adsabs/WIESP2022-NER huggingface dataset:
Paper: 2016A&A...587A..81B (acknowledgments)
This work has been made possible thanks to the ESAC Science Operations Division research funds, code EXPRO IPL-PSS/GP/gp/44.2014, plus support from the ESAC Space Science Faculty. Pablo Riviere-Marichalar and Carlo Manara acknowledge funding from the ESA Research Fellowship program. H. Bouy is funded by the Spanish Ramn y Cajal fellowship program number RYC-2009- 04497. This research made use of the SIMBAD database, operated at the CDS, Strasbourg, France. This work made extensive use of Topcat (TOPCAT http:// www.star.bristol.ac.uk/~mbt/topcat/ and STILTS, Taylor 2005, 2006). We thank the referee, Manuel Güdel, for his comments and corrections, which help to make this work complete. We would also like to thank Benjamin Montesinos and Nuria Huelamo for their comments and help.
Paper: 2015A&A...579A..51B (acknowledgments)
Based on observations with the 100-m Telescope of the MPIfR (Max-Planck-Institut für Radioastronomie) at Effelsberg. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. S.E.R. and R.J.S. acknowledge support from the DFG via the SPP 1573 Physics of the ISM (grants RA 2158/1-1 and SM321/1-1). R.J.S. also acknowledge support from the SFB 881 The Milky Way System.
Paper: 2019ApJ...884..149H (acknowledgments)
We thank the referee for many insightful comments and for discussion that helped to improve this paper significantly. The authors thank Merel van ’t Hoff, Jeong-Eun Lee, and Marc Audard for providing valuable discussions. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2017.1.01693.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. T.H.H. and N.H. acknowledge the support by Ministry of Science and Technology of Taiwan (MoST) 107-2119-M-001-041 and 108-2112-M-001-048. N.H. acknowledges a grant from MoST 108-2112-M-001-017. C.W. acknowledges financial support from the University of Leeds and from the Science Facilities and Technology Council (STFC), under grant No. ST/R000549/1. J.K.J. acknowledges support from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation program (grant agreement No. 646908). S.-P.L. acknowledges the support from the Ministry of Science and Technology ( MOST ) of Taiwan with grant MOST 106-2119-M-007-021-MY3. Software: CASA (McMullin et al. 2007 ), RADMC-3D (Dullemond et al. 2012 ), Astropy (Astropy Collaboration et al. 2013 ), APLpy (Robitaille Bressert 2012 ).
Paper: 2015ApJ...804...25A (acknowledgments)
We would like to give our special thanks to the authors of Pierbattista et al. ( 2012 ), particularly to Dr. M. Pierbattista for producing new fits for the simulated data and Prof. P. Gonthier for reading a draft of our paper and giving us constructive feedback. We also thank Prof. K. Tollefson and Dr. J. Pretz for useful suggestions and Dr. G. Sinnis and Prof. M. Voit for their encouragement to publish this work. This work was supported by the National Science Foundation.
Paper: 2018A&A...620A..61C (acknowledgments)
RC would like to thank Raphael Gavazzi for useful discussions. The authors would like to thank the anonymous referee, whose comments were helpful in improving the paper, and the telescope staff at the IRAM 30-m telescope for their excellent support during observations. We are also very grateful to the former director of IRAM, P. Cox, for his generous attribution of Director’s Discretionary Time early on during the program, and to Daniel Dicken for sharing telescope time. This work is based on observations carried out under projects number 082-12, D09-12, 065-13, 094-13, 223-13, 108-14, and 217-14 with the IRAM 30-m telescope. IRAM is supported by INSU/CNRS (France), MPG (Germany) and IGN (Spain). This work was supported by the Programme National Cosmology et Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES. RC was supported by DFF – 4090-00079. ML acknowledges CNRS and CNES for support. CY was supported by an ESO Fellowship.
Paper: 2016MNRAS.456.3375B (acknowledgments)
We thank the anonymous referee for the valuable comments that helped us to improve the paper. PB thanks CSIR, India for Research Fellowship grant.
Paper: 2015MNRAS.446.3731K (acknowledgments)
PC acknowledges the financial support of the European Research Council (ERC; project PALs 320620)
Paper: 2015ApJ...805..159M (acknowledgments)
We thank the referee for helpful comments that improved the quality of our work. R.M. is grateful to the Aspen Center for Physics and the NSF Grant #1066293 for hospitality during the completion of this work and for providing a stimulating environment that inspired this project. Support for this work was provided by the David and Lucile Packard Foundation Fellowship for Science and Engineering awarded to A.M.S.
Paper: 2018MNRAS.478.4939P (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the French–Brazilian exchange program CAPES-COFECUB. We are grateful to T. Been, C. Grygiel, A. Domaracka and J. M. Ramillon for their invaluable support. The Brazilian agencies CNPq (INEspaço), CNPq (301868/2017-4), CAPES (BEX 5383/15-3) and FAPERJ (E-26/213.577/2015, E-26/216.730/2015, E-05/2015-214814 and E-03/2017-203.204) are also acknowledged.
Paper: 2015MNRAS.446.1848K (acknowledgments)
I am grateful to the referee, for helpful comments and suggestions that improved the paper.
Paper: 2017MNRAS.469S.416C (acknowledgments)
Acknowledgements Rosetta is an ESA mission with contributions from its member states and NASA. We thank CNES for sponsoring the French participations to Alice hardware and VIRTIS_H development, operations and scientific analysis. The Alice team acknowledges continuing support from NASA’s Jet Propulsion Laboratory through contract 1336850 to the Southwest Research Institute. We thank an anonymous reviewer for the valuable comments and suggestions that has improved the manuscript.
Paper: 2018ApJ...858...82Y (acknowledgments)
We thank Barbara De Marco and Agata Różańska for discussion and comments. This research was supported by Polish National Science Centre grant nos. 2015/17/B/ST9/03422 and 2015/18/M/ST9/00541 and by Ministry of Science and Higher Education grant W30/7.PR/2013. This research was supported by “the Fundamental Research Funds for the Central Universities.” It received funding from the European Union Seventh Framework Programme (FP7/2007–2013) under grant agreement no. 312789, Polish National Science Center grant Polonez 2016/21/P/ST9/04025, the National Program on Key Research and Development Project (grant no. 2016YFA0400803), and the Chinese National Science Foundation (grant no. 11622326). This research was partly financed by grant DEC-2011/03/B/ST9/03459 from the Polish National Science Centre. This work made use of the High Performance Computing Resource in the Core Facility for Advanced Research Computing at Shanghai Astronomical Observatory.
Paper: 2018ApJ...857..103K (acknowledgments)
We thank the anonymous referee for a very careful reading of our manuscript that has led to a marked improvement in the clarity of this paper. M.B.K. is grateful to the University of Sheffield and the Hungarian Academy of Sciences for the support received. M.B.K. also acknowledges the open research program of CAS Key Laboratory of Solar Activity, National Astronomical Observatories, No. KLSA201610. P.C. thanks the University of Sheffield for hospitality and support for a visit during which this work was initiated and the CAS PIFI project 2017VMC0002 and National Astronomical Observatories, Beijing, for support. The simulation was carried out on NASA’s Pleiades supercomputer under GID s1061. P.C. also acknowledges computing time awarded on the PARAM Yuva-II supercomputer at C-DAC, India, under the grant name Hydromagnetic-Turbulence-PR. We have used the 3D visualization software Paraview for volume rendering and field line plotting. R.E. is grateful to the Science and Technology Facilities Council (STFC; grant Nos. ST/L006316/1 and ST/M000826/1) UK and the Royal Society for their support. The authors also express their gratitude to Christopher J. Nelson and Michael S. Ruderman (both at University of Sheffield, UK) for a number of useful discussions and improving the manuscript.
Paper: 2018A&A...618A.107R (acknowledgments)
M. I. R.-B. and Ch. H. acknowledge financial support of the European Community under the FP7 by the ERC starting grant 257431. Ch. H. thanks for the hospitality of the Kaptyn Astronomical Insititut at the University of Groningen, and travel support from NWO and LKBF. We thank A. Sicilia-Aguilar and P. Rimmer for the insightful and valuable discussions of the manuscript. Most literature search was performed using the ADS. We gratefully acknowledge our local computer support.
Paper: 2019MNRAS.485.2656C (acknowledgments)
ACKNOWLEDGEMENTS We thank the referee for useful comments and suggestions that improved the clarity of this paper. LC is the recipient of an Australian Research Council Future Fellowship (FT180100066) funded by the Australian Government. This research was conducted by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. JvdS is funded under Bland-Hawthorn’s ARC Laureate Fellowship (FL140100278). CPL has received funding from a Discovery Early Career Researcher Award (DE150100618) and the MERAC Foundation for a Post-doctoral Research Award. SB acknowledges the funding support from the Australian Research Council through a Future Fellowship (FT140101166). MSO acknowledges the funding support from the Australian Research Council through a Future Fellowship (FT140100255). The SAMI Galaxy Survey is based on observations made at the Anglo-Australian Telescope. The Sydney-AAO Multi-object Integral field spectrograph (SAMI) was developed jointly by the University of Sydney and the Australian Astronomical Observatory. The SAMI input catalogue is based on data taken from the Sloan Digital Sky Survey, the GAMA Survey, and the VST ATLAS Survey. The SAMI Galaxy Survey is supported by the Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013, the Australian Research Council Centre of Excellence for All-sky Astrophysics (CAASTRO), through project number CE110001020, and other participating institutions. The SAMI Galaxy Survey website is http://sami-survey.org/ GAMA is a joint European–Australasian project based around a spectroscopic campaign using the Anglo-Australian Telescope. The GAMA input catalogue is based on data taken from the Sloan Digital Sky Survey and the UKIRT Infrared Deep Sky Survey. Complementary imaging of the GAMA regions is being obtained by a number of independent survey programs including GALEX MIS, VST KiDS, VISTA VIKING, WISE, Herschel -ATLAS, GMRT, and ASKAP providing UV to radio coverage. GAMA is funded by the STFC (UK), the ARC (Australia), the AAO, and the participating institutions. The GAMA website is http://www.gama-survey.org/ . Part of this work was performed on the gSTAR national facility at Swinburne University of Technology. gSTAR is funded by Swinburne and the Australian Government’s Education Investment Fund. 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, Bruyeres-le-Chatel.
Paper: 2019MNRAS.489..385T (acknowledgments)
ACKNOWLEDGEMENTS DT acknowledges financial post-doctoral support from The Claude Leon Foundation (South Africa). YZM would like to acknowledge the supports from National Research Foundation with grant no. 105925 and 110984, and from the National Science Foundation of China, no. 11828301. The Parkes radio telescope is part of the Australia Telescope National Facility which is funded by the Australian Government for operation as a National Facility managed by CSIRO (Commonwealth Scientific and Industrial Research Organisation). The authors would like to thank Dr. Christopher Anderson for granting access to the processed Parkes 21-cm maps, and for several valuable suggestions about the analysis presented in this work.
Paper: 2020A&A...634A..36M (acknowledgments)
D.M., E.K., and M.C. acknowledge support from the European Research Council through the Consolidator Grant ERC-2017-CoG-771310-PI2FA. R. O. acknowledges support from the Spanish Ministry of Economy, Industry and Competitiveness through the grant AYA2017-85465-P. R.O. also acknowledges the travel support received from the International Space Science Institute (Bern, Switzerland) as well as discussions with members of the ISSI team on “Observed multi-scale variability of coronal loops as a probe of coronal heating”, led by C. Froment and P. Antolin. The authors thankfully acknowledge the technical expertise and assistance provided by the Spanish Supercomputing Network (Red Espanola de Supercomputacion), as well as the computer resources used: the LaPalma Supercomputer, located at the Instituto de Astrofisica de Canarias.
Paper: 2016MNRAS.458.1427H (acknowledgments)
CH acknowledges the support from the Science and Technology Facilities Council (STFC) for PhD funding. We thank the groups that have spent time developing molecular line lists, particularly ExoMol, HITEMP and HITRAN, without which this work would not be possible. We also thank Richard Freedman, Iouli Gordon, Jonathan Tennyson and Sergey Yurchenko for helpful discussions. We would like to thank the anonymous reviewer for a very helpful review.
Paper: 2016MNRAS.456.3386J (acknowledgments)
This work has been funded by the National Natural Science Foundation of China under Grant No. 11403015, 11203016, 11143012 and U1531105. This work is partly supported by the Natural Science Foundation of Shandong Province under grant no. ZR2012AQ008 and ZR2014AQ007.
Paper: 2016MNRAS.455.2656L (acknowledgments)
ELR would like to thank the anonymous referee for their useful comments, which improved the Letter significantly. ELR acknowledges support from the University of Texas at San Antonio and University of Texas at Austin.
Paper: 2016MNRAS.458..868L (acknowledgments)
We would like to thank Cees Bassa and Jason Hessels for helping to conceive and develop toaster . We would also like to thank Paulo Freire and Gregory Desvignes for useful discussions, as well as Stefan Osłowski, Golam Shaifullah, Antoine Lassus, and John Antoniadis for helping to observe. PL and EG acknowledge support from IMPRS Bonn/Cologne. RNC acknowledges the support of IMPRS Bonn/Cologne and the Bonn–Cologne Graduate School. KJL gratefully acknowledges support from National Basic Research Program of China, 973 Program, 2015CB857101 and NSFC 11373011. The PSRIX backend was constructed as part of the LEAP project, which was funded by the ERC Advanced Grant LEAP, Grant Agreement Number 227947 (PI M. Kramer).
Paper: 2016MNRAS.461.4088D (acknowledgments)
We thank the anonymous referee for her/his useful comments. Fruitful discussions with F. Fraternali, J.P. Naiman, R. Sancisi, M. Tosi, and G. Zamorani are also acknowledged. FD'A and AD'E acknowledge support from PRIN INAF 2014 (principal investigator S. Cassisi). EV acknowledges support from grant NASA-NNX13AF45G .
Paper: 2016A&A...594A..12P (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, JA, 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 . Particular thanks are due to the extraordinary NERSC staff, who have supported the Planck mission for over a decade and who facilitated the production and distribution of FFP8 in numerous ways.
Paper: 2017A&A...597A.109S (acknowledgments)
The authors would like to thank the anonymous referee for his/her fruitful comments, R. Lecocguen, D. Crussaire and the team at the MSDP for acquiring the H observations. We thank G. Aulanier for fruitful discussions and the sketch of a “tornado”, which has been drawn by Sylvain Cnudde. We deeply thank L. Fletcher for giving many comments on the manuscript to improve its clarity.P.J.L. acknowledges support from an STFC Research Studentship ST/K502005/1. N.L. acknowledges support from STFC grant ST/L000741/1. L.O. would like to acknowledge support by NASA Cooperative Agreement grant NNG11PL10A to CUA. The AIA data are provided courtesy of NASA/SDO and the AIA science team.
Paper: 2016MNRAS.455..276E (acknowledgments)
The authors warmly thank Evelyne Roueff, Jonathan Tennyson and Alexandre Faure for numerous fruitful discussions. We acknowledge the support of the European COST Actions ‘Our Astrochemical History’ CM1401 and ‘Molecules in motion’ (MOLIM) CM1405. We are grateful to the International Atomic Energy Agency (IAEA, Vienna) for scientific and financial support through the Contract No. 16712 with the University of Douala (CAMEROON) and through the Coordinated Research Projects ‘Atomic and Molecular Data for State-Resolved Modelling of Hydrogen and Helium and their Isotopes in Fusion Plasmas’ and ‘Light Element Atom, Molecule and Radical Behaviour in the Divertor and Edge Plasma Regions’. We thank the financial support from the French CNRS via the programmes ‘Physique et Chimie du Milieu Interstellaire’, the ‘Physique théorique et ses interfaces’ projects TheMS, TPCECAM and ‘InPhynity MEXAT’. We are very grateful for the generous support of Agence Nationale de la Recherche via the projects ‘SUMOSTAI’ (ANR-09-BLAN-020901) and ‘HYDRIDES’ (ANR-12-BS05-0011-01), of IFRAF-Triangle de la Physique via the project ‘SpecoRyd’, and of Fédération de Recherche Fusion par Confinement Magnétique - ITER. We acknowledge the constant financial support from La Région Haute-Normandie via the CPER ‘THETE’ project, and the GRR Electronique, Energie et Matériaux. Part of this work has been performed in the frame of the ‘Fédération de Recherche Energie, Propulsion, Environnement’, and of the LabEx EMC 3 , via the project PicoLIBS (ANR-10-LABX-09-01). Finally, MDEE and OM thank the Laboratoire Ondes et Milieux Complexes of the University of Le Havre for hospitality.
Paper: 2015MNRAS.446.4271S (acknowledgments)
The authors are grateful to Joe Weingartner, Tiffany Lewis and Michael Efroimsky for numerous discussions which contributed to the development of this work. We would also like to thank Nick Cowan for his many helpful comments and suggestions that improved the quality of this study.
Paper: 2019MNRAS.486.3134K (acknowledgments)
ACKNOWLEDGEMENTS JMDK gratefully acknowledges funding from the German Research Foundation (DFG) in the form of an Emmy Noether Research Group (grant number KR4801/1-1, PI Kruijssen), from the European Research Council (ERC) under the European Union’s Horizon 2020 research and innovation programme via the ERC Starting Grant MUSTANG (grant agreement number 714907, PI Kruijssen), and from Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (subproject B2) of the DFG. JP and NB gratefully acknowledge funding from the ERC under the European Union’s Horizon 2020 research and innovation programme via the ERC Consolidator Grant Multi-Pop (grant agreement number 646928, PI Bastian). NB and RAC are Royal Society University Research Fellows. This work made use of high-performance computing facilities at Liverpool John Moores University, partly funded by the Royal Society and LJMU’s Faculty of Engineering and Technology. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC HPC Facility ( www.dirac.ac.uk ). This equipment was funded by BIS National E-infrastructure capital grant ST/K00042X/1, STFC capital grants ST/H008519/1 and ST/K00087X/1, STFC DiRAC Operations grant ST/K003267/1 and Durham University. DiRAC is part of the National E-Infrastructure. This work has made use of numpy (van der Walt, Colbert Varoquaux 2011 ), scipy (Jones et al. 2001 ), and astropy (Astropy Collaboration 2013 ). All figures in this paper were produced using the python library matplotlib (Hunter 2007 ). The authors thank Marta Reina-Campos, Benjamin Keller, and Mélanie Chevance for advice and helpful discussions during the development of this work. We thank an anonymous referee for comments that improved the presentation of this paper.
Paper: 2018ApJ...861...28S (acknowledgments)
The authors thank the referee for comments that helped to improve this paper. We acknowledge the use of the data from SOHO , STEREO , Wind , DSCOVR , and GOES satellites and the world data center (WDC) for Geomagnetism, Kyoto. This work is supported by grants from CAS (Youth Innovation Promotion Association CAS and Key Research Program of Frontier Sciences QYZDB-SSW-DQC015), NSFC (41774181, 41774178, 41574165, 41474164, 41761134088), the Fundamental Research Funds for the Central Universities (WK2080000077), and the Specialized Research Fund for State Key Laboratories.
Paper: 2015MNRAS.447.1247S (acknowledgments)
We thank all the python , numpy and scipy communities for the high-quality free software they made available. MS thanks Philipp Edelmann for all the technical support during the developing of this work. EEOI acknowledges financial support from Brazilian agencies FAPESP (2011/09525-3) and CAPES (9229-13-2). Supported by German DFG Cluster of Excellence ‘Origin and Structure of the Universe’ and the DFG Transregio Project 33 ‘Dark Universe’. We thank Dan Birchall for observing assistance, the technical and scientific staffs of the Palomar Observatory, the High Performance Wireless Radio Network (HPWREN) and the University of Hawaii 2.2-m telescope. We recognize the significant cultural role of Mauna Kea within the indigenous Hawaiian community, and we appreciate the opportunity to conduct observations from this revered site. This work was supported by the Director, Office of Science, Office of High Energy Physics, of the US Department of Energy under Contract No. DE-AC02-05CH11231; by a grant from the Gordon Betty Moore Foundation; in France by support from CNRS/IN2P3, CNRS/INSU, PNCG and the Lyon Institute of Origins under grant ANR-10-LABX-66; and in Germany by the DFG through TRR33 ‘The Dark Universe’. Some results were obtained using resources and support from the National Energy Research Scientific Computing Center, supported by the Director, Office of Science, Office of Advanced Scientific Computing Research, of the US Department of Energy under Contract No. DE-AC02-05CH11231. HPWREN is funded by National Science Foundation Grant Number ANI-0087344, and the University of California, San Diego. This work was written using the collaborative ShareLaTeX platform.