adsabs/WIESP2022-NER huggingface dataset:
Paper: 2018MNRAS.480.2609L (acknowledgments)
ACKNOWLEDGEMENTS RI, NL, and NFM gratefully acknowledge funding from CNRS/INSU through the Programme National Galaxies et Cosmologie and through the CNRS grant PICS07708. We gratefully thank the CFHT staff for performing the observations in queue mode. NF Martin acknowledges the Kavli Institute for Theoretical Physics in Santa Barbara and the organizers of the ‘Cold Dark Matter 2018’ program, during which some of this work was performed. This research was supported in part by the National Science Foundation under grant no. NSF PHY11-25915. BPML gratefully acknowledges support from FONDECYT postdoctoral fellowship no. 3160510. Based on observations obtained at the Canada–France–Hawaii Telescope (CFHT) which is operated by the National Research Council of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawaii. 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. Furthermore, 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. The Pan-STARRS1 Surveys (PS1) have been made possible through contributions of the Institute for Astronomy, the University of Hawaii, the Pan-STARRS Project Office, the Max-Planck Society and its participating institutes, the Max Planck Institute for Astronomy, Heidelberg and the Max Planck Institute for Extraterrestrial Physics, Garching, The Johns Hopkins University, Durham University, the University of Edinburgh, Queen’s University Belfast, the Harvard–Smithsonian Center for Astrophysics, the Las Cumbres Observatory Global Telescope Network Incorporated, the National Central University of Taiwan, the Space Telescope Science Institute, the National Aeronautics, and Space Administration under grant no. NNX08AR22G issued through the Planetary Science Division of the NASA Science Mission Directorate, the National Science Foundation under grant no. AST-1238877, the University of Maryland, and Eotvos Lorand University (ELTE). 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.
Paper: 2018ApJ...859...91S (acknowledgments)
We gratefully acknowledge support from NSF grants AST-1716093 (EMH, AS) and AST-1715145 (AJB) and from the trustees of the William F. Vilas Estate and the University of Wisconsin–Madison Office of the Vice Chancellor for Research and Graduate Education with funding from the Wisconsin Alumni Research Foundation (AJB). The NB921 filter was supported by KAKENHI (23244025) Grant-in-Aid for Scientific Research (A) through the Japan Society for the Promotion of Science (JSPS). The NB816 filter was supported by a grant from Ehime University. We would like to thank Claudia Scarlata for permission to quote unpublished data, David Sobral and Jorryt Matthee for extremely helpful comments on a first draft of the paper, and the anonymous referee for a very useful and constructive report that improved the paper. 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.
Paper: 2018MNRAS.475L..72S (acknowledgments)
ACKNOWLEDGEMENTS Sharanya Sur acknowledges computing time at CDAC National Param Supercomputing Facility Pune, Texas Advanced Computing centre and the use of HPC facilities at IIA. Pallavi Bhat is supported by NSF-DOE Award No. DE-SC0016215. The software used in this work was in part developed by the DOE NNSA-ASC OASCR Flash Center at the University of Chicago.
Paper: 2017MNRAS.472.3455E (acknowledgments)
Acknowledgements We thank the referee for his/her constructive suggestions that improved the paper. The research work at Physical Research Laboratory is funded by the Department of Space, Government of India. This research has made use of data obtained through HEASARC Online Service, provided by NASA/GSFC, in support of NASA High Energy Astrophysics Programs.
Paper: 2016A&A...596A..74S (acknowledgments)
T.K.S. is supported by the Astrobiology Center Project of National Institute of Natural Sciences (NINS) (Grant Number AB271020, AB281018). A.M., A.C. and T.G. acknowledge support by the French ANR, project number ANR-13–13-BS05-0003-01 project MOJO (Modeling the Origin of JOvian planets). T.K.S. thanks Hiroshi Kobayashi and Shinsuke Takasao for fruitful discussions. The authors thank the referee for many valuable comments.
Paper: 2019MNRAS.486.1563M (acknowledgments)
ACKNOWLEDGEMENTS This research is supported by the CHE-ISF I-Core centre for excellence in Astrophysics. TM is supported by JSPS Overseas Challenge Program for Young Researchers and by Grant-in-Aid for JSPS Research Fellow 17J09895. TP is supported by an advanced ERC grant TReX and by the Templeton foundation. EN is partially supported by an consolidator ERC grant (JetNS) and an ISF grant.
Paper: 2019ApJ...870....2C (acknowledgments)
The work at NC State (S.C., K.E., and C.F.) was supported by the Department of Energy through an Early CAREER Award (DOE grant No.SC0010263). C.F. acknowledges support from the Research Corporation for Science Advancement through a Cottrell Scholar Award. The effort at the Universität Basel was supported by the Schweizerischer Nationalfond and by the ERC Advanced Grant “FISH.” K.E. acknowledges support from the GSI. A.P. acknowledges support from the INFN project “High Performance data Network” funded by the Italian CIPE. Software : Agile (Liebendörfer 2001 ), CFNET (Fröhlich et al. 2006b ), Matplotlib (Hunter 2007 ).
Paper: 2018MNRAS.474.2313L (acknowledgments)
Acknowledgements We acknowledge financial support from the U.S. National Science Foundation, Grant No. CHE-1565872. JK acknowledges XSEDE.org Grant No. CHE-130120 and University of Maryland High-Performance Deepthought facilities for computational time. FL and SDLP acknowledge the programme ‘Physique et Chimie du Milieu Interstellaire’ (PCMI) of CNRS/INSU with INC/INP co-funded by CEA and CNES. FL and SDLP acknowledge financial support from the Institut Universitaire de France.
Paper: 2016MNRAS.461.2867Z (acknowledgments)
We would like to thank Will Percival for helpful conversations. This work was supported in part by the National Science Foundation under Grant no. PHYS-1066293 and the hospitality of the Aspen Center for Physics. NP and FZ are supported in part by a DOE Early Career Grant DE-SC0008080. Funding for SDSS-III has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, and the US Department of Energy Office of Science. The SDSS-III website is http://www.sdss3.org/ . SDSS-III is managed by the Astrophysical Research Consortium for the Participating Institutions of the SDSS-III Collaboration including the University of Arizona, the Brazilian Participation Group, Brookhaven National Laboratory, Carnegie Mellon University, 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. Some of the codes in this paper made use of the Chapel programming language. 1
Paper: 2018MNRAS.480.2508M (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for a careful reading of this paper. We thank Carlos De Breuck, Palle Mø ller, and the APEX team for their support. Based on observations collected by the European Organisation for Astronomical Research in the Southern Hemisphere under ESO program 098.B-0657 and 099.B-0063 (APEX) and 196.B-0578 (VLT/MUSE). We acknowledge funding from the INAF PRIN-SKA 2017 program 1.05.01.88.04. YLJ acknowledges support from CONICYT PAI (Concurso Nacional de Inserción en la Academia 2017) No. 79170132. BV acknowledges the support from an Australian Research Council Discovery Early Career Researcher Award (PD0028506). This work made use of the KUBEVIZ software, which is publicly available at http://www.mpe.mpg.de/dwilman/kubeviz/ .
Paper: 2019MNRAS.489.1543O (acknowledgments)
ACKNOWLEDGEMENTS TEEO gratefully acknowledges funding from the Vermont Space Grant Consortium. The authors wish to acknowledge Ben Stappers for providing timing solutions for some pulsars and Joel Weisberg for providing ionospheric rotation-measure estimates. Portions of this work were carried out with support from US National Science Foundation grants AST 0968296 and 1814397. DM acknowledges funding from the grant ‘Indo-French Centre for the Promotion of Advanced Research – CEFIPRA’. The National Astronomy and Ionosphere Center (also known as Arecibo Observatory) is operated by the University of Central Florida under a cooperative agreement with the US National Science Foundation, and in alliance with Yang Enterprises and the Ana G. Méndez-Universidad Metropolitana. This work made use of the NASA ADS astronomical data system.
Paper: 2015MNRAS.449.2024S (acknowledgments)
MS thanks Keiichi Umetsu for useful discussions and Adi Zitrin and Julian Merten for providing useful information on the SL analysis of the CLASH clusters. LM and MS acknowledge financial contributions from contracts ASI/INAF I/023/12/0, by the PRIN MIUR 2010-2011 ‘The dark Universe and the cosmic evolution of baryons: from current surveys to Euclid’ and by the PRIN INAF 2012 ‘The Universe in the box: multiscale simulations of cosmic structure’. CG's research is part of the project GLENCO, funded under the European Seventh Framework Programme, Ideas, Grant Agreement no. 259349.
Paper: 2017ApJ...841...68V (acknowledgments)
We thank Nacho Martín-Navarro for comments on the manuscript, and the anonymous referee for an excellent and thorough report that improved the paper. Support from NASA grant NNX15AK14G, STScI grant GO-13681, and NSF grants AST-1313280, AST-1515084, AST-1518294, AST-1616598, and AST-1616710 is gratefully acknowledged. C.C. acknowledges support from the Packard Foundation. A.V. is supported by an NSF Graduate Research Fellowship. A.J.R. is supported as a Research Corporation for Science Advancement Cottrell Scholar. Based on data obtained with the W.M. Keck Observatory, on Maunakea, Hawaii. 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.
Paper: 2017MNRAS.472..998S (acknowledgments)
Acknowledgements This material is based upon work supported by the National Science Foundation under Grant No. 1411943. Part of the work presented herein is supported by NASA Grant No. NNX15AK92G. This study is based on data taken with the Karl G. Jansky VLA which is operated by the NRAO. The NRAO is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This work is based, in part, on data collected at the Subaru Telescope and obtained from the Subaru Mitaka Okayama Kiso Archive (SMOKA), which is operated by the Astronomy Data centre, National Astronomical Observatory of Japan; observations made with the Spitzer Space Telescope , which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA; and data collected at UKIRT which is supported by NASA and operated under an agreement among the University of Hawaii, the University of Arizona, and Lockheed Martin Advanced Technology centre; operations are enabled through the cooperation of the East Asian Observatory. When the data reported here were acquired, UKIRT was operated by the Joint Astronomy Centre on behalf of the Science and Technology Facilities Council of the U.K. This study is also based, in part, on observations obtained with WIRCam, a joint project of Canada–France–Hawaii Telescope (CFHT), Taiwan, Korea, Canada, France, and the CFHT which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l'Univers of the Centre National de la Recherche Scientifique of France, and the University of Hawai'i. The scientific results reported in this article are based in part on observations made by the Chandra X-ray Observatory and data obtained from the Chandra Data Archive. The spectrographic 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. We wish to thank the indigenous Hawaiian community for allowing us to be guests on their sacred mountain, a privilege, without with, this work would not have been possible. We are most fortunate to be able to conduct observations from this site.
Paper: 2016MNRAS.463.3398B (acknowledgments)
We acknowledge M. Barkov, E. Derishev, Ya. Istomin, M. Drozdova and especially N. Zakamska for useful comments. We also thank the anonymous referee for helpful remarks. This work was supported by the Russian Science Foundation , grant 16-12-10051 .
Paper: 2017MNRAS.467.2943S (acknowledgments)
Acknowledgments The authors are thankful to the anonymous referee for his/her useful comments. HB acknowledges the Inspire Faculty Grant Support (IFA11-PH02) of the Department of Science and Technology, India. The observations reported in this paper were obtained using the 1-m Sampurnanand Telescope, Nainital, India, and the 2-m HCT at IAO, Hanle, the High Altitude Station of the Indian Institute of Astrophysics, Bangalore, India. This publication makes use of data from the Two Micron All Sky Survey (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...813...52S (acknowledgments)
This work was supported by a Procter Fellowship at Princeton University, and the US Department of Energy Grant DE-AC02-09-CH11466. We would like to thank A. Schekochihin, J. Krommes, I. Rogachevskii, and G. Lesur for enlightening discussion and useful suggestions.
Paper: 2020MNRAS.491L..24I (acknowledgments)
ACKNOWLEDGEMENTS We are grateful to the reviewer for his/her useful comments. We thank Volker Springel for kindly providing the simulation code arepo and Thomas Greif for providing the outputs of his simulations. This study was supported by World Premier International Research Center Initiative (WPI), MEXT, Japan and by SPPEXA through JST CREST JPMHCR1414. SI receives the funding from KAKENHI Grant-in-Aid for Young Scientists (B), No. 17K17677. Final note: This letter is dedicated to our friend and colleague Dr. Thomas H. Greif (1981–2019).
Paper: 2018A&A...616L..13L (acknowledgments)
We thank the referee for her/his suggestions on sharpening the focus of our Letter. PM, GP, MT acknowledge the support from the ERC Consolidator Grant funding scheme ( project STARKEY , G.A. n. 615604).
Paper: 2019A&A...622A..85N (acknowledgments)
The authors would like to thank Timo Reinhold, Alexander Shapiro, and Gibor Basri for useful discussions. MBN and LG acknowledge support from NYUAD Institute grant G1502. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission directorate. 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.
Paper: 2017MNRAS.470.1298P (acknowledgments)
Acknowledgements The research of AP is supported by the Associateship Scheme of ICTP, Trieste and the Ramanujan Fellowship awarded by the Department of Science and Technology, Government of India.
Paper: 2020MNRAS.491.5881Y (acknowledgments)
ACKNOWLEDGEMENTS We are also very grateful to the anonymous referee for her/his instructive comments which significantly improved the content of the paper. This work is supported by the National Key Research and Development Program of China (No. 2017YFA0402703). This work has been supported by the National Science Foundations of China (Nos. 11973029 and 11873032).
Paper: 2018ApJ...867....8P (acknowledgments)
Based on observations obtained at the SOAR telescope, which is a joint project of the Ministério da Ciência, Tecnologia, Inovações e Comunicações (MCTIC) do Brasil, the U.S. National Optical Astronomy Observatory (NOAO), the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU). A.K. gratefully acknowledges support from the German Research Foundation (DFG) via Sonderforschungsbereich SFB 881 (“The Milky Way System,” subproject A08). We thank C.I. Johnson and A. Mucciarelli for useful comments. We thank the referee for the thorough reading of the manuscript and timely suggestions to improve it.
Paper: 2015A&A...575A..34M (acknowledgments)
F.M. thanks the Agence Nationale de la Recherche for financial support (grant ANR-11-JS56-0007). We thank John Hillier for making his atmosphere code CMFGEN available and for constant help with it. G.A.W. acknowledges Discovery Grant support from the Natural Sciences and Engineering Research Council of Canada (NSERC). We thank an anonymous referee for a prompt and positive report.
Paper: 2017MNRAS.470..340P (acknowledgments)
Acknowledgments We thank Alireza Rahmati, Alexandre Refregier and Sergey Koposov for useful discussions, and Robert Crain for kindly providing the data from the EAGLE simulations. This work has made use of the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in the AAS 143, 23. HP's research is supported by the Tomalla Foundation. GK gratefully acknowledges support from the ERC Advanced Grant 320596 ‘The Emergence of Structure During the Epoch of Reionization’.
Paper: 2019ApJ...882...19C (acknowledgments)
K. S. Croker warmly acknowledges: N. Kaiser (ENS) for numerous conversations clarifying the historical understanding of pressure within FLRW models; X. Tata (Hawai‘i) for penetrating feedback and explicit revisions; E. Mottola (LANL) for traveling to Hawai‘i for discussions concerning applications of this work and for pointing out omissions in early arguments; D. Farrah (Hawai‘i) for comments on clarity; J. D. Bjorken (SLAC) for regular correspondence and encouragement; and I. Szapudi (IfA) for criticism, which significantly strengthened the arguments presented. Portions of this work were performed with financial support from the Fulbright U.S. Student Program and the UH Vice Chancellor for Research. Software : Maxima 8 8 http://maxima.sourceforge.net (Maxima 2019 ).
Paper: 2019MNRAS.488.5702B (acknowledgments)
ACKNOWLEDGEMENTS PRB is supported by Track I award OIA-1458952 and is a member of the NANOGrav Physics Frontiers Center, which is supported by National Science Foundation award number 1430284. The Parkes radio telescope is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by the Commonwealth Scientific and Industrial Research Organisation. Data taken at Parkes is available via a public archive. We thank the referee Patrick Weltevrede for valuable comments that helped to improve the text.
Paper: 2017A&A...608A..13L (acknowledgments)
This research has made use of the 2MASS archive, provided by 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. Additionally, this research has made use of the SIMBAD database, operated at CDS, Strasbourg, France.
Paper: 2017A&A...597A.121W (acknowledgments)
This research was primarily supported by the Natural Sciences and Engineering Research Council of Canada (NSERC) through a Canada Graduate Scholarship (J. West) and the Canada Research Chairs and Discovery Grants Programs (S. Safi-Harb). The modeling was performed on a local computing cluster funded by the Canada Foundation for Innovation (CFI) and the Manitoba Research and Innovation Fund (MRIF). The radio images presented in this paper and companion website made use of data obtained with the following facilities: CHIPASS 1.4 GHz radio continuum map, Canadian Galactic Plane Survey (CGPS) and other data from the Dominion Radio Astrophysical Observatory, Southern Galactic Plane Survey, Effelsberg 100 m Telescope and Stockert Galactic plane survey (2720 MHz; via MPIfR’s Survey Sampler), Molonglo Observatory Synthesis Telescope (MOST) Supernova Remnant Catalogue (843 MHz), Sino-German 6 cm survey. Additionally we acknowledge the use of NASA’s SkyView facility ( http://skyview.gsfc.nasa.gov ) located at NASA Goddard Space Flight Center for the data from the 4850 MHz Survey/GB6 Survey, NRAO VLA Sky Survey, Sydney University Molonglo Sky Survey (843 MHz), and the Westerbork Northern Sky Survey (325 MHz Continuum). Very Large Array (VLA) data was acquired via the NRAO Science Data Archive and the Multi-Array Galactic Plane Imaging Survey. We thank Michael Bietenholz and David Kaplan for providing the VLA images of G021.6–00.8 and G042.8+00.6, respectively. This research made use of APLpy, an open-source plotting package for Python ( http://aplpy.github.com ) and Astropy, a community-developed core Python package for Astronomy (Astropy Collaboration 2013). This research also made use of Montage, which is funded by the National Science Foundation under Grant Number ACI-1440620, and was previously funded by the National Aeronautics and Space Administration’s Earth Science Technology Office, Computation Technologies Project, under Cooperative Agreement Number NCC5-626 between NASA and the California Institute of Technology. This research has made use of the NASA Astrophysics Data System (ADS). We thank the referee for comments that improved the manuscript.
Paper: 2016A&A...590A..35D (acknowledgments)
The research leading to these results has received funding from the European Research Council under the European Unions Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement No. 308024. This work was partly supported by the European Union FP7 programme through ERC grant number 320360. The authors would like to thank the anonymous referee for the comments that greatly helped us to improve the paper.