR02). We thank the referee, Jim Condon, for critically reading the manuscript and suggesting substantial improvements which have significantly improved the paper.
Paper: 2018MNRAS.479.5696K (acknowledgments)
ACKNOWLEDGEMENTS WEK was supported by an ESO Fellowship and the Excellence Cluster Universe, Technische Universität München, Boltzmannstrasse 2, D-85748 Garching, Germany. Support for program #13432 was provided to KSL and PFW by NASA through grant HST -GO-13432 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. PFW acknowledges additional support from the NSF through grant AST-1714281. We would like to acknowledge the detailed discussions and input from Marten van Kerkwijk and Kim Venn during the preparation of the HST proposal that led to the observations reported here. We would like to acknowledge the helpful comments by our referee.
Paper: 2015A&A...584A.110P (acknowledgments)
We thank an anonymous referee for his useful comments and suggestions. G. Picogna acknowledges the support through the German Research Foundation (DFG) grant KL 650/21 within the collaborative research program “The first 10 Million Years of the Solar System”. Some simulations were performed on the bwGRiD cluster in Tübingen, which is funded by the Ministry for Education and Research of Germany and the Ministry for Science, Research and Arts of the state Baden-Württemberg, and the cluster of the Forschergruppe FOR 759 “The Formation of Planets: The Critical First Growth Phase” funded by the DFG.
Paper: 2020A&A...634L...2S (acknowledgments)
The authors would like to thank Mayte Alfaro Cuello, Moritz Reichert and Thomas de Boer for readily sharing their results with us. 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. 804240).
Paper: 2015ApJ...809...77S (acknowledgments)
We are grateful to the referee, Scott Gaudi, for providing constructive criticism that has led to improvements in this paper. We thank the members of the TESS Science Team for their contributions to the mission. In particular, Jacob Bean, Tabetha Boyajian, Eric Gaidos, Daniel Huber, Geoffrey Marcy, Roberto Sanchis-Ojeda, and Keivan Stassun provided helpful comments on the manuscript, and discussions with Jon Jenkins helped inform our approach to the simulations. We acknowledge Anthony Smith, Kristin Clark, and Michael Chrisp at MIT-Lincoln Laboratory for their respective roles in the project management, systems engineering, and optical design for the TESS payload. In addition, Barry Burke and Vyshnavi Suntharalingam at MIT-LL provided useful input to the PSF model. We thank Leo Girardi for adding the TESS bandpass to the TRILEGAL simulation and for providing a perl script to facilitate the queries. We also thank Gibor Basri for sharing the stellar variability data from Kepler . This publication makes use of data products from the 2MASS, 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: 2015ApJ...812...75G (acknowledgments)
We acknowledge helpful comments and suggestions from our referee. We thank Spanish MINECO for funding support under grants CSD2009-00038, AYA2009-07304, and AYA2012-32032. We also thank the ERC for support under grant ERC-2013-Syg-610256-NANOCOSMOS. Part of this research was carried out at the Jet Propulsion Laboratory (JPL), California Institute of Technology (Caltech), under a contract with the National Aeronautics and Space Administration (NASA). Support for this work was provided by NASA through an award issued by JPL/Caltech. This work was supported by the German Deutsche Forschungsgemeinschaft, DFG project number SFB 956, C1. This work was in part also supported by theCNRS program “Physique et Chimie du Milieu Interstellaire (PCMI).” Facilities: Herschel Space Observatory , IRAM:30m.
Paper: 2018ApJ...854..128S (acknowledgments)
M.Y.S. thanks K. D. Denney for a beneficial discussion. We thank the anonymous referee for helpful comments that improved the paper. M.Y.S. and Y.Q.X. acknowledge the support from NSFC-11603022, NSFC-11473026, NSFC-11421303, the 973 Program (2015CB857004), the China Postdoctoral Science Foundation (2016M600485), the CAS Frontier Science Key Research Program (QYZDJ-SSW-SLH006), and the Fundamental Research Funds for the Central Universities. W.N.B. acknowledges support from NSF Grant AST-1516784 and Chandra X-ray Center grant GO6-17083X. 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 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. Software: Astropy (Astropy Collaboration et al. 2013 ), Kapteyn (Terlouw Vogelaar 2015 ), Matplotlib (Hunter 2007 ), Numpy Scipy (Van Der Walt et al. 2011 ).
Paper: 2018ApJ...853...10L (acknowledgments)
The authors are very grateful to Stephen Bougher for generously providing access to the M-GITM model, and acknowledge valuable discussions with Andrew Knoll, Janet Luhmann, Michael Summers, Lei Dai, Takuya Shibayama, and David Pawlowski. The detailed and insightful report furnished by the referee is also much appreciated. M.L. and A.L. were partly supported by grants from the Breakthrough Prize Foundation for the Starshot Initiative and Harvard University’s Faculty of Arts and Sciences, and by the Institute for Theory and Computation (ITC) at Harvard University. C.D. was supported by the NASA Living With a Star Jack Eddy Postdoctoral Fellowship Program, administered by the University Corporation for Atmospheric Research. X.F. and B.M.J. acknowledge support from NASA’s MAVEN mission. Resources for this work were provided by the NASA High-End Computing (HEC) Program through the NASA Advanced Supercomputing (NAS) Division at Ames Research Center.
Paper: 2019A&A...631A..36D (acknowledgments)
FD is indebted to the ScaLAPACK team for both the provision of their libraries and their responses to numerous questions. FD thanks the European Research Council (ERC) for funding under the H2020 research innovation programme (grant agreement #740651 NewWorlds). NJM is part funded by a Leverhulme Trust Research Project Grant and partly supported by a Science and Technology Facilities Council Consolidated Grant (ST/R000395/1), both of which we gratefully acknowledge. This study uses material produced using Met Office Software. Additionally, used the DiRAC Complexity system, operated by the University of Leicester IT Services, which forms part of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment is funded by BIS National E-Infrastructure capital grant ST/K000373/1 and STFC DiRAC Operations grant ST/K0003259/1. DiRAC is part of the National e-Infrastructure. Additionally, this research made use of the ISCA High Performance Computing Service at the University of Exeter. Finally, this work was also partly funded by the ERC grant No. 320478-TOFU.
Paper: 2016A&A...596A..21I (acknowledgments)
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. This research has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The High-Energy Astrophysics Group of Palermo acknowledges support from the Fondo Finalizzato alla Ricerca (FFR) 2012/13, project No. 2012-ATE-0390. We also acknowledge a financial contribution from the agreement ASI-INAF I/037/12/0. M.D.S. thanks the Dipartimento di Fisica e Chimica, Università di Palermo, for its hospitality. A.R. and A.S. gratefully acknowledge the Sardinia Regional Government for its financial support (P.O.R. Sardegna F.S.E. Operational Programme of the Autonomous Region of Sardinia, European Social Fund 2007-2013 – Axis IV Human Resources, Objective l.3, Line of Activity l.3.1.). A.P. acknowledges grant SGR2014-1073 and partial support from “NewCompStar”, COST Action MP1304. A.P. acknowledges support via an EU Marie Skłodowska-Curie fellowship under grant No. 660657-TMSP-H2020-MSCA-IF-2014, as well as fruitful discussion with the international team on “The diskmagnetosphere interaction around transitional millisecond pulsars” at ISSI (International Space Science Institute), Bern.
Paper: 2017MNRAS.466..780M (acknowledgments)
We thank Matias Zaldarriaga for useful discussions. US acknowledges support from NASA grant NNX15AL17G. ZV is supported in part by the U.S. Department of Energy contract to SLAC no. DE-AC02-76SF00515. IM is supported by Fermi Research Alliance, LLC under Contract No. De-AC02-07CH11359 with the United States Department of Energy.
Paper: 2020MNRAS.492.4591J (acknowledgments)
ACKNOWLEDGEMENTS We acknowledge financial support from the national programs (PNP, PNPS, PCMI) of INSU, CNRS, CEA, and CNES, France. This project was partly supported by the IDEXLyon project (contract nANR-16-IDEX-0005) under the auspices University of Lyon. This project has received funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement No 823823. This work has received funding from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme (grant agreement ERC advanced grant 740021-ARTHUS, PI: Thomas Buchert). We thank the referee for his constructive report. We have used mathematica (Wolfram Research 14 ).
Paper: 2019A&A...623A..87N (acknowledgments)
Both BN and MS acknowledge the financial support and hospitality provided by the European Southern Observatory (ESO) through the award of an ESO studentship and visiting fellowship, respectively. EMC, EDB, LM, and AP acknowledge financial support from Padua University through grants DOR1699945/16, DOR1715817/17, DOR1885254/18, and BIRD164402/16.
Paper: 2018MNRAS.479.4907D (acknowledgments)
ACKNOWLEDGEMENTS Parts of this research were conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. The authors would also like to thank referee Santiago García-Burillo, who provided valuable input and helped improve the condition of the publication.
Paper: 2018MNRAS.480.5529G (acknowledgments)
ACKNOWLEDGEMENTS We thank Matthias Bartelmann for helpful comments on this analysis and for acting as the external blinder for the KiDS-450 data. We are also very grateful to Mike Jarvis for the treecorr correlation function measurement software and Martin Kilbinger for the nicaea theoretical modelling software. We are thankful to Vasiliy Demchenko, Naomi Robertson, Shahab Joudaki, Laura Jean Wells, and members of the KiDS consortium for useful discussions. We extend our gratitude to the anonymous referee for their comments which improved this paper. BG, CH, JHD, AA, MA, and TT acknowledge support from the European Research Council under grant number 647112. JHD also acknowledges support from the European Commission under a Marie-Sklodwoska-Curie European Fellowship (EU project 656869). LvW is supported by NSERC of Canada. HH is supported by an Emmy Noether grant (No. Hi 1495/2-1) of the Deutsche Forschungsgemeinschaft. KK acknowledges support from the Alexander von Humboldt Foundation. PS acknowledges support from the Deutsche Forschungsgemeinschaft in the framework of the TR33 ‘The Dark Universe’. TT acknowledges funding from the European Union’s Horizon 2020 research and innovation programme under the Marie Sklodowska-Curie grant agreement number 797794. This KiDS data are based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme IDs 177.A-3016, 177.A-3017, and 177.A-3018. Computations for the SLICS N -body simulations (now publicly available; http://slics.roe.ac.uk ) were performed in part on the Orcinus supercomputer at the WestGrid High Performance Computing (HPC) Consortium ( www.westgrid.ca ), in part on the General Purpose Cluster supercomputer at the SciNet HPC Consortium. SciNet is funded by: the Canada Foundation for Innovation under the auspices of Compute Canada; the Government of Ontario; Ontario Research Fund – Research Excellence; and the University of Toronto. All authors contributed to the development and writing of this paper. The authorship list is given in three groups: the lead authors (BG, CH, JHD, and FS), followed by two alphabetical groups. The first alphabetical group includes those who are key contributors to both the scientific analysis and the data products. The second group covers those who have either made a significant contribution to the data products, or to the scientific analysis.