adsabs/WIESP2022-NER huggingface dataset:
Paper: 2015MNRAS.450.2708L (acknowledgments)
We thank the anonymous referee for a helpful report. ADB wishes to acknowledge partial support from grants NSF-AST 0955836 and 1412419. MR wishes to acknowledge support from CONICYT(CHILE) through FONDECYT grant no. 1140839 and partial support through project BASAL PFB-06. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc.
Paper: 2015ApJ...800...32L (acknowledgments)
The RXTE /PCA data were obtained from the RXTE Guest Observer Facility (GOF) at NASA's Goddard Space Flight Centre (GSFC). This work was supported by the Natural Sciences and Engineering Research Council of Canada. D.L. thanks the referee for suggestions that led to improvements in this work.
Paper: 2017MNRAS.471L...6L (acknowledgments)
Acknowledgments The authors would like to thank the anonymous referee for valuable comments that improved the manuscript. We thank the teams of Fermi and GOES for their open data-use policy. This study is supported by the National Natural Science Foundation of China (NSFC) under grants 11603077, 11573072, 11333009, 973 programme (2014CB744200) and Laboratory No. 2010DP173032. DL is supported by the Youth Fund of Jiangsu No. BK20161095. QMZ is supported by the Surface Project of Jiangsu No. BK20161618 and the Youth Innovation Promotion Association CAS. The authors wish to thank the International Space Science Institute in Beijing (ISSI-BJ) for supporting and hosting the meetings of the International Team on ‘Magnetohydrodynamic Seismology of the Solar Corona in the Era of SDO/AIA', during which discussions leading to this publication were held.
Paper: 2016ApJ...820..122F (acknowledgments)
Y.F. is supported from the Grant-in-Aid No. 25887024 by the Japan Society for the Promotion of Science and from an appointment to the NASA Postdoctoral Program at NASA Goddard Institute for Space Studies, administered by Oak Ridge Affiliated Universities. D.S.S. gratefully acknowledges support from a fellowship from the AMIAS group. J.N. acknowledges support from NASA grant HST AR-12146.04-A and NSF grant AST-1102738. We thank David Hogg for encouraging us to pursue calculations of exoplanetary radio emission. We thank Greg Novak for helpful conversations. We thank Jake VanderPlas for developing the XKCD-style plotting package for matplotlib, and acknowledge its use. A.P. is grateful for support from NSF grants 1352519 and 1440343. Y.F. greatly acknowledges insightful and helpful discussions with Tomoki Kimura and Hiroki Harakawa. The portion of this research for which T.M. is responsible was performed under a National Research Council Research Associateship Award at the Naval Research Laboratory (NRL). Basic research in radio astronomy at NRL is supported by 6.1 Base funding.
Paper: 2019ApJ...882..152Z (acknowledgments)
The authors thank Huanqing Chen and Philip Mansfield for their helpful insights and comments during this project. H.Z. acknowledges support from the Heising-Simons Foundation, the Kavli Institute for Cosmological Physics and the Blue Waters Student Internship Program. C.A. acknowledges support from both the Enrico Fermi Institute and the Kavli Institute for Cosmological Physics. N.G.’s contribution to this work used the resources of the Fermi National Accelerator Laboratory (Fermilab), a U.S. Department of Energy, Office of Science, HEP User Facility. Fermilab is managed by Fermi Research Alliance, LLC (FRA), acting under contract No. DE-AC02-07CH11359. This work was partly supported by a NASA ATP grant NNX17AK65G, and used resources of the Argonne Leadership Computing Facility, which is a DOE Office of Science User Facility supported under Contract DE-AC02-06CH11357. An award of computer time was provided by the Innovative and Novel Computational Impact on Theory and Experiment (INCITE) program. This research is also part of the Blue Waters sustained-petascale computing project, which is supported by the National Science Foundation (awards OCI-0725070 and ACI-1238993) and the state of Illinois. Blue Waters is a joint effort of the University of Illinois at Urbana-Champaign and its National Center for Supercomputing Applications.
Paper: 2019MNRAS.482.3736C (acknowledgments)
ACKNOWLEDGEMENTS Parts of this research were conducted by the Australian Research Council Centre of Excellence for Gravitational Wave Discovery (OzGrav) through project number CE170100004. The authors would like to thank John Bowman at Walmart Labs (user ‘jbowman’ on stats.stackexchange.com ) for suggesting useful modifications to the likelihood function.
Paper: 2015MNRAS.453.1550F (acknowledgments)
The author acknowledges the Big Bear Solar Observatory, Observatory Paris–Meudon, STEREO , SDO teams for the high-quality data supplied. The author thanks the referee for critical comments and useful suggestions. Movies created using the ESA and NASA funded Helioviewer Project. This work was supported in part by the Russian Foundation for Basic Research (grant 14-02-92690).
Paper: 2018A&A...616L...1G (acknowledgments)
We are indebted to Tom Bell for initiating this project and for his help in the early data reduction. We thank our anonymous referee for useful comments. We also thank the Spanish MCIU and the ERC for funding support under grants AYA2017-85111-P and ERC-2013-Syg-610256-NANOCOSMOS.
Paper: 2019MNRAS.482..771G (acknowledgments)
ACKNOWLEDGEMENTS MG wishes to acknowledge the support by the Austrian FWF project J-3588-N27, and thanks Y. Cavecchi for suggestions to improve the computations; S. Aljbaae running some of our numerical orbital integrations on a cluster at FEGP-UNESP (Brazil); and Western University for providing computational facilities (the TITAN supercluster and the SHARCNET). EAS gratefully acknowledges the Natural Sciences and Engineering Research Council of Canada (NSERC) Postdoctoral Fellowship programme for supporting this project. RD acknowledges the support by the Austrian FWF project S11603-N16. We gratefully acknowledge the developers of iSALE-2D ( http://www.isale-code.de ), the simulation code used in our research, including G. Collins, K. Wunnemann, D. Elbeshausen, B. Ivanov, and J. Melosh. The authors also thank the referee Mario Melita for valuable advice allowing us to improve this paper.
Paper: 2015ApJ...804...16M (acknowledgments)
Herschel is an ESA space observatory with science instruments provided by European-led Principal Investigator consortia and with important participation from NASA. M.M. acknowledges support by NASA through a Hubble Fellowship grant No. HST -HF51308.01 A awarded by the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., for NASA, under contract NAS 5-26555. We also acknowledge support from grant HST -GO-12570.01 A. N.W. thanks Rebecca Canning for helpful discussions.
Paper: 2017ApJ...849...11G (acknowledgments)
We thank Pierre Maxted for interesting discussions and John Southworth for help compiling Table 6 . This paper includes data collected by the Kepler / K 2 mission. Funding for the K 2 mission of Kepler is provided by the NASA Science Mission directorate. Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST) under support by the NASA Office of Space Science via grant NNX09AF08G and by other grants and contracts. Some of the data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California, and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation. The authors wish to recognize and acknowledge the very significant cultural role and reverence that the summit of Maunakea has always had within the indigenous Hawaiian community. We are most fortunate to have the opportunity to conduct observations from this mountain. Finally, we would like to thank the anonymous referee for their careful reading of the manuscript and helpful suggestions for improvement. Facilities: Kepler ( K2 ), Keck:I, Sloan , CTIO:2MASS, FLWO:2MASS , WISE . Software: astropy (Astropy Collaboration et al. 2013 ), emcee (Foreman-Mackey et al. 2013 ), george (Ambikasaran et al. 2014 ).
Paper: 2018ApJ...856..143I (acknowledgments)
We thank the anonymous referee for valuable comments, which helped improve the clarity of this manuscript. We are grateful to Dr. K. Saigo, Y. Ao, A. Kawamura, and F. Egusa for their supports regarding ALMA data reduction. M.I. was supported by JSPS KAKENHI grant Nos. 23540273 and 15K05030 and the ALMA Japan Research Grant of the NAOJ Chile Observatory, NAOJ-ALMA-0001, 0023, 0072. This paper made use of the following ALMA data: ADS/JAO.ALMA#2013.1.00032.S, 2015.1.00027.S, and 2016.1.00051.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. Data analysis was in part carried out on the open use data analysis computer system at the Astronomy Data Center, ADC, of the National Astronomical Observatory of Japan. This research has made use of NASA’s Astrophysics Data System and the NASA/IPAC Extragalactic Database (NED), which is operated by the Jet Propulsion Laboratory, California Institute of Technology, under contract with the National Aeronautics and Space Administration.
Paper: 2015MNRAS.447.3756S (acknowledgments)
We are grateful to Paweł Moskalik for stimulating discussions, reading the manuscript and detailed comments. Fruitful conversation with Wojtek Dziembowski is also acknowledged. This research is supported by the Polish National Science Centre through grant DEC-2012/05/B/ST9/03932 and by the Polish Ministry of Science and Higher Education through the program ‘Ideas Plus’ award no. IdP2012 000162. The OGLE project has received funding from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013)/ERC grant agreement no. 246678 to AU.
Paper: 2016ApJ...824..109C (acknowledgments)
We thank A. Gould for valuable discussions. SCN acknowledges support by JPL grant 1500811. GS thanks NExScI for hospitality at Caltech during part of this work.
Paper: 2018MNRAS.480.5385S (acknowledgments)
ACKNOWLEDGEMENTS We thank Ryoma Murata for the detailed investigation that found the error with respect to constraining average M vs average log M.
Paper: 2015ApJ...809..187S (acknowledgments)
We thank the referee for providing a helpful report. We also thank Taysun Kimm, Chris Matzner, and Jim Stone for helpful comments and suggestions on the manuscript. This work was supported by Grants No. AST-1312006 and PHY-1144374 from the National Science Foundation. MAS is supported by the Max-Planck/Princeton Center for Plasma Physics. Part of this project was conducted during a visit to the KITP at U.C. Santa Barbara, which is supported by the National Science Foundation under Grant No. PHY-1125915. Simulations were performed on the computational resources supported by the PICSciE TIGRESS High Performance Computing Center at Princeton University.
Paper: 2015A&A...579A.114M (acknowledgments)
This paper made use of the following ALMA data: ADS/JAO.ALMA 2011.0.00902.S and 2013.1.01004.S. ALMA is a partnership of ESO (representing its member states), NSF (USA), and NINS (Japan), together with NRC (Canada) and NSC and ASIAA (Taiwan), in cooperation with the Republic of Chile. The Joint ALMA Observatory is operated by ESO, AUI/NRAO, and NAOJ. The 2011.0.00902.S data was obtained by N.M.M. while she was a Master student at National Tsing Hua University, Taiwan, under the supervision of S.P.L. The authors thank J. C. Mottram for his help in using RATRAN; and M. Hogerheijde for permission to use the 2D version of RATRAN. Astrochemistry in Leiden is supported by the Netherlands Research School for Astronomy (NOVA), by a Royal Netherlands Academy of Arts and Sciences (KNAW) professor prize, and by the European Union A-ERC grant 291141 CHEMPLAN. This work is supported by grant 639.041.335 from the Netherlands Organisation for Scientific Research (NWO) and by the Netherlands Research School for Astronomy (NOVA) and by the Space Research Organization Netherlands (SRON). S.P.L. acknowledges support from the Ministry of Science and Technology of Taiwan with Grants MOST 102-2119-M-007-004-MY3.
Paper: 2020ApJ...889...29C (acknowledgments)
We thank the referee Ioannis Contopoulos for valuable comments and suggestions. We would like to thank Jérôme Pétri for some useful discussions. We acknowledge the financial support from the National Natural Science Foundation of China 11573060 and 11661161010, the National Science Foundation of China 11673060, the National Science Foundation of China 11871418.
Paper: 2015ApJ...799...98M (acknowledgments)
We thank Andy Fabian, Rich Plotkin, Amy Reines, Claudia Scarlata, and Anil Seth for helpful discussions, and an anonymous referee for constructive comments. This work was supported in part by Chandra Award Number 11620915, by the National Science Foundation under grant no. NSF PHY11-25915 and by NASA through grant HST-GO-12591.01 from the Space Telescope Science Institute, which is operated by AURA, Inc., under NASA contract NAS 5-26555. J.H.W. acknowledges support by the National Research Foundation of Korea grant funded by the Korea government (No. 2012-006087 and No. 2010-0027910).
Paper: 2018MNRAS.475.1274S (acknowledgments)
ACKNOWLEDGEMENTS We thank an anonymous reviewer whose comments greatly improved the manuscript. We also thank EPnetFaN members for providing us with the computational environment and technical advice. We would like to thank Enago ( http://www.enago.jp ) for the English language review. This work was supported by MEXT/JSPS KAKENHI Grant Numbers 23103003, 22540427, 11740117, and 17H06457.
Paper: 2018ApJ...864..119H (acknowledgments)
The authors thank Lorne Nelson for sharing computing facilities. The computations were partially carried out on facilities managed by Calcul Québec and Compute Canada. This work has been supported by the Japan Society for the Promotion of Science (JSPS) KAKENHI Grant Numbers JP16H03986 and JP17K18792. The work has also been supported by a Humboldt Research Award to Ph.P. at the University of Bonn. R.H. was supported by the JSPS Overseas Research Fellowship No. 29–514. Software: MESA (v10108; Paxton et al. 2011 , 2013 , 2015 , 2018 ).
Paper: 2015MNRAS.447.3960C (acknowledgments)
This research has made use of data obtained through the HEASARC Online Service, provided by the NASA/GSFC, in support of NASA High Energy Astrophysics Programs. MC acknowledges the many discussion with suggestions provided by Professor A R Rao, TIFR, Mumbai, India. This research has made use of the General High-energy Aperiodic Timing Software (GHATS) package developed by T. M. Belloni at INAF – Osservatorio Astronomico di Brera.
Paper: 2017MNRAS.465L..20S (acknowledgments)
We thank Scott Dodelson, Enrique Gaztanaga, Ashley Ross, Martin Crocce, Eduardo Rozo, Jonathan Blazek, Adam Amara, Benjamin Joachimi, Catherine Heymans, Rachel Mandelbaum, Josh Frieman and the DES MPP group for helpful conversations. SS recognizes receipt of a UK Science and Technology Facilities Council (STFC) Doctoral Training Grant. SLB, MT, JZ and DK acknowledge support from the European Research Council.
Paper: 2018ApJ...866..149Z (acknowledgments)
Breakthrough Listen is funded by the Breakthrough Initiatives ( breakthroughinitiatives.org ). Y.G.Z. thanks Dan Werthimer, Deepthi Gorthi, Aman Dhar, and Liam Conner for helpful discussions. V.G. would like to acknowledge NSF grant 1407804 and the Marilyn and Watson Alberts SETI Chair funds.
Paper: 2018A&A...620A..51P (acknowledgments)
Part of this work was supported by the French CNRS, the French Programme National de Cosmologie et Galaxies (PNCG) of CNRS/INSU with INP and IN2P3, co-funded by CEA and CNES. We acknowledge support from the Spanish Programa Nacional de Astronomía y Astrofísica under grant AYA 2006-02358 and the Swiss National Science Foundation. Partially funded by the Spanish MEC under the Consolider-Ingenio 2010 Program grant CSD2006-00070: First Science with the GTC ( http://www.iac.es/consolider-ingenio-gtc/ ). This work recieved support from Agence Nationale de la recherche bearing the reference ANR-09-BLAN-0234, and from the ECOS SUD Program C16U02. This work has been carried out thanks to the support of the OCEVU Labex (ANR-11-LABX-0060) and the A*MIDEX project (ANR-11-IDEX-0001-02) funded by the “Investissements d’Avenir” French government program managed by the ANR. NL acknowledges financial support from European Research Council Advanced Grant FP7/669253. JG and NC acknowledge financial support from Spanish MINECO (AYA2016-75808-R). MB acknowledges support from AYA grant 2009-11139. This paper is based on observations obtained with WIRCam, a joint project of CFHT, Taiwan, Korea, Canada, France, and the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institute National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. Funding for the DEEP2 survey has been provided by NSF grants AST95-09298, AST-0071048, AST-0071198, AST-0507428, and AST-0507483 as well as NASA LTSA grant NNG04GC89G.
Paper: 2019MNRAS.488..954Q (acknowledgments)
ACKNOWLEDGEMENTS MNSQ acknowledges financial support from the Higher Education Commission (HEC), Pakistan to visit INAF-IAPS in Rome, Italy under the HEC Program of Short Research Visit Abroad: Pakistan Program for Collaborative Research (PPCR) and HEC Project No. 7558/Punjab/NRPU/RD/HEC/2017. We also acknowledge the PEACE instrument team and ESA Cluster Active Archive from where the data has been downloaded.
Paper: 2016MNRAS.462.2715Z (acknowledgments)
LSP, EKG, and IAZ acknowledge support within the framework of Sonderforschungsbereich SFB 881 on ‘The Milky Way System’ (especially subproject A5), which is funded by the German Research Foundation (DFG). LSP and IAZ thank the Astronomisches Rechen-Institut at Heidelberg University, where part of this investigation was carried out, for the hospitality. LSP and IAZ acknowledge the support of the Volkswagen Foundation under the Trilateral Partnerships grant no. 90411. IAZ also acknowledges the special support by the NASU under the Main Astronomical Observatory GRID/GPU computing cluster golowood project. This work was partly funded by a subsidy allocated to the Kazan Federal University for the state assignment in the sphere of scientific activities (LSP). SFS thanks the CONACYT-125180 and DGAPA-IA100815 projects for providing him support in this study. This study uses data provided by the Calar Alto Legacy Integral Field Area (CALIFA) survey ( http://califa.caha.es/ ). Based on observations collected at the Centro Astronómico Hispano Alemán (CAHA) at Calar Alto, operated jointly by the Max-Planck-Institut für Astronomie and the Instituto de Astrofísica de Andalucía (CSIC). This research made use of Montage, funded by the National Aeronautics and Space Administration's Earth Science Technology Office, Computational Technnologies Project, under Cooperative Agreement Number NCC5-626 between NASA and the California Institute of Technology. The code is maintained by the NASA/IPAC Infrared Science Archive. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the US Department of Energy, the National Aeronautics and Space Administration, the Japanese Monbukagakusho, the Max Planck Society, and the Higher Education Funding Council for England. The SDSS Web Site is http://www.sdss.org/ .
Paper: 2016MNRAS.460..458D (acknowledgments)
This study was supported by the ERDF – Research and Development Operational Programme under the project ‘University Scientific Park Campus MTF STU – CAMBO’ ITMS: 26220220179. AD acknowledges the Slovak grant VEGA 1/0335/16. Furthermore, we acknowledge constructive comments of the anonymous reviewer, who helped us to improve this work.
Paper: 2016ApJ...826..138B (acknowledgments)
We thank an anonymous referee for some useful comments and suggestions. This work was supported by the Natural Sciences and Engineering Research Council of Canada, the Fond Québécois pour la Recherche—Nature et Technologie, the Canadian Foundation for Innovation, and time allocation on the computing infrastructures of Calcul Québec, a member of the Compute Canada consortium.
Paper: 2018MNRAS.476..804D (acknowledgments)
Acknowledgements We thank C. Mason and T. Yuan for providing their data and models. This work made use of I mfit and B arolo softwares. EMDT acknowledges the support of the Australian Research Council through grant DP160100723. CG acknowledges support by VILLUM FONDEN Young Investigator Programme through grant no. 10123. FF acknowledges hospitality at the European Southern Observatory in Garching as a scientific visitor. AM, PR, GBC and ML acknowledge financial support from PRIN-INAF 2014 1.05.01.94.02.
Paper: 2019MNRAS.485...30M (acknowledgments)
ACKNOWLEDGEMENTS We would like to sincerely thank the referee for a critical review which proved to be crucial for this study. We acknowledge the work of people involved in the designing, construction and deployment of the COS onboard HST . We also wish to extend our thanks to all those who had carried out data acquisition through Far-UV observations towards the sightlines mentioned in this paper. The plots in Figs 2 , 3 , and 9 were generated using the graphics environment developed by Hunter ( 2007 ).
Paper: 2020MNRAS.492.2910G (acknowledgments)
ACKNOWLEDGEMENTS We thank M. Sun for help with setting up the binary model, Y. Shen and K. Gültekin for helpful discussions, Z. Haiman for useful comments, and an anonymous referee for a quick and constructive report that significantly improved this work.
Paper: 2019A&A...630A..73M (acknowledgments)
Acknowledgements We thank the referee for his/her comments during the reviewing process.. F.M., A.S.M., P.S., A.S. research is carried out within the Collaborative Research Centre 956, sub-projects A6 and C3, funded by the Deutsche Forschungsgemeinschaft (DFG) - project ID 184018867. MP acknowledges funding from the European Unions Horizon 2020 research and innovation program under the Marie Skłodowska-Curie grant agreement No 664931. This research made use of Astropy 4 , a community-developed core Python package for Astronomy ( Astropy Collaboration 2013 , 2018 ).
Paper: 2019ApJ...871..223R (acknowledgments)
We thank Andreas Lagg and Markus Fränz (MPS) for extensive software support and Martha Kusterer and Jon Vandegriff (both JHUAPL) for reducing the MIMI data. Cassini data analysis at MPS was supported by the German Space Agency (DLR) through contracts 50 OH 1101 and 50 OH 1502 and by the Max Planck Society. The JHUAPL authors, as well as K.D., were partially supported by the NASA Office of Space Science under task order 003 of contract NAS5-97271 between NASA/GSFC and JHU and subcontract to the Academy of Athens. E.E. thanks the Brazilian Federal Research Foundation agency (CNPq302583/2015-7) for financial support.
Paper: 2019A&A...629A..64B (acknowledgments)
Acknowledgements The authors thank the anonymous referee who’s comments helped improve the manuscript and Cléa Serpollier for her early investigative work in the subject. This work has been carried out within the frame of the National Centre for Competence in Research PlanetS funded by the Swiss National Science Foundation (SNSF). The authors acknowledge the financial support from the SNSF under grant 200020_172746.