adsabs/WIESP2022-NER huggingface dataset:
Paper: 2018MNRAS.481.5470X (acknowledgments)
ACKNOWLEDGEMENTS We thank Kyle Dawson and Xiaohu Yang for useful discussions. HX acknowledges the support by a fellowship from the Willard L. and Ruth P. Eccles Foundation. IZ is supported by NSF grant AST-1612085. During the final stage, this project has been supported by a grant from Science and Technology Commission of Shanghai Municipality (Grants No.16DZ2260200) and National Natural Science Foundation of China (Grants No.11655002). We gratefully acknowledge the High Performance Computing Resource for Advanced Research Computing at Shanghai Astronomical Observatory. The support and resources from the Center for High Performance Computing at the University of Utah are gratefully acknowledged. The authors gratefully acknowledge the Gauss Centre for Supercomputing e.V. ( www.gauss-centre.eu ) and the Partnership for Advanced Supercomputing in Europe (PRACE, http://www.prace-ri.eu ) for funding the MultiDark simulation project by providing computing time on the GCS Supercomputer SuperMUC at Leibniz Supercomputing Centre (LRZ, http://www.lrz.de ). The CosmoSim database used in this paper is a service by the Leibniz-Institute for Astrophysics Potsdam (AIP). The MultiDark database was developed in cooperation with the Spanish MultiDark Consolider Project CSD2009-00064. Funding for the SDSS and SDSS-II has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Science Foundation, the U.S. 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/ . The SDSS is managed by the Astrophysical Research Consortium for the Participating Institutions. The Participating Institutions are the American Museum of Natural History, Astrophysical Institute Potsdam, University of Basel, University of Cambridge, Case Western Reserve University, University of Chicago, Drexel University, Fermilab, the Institute for Advanced Study, the Japan Participation Group, Johns Hopkins University, the Joint Institute for Nuclear Astrophysics, the Kavli Institute for Particle Astrophysics and Cosmology, the Korean Scientist Group, the Chinese Academy of Sciences (LAMOST), Los Alamos National Laboratory, the Max-Planck-Institute for Astronomy (MPIA), the Max-Planck-Institute for Astrophysics (MPA), New Mexico State University, Ohio State University, University of Pittsburgh, University of Portsmouth, Princeton University, the United States Naval Observatory, and the University of Washington.
Paper: 2018MNRAS.475L..57C (acknowledgments)
ACKNOWLEDGEMENTS The Parkes Observatory is part of the Australia Telescope National Facility which is funded by the Australian Government for operation as a National Facility managed by Commonwealth Scientific and Industrial Research Organisation. The Green Bank Observatory is a facility of the National Science Foundation (NSF) operated under cooperative agreement by Associated Universities, Inc. Pulsar research at the Jodrell Bank Centre for Astrophysics and the observations using the Lovell Telescope are supported by a consolidated grant from the Science and Technology Facilities Council in the UK. This work is also based on observations with the 100-m telescope of the Max-Planck-Institut für Radioastronomie at Effelsberg. This work is supported by the ARC Centres of Excellence CE110001020 (CAASTRO) and CE170100004 (OzGrav). Survey processing was conducted in association with CAASTRO at the Australian National Computational Infrastructure high-performance computing centre at the Australian National University. The authors wish to thank Marina Berezina, Eleni Graikou, Alex Kraus, and Laura Spitler for their assistance with observations at Effelsberg, along with Natalia Lewandowska and Ryan Lynch for their assistance with observations at the GBT. We also thank West Virginia University for its financial support of GBT operations, which enabled some of the observations for this project. ADC acknowledges the support of both the International Max Planck Research School for Astronomy and Astrophysics at the Universities of Bonn and Cologne, and the Bonn-Cologne Graduate School of Physics and Astronomy. PCCF and AR gratefully acknowledge financial support by the European Research Council (ERC) for the ERC Starting grant BEACON under contract No. 279702, and continued support from the Max Planck Society. MK, RK, and RPE gratefully acknowledge support from ERC Synergy Grant ‘BlackHoleCam’ Grant Agreement Number 610058. MAM was supported by NSF award number AST-1517003. DRL was supported by NSF award number OIA-1458952.
Paper: 2016MNRAS.462.4171B (acknowledgments)
This work was supported by Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (sub-projects B1, B2, B5 and B8) of the German Research Foundation (DFG) and SPP 1573, ‘Physics of the Interstellar Medium’ (grant number GL 668/2-1). In addition, RSK acknowledges support from the European Research Council under the European Community's Seventh Framework Programme (FP7/2007-2013) via the ERC Advanced Grant STARLIGHT (project number 339177). The numerical simulations presented in this work were performed on the Milky Way supercomputer, which is funded by the Deutsche Forschungsgemeinschaft (DFG) through the Collaborative Research Center (SFB 881) ‘The Milky Way System’ (subproject Z2) and hosted and co-funded by the Jülich Supercomputing Center (JSC). The authors thank the anonymous referee for helpful and constructive comments. CBM thanks Patrick Hennebelle, Pavel Kroupa, Tilman Hartwig and Scott Trager for helpful discussions.
Paper: 2019MNRAS.488.1111T (acknowledgments)
ACKNOWLEDGEMENTS JET and SC acknowledge support from the Natural Sciences and Engineering Research Council (NSERC) of Canada through respective Discovery Grants. NNQO acknowledges support from NSERC through a PGS D scholarship. We thank the anonymous referee for several comments and questions that improved the paper significantly. We also thank B. Tully, M. Hudson, N. Dalal, and the participants of the conference ‘The Physics of Galaxy Scaling Relations and the Nature of Dark Matter’ held at Queen’s University in July 2018 for many useful comments on a preliminary version of this work. This work made use of the VizieR catalogue access tool, CDS, Strasbourg, France (DOI : 10.26093/cds/vizier; https://vizier.u-strasbg.fr/vizier ). The original description of the VizieR service was published in AAS 143, 23.
Paper: 2015ApJ...809...89T (acknowledgments)
We are indebted to the staff of the W.M. Keck Observatory who keep the instruments and telescopes running effectively. We also wish to extend thanks to those of Hawaiian ancestry on whose sacred mountain we are privileged to be guests. This work has been supported in part by the US National Science Foundation through grants AST-0908805 and AST-1313472. We thank Mariska Kriek and Eliot Quataert for many useful discussions as well as the anonymous referee for comments and suggestions that significantly improved this work. R.F.T. also acknowledges support from Dennis and Carol Troesh and from the Miller Institute for Basic Research in Science at the University of California, Berkeley.
Paper: 2020MNRAS.492..770G (acknowledgments)
ACKNOWLEDGEMENTS ARG-J thanks the financial support of Coordenação de Aperfeiçoamento de Pessoal de Nível Superior – Brasil (CAPES), Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq), and Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP) (proc. 2018/11239-8). MA thanks CNPq (Grants 427700/2018-3, 310683/2017-3, and 473002/2013-2) and Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro (FAPERJ) (grant E-26/111.488/2013). FB-R acknowledges CNPq grant 309578/2017-5. GB-R is thankful for the support of CAPES/Brazil and FAPERJ (grant E26/203.173/2016). BM thanks the CAPES/Cofecub-394/2016-05 grant. RV-M acknowledges grants CNPq: 304544/2017-5, 401903/2016-8, Faperj: PAPDRJ-45/2013 and E-26/203.026/2015, CAPES/Cofecub: 2506/2015. JIBC acknowledges CNPq grant 308150/2016-3. Based on observations obtained at the SOAR telescope, which is a joint project of the Ministério da Ciência, Tecnologia, Inovações e Comunicações do Brasil, the U.S. National Optical Astronomy Observatory, the University of North Carolina at Chapel Hill (UNC), and Michigan State University (MSU). Based on data obtained at Complejo Astronómico El Leoncito, operated under agreement between the Consejo Nacional de Investigaciones Cientf́icas y Técnicas de la República Argentina and the National Universities of La Plata, Córdoba and San Juan. The work was based on observations made at the Laboratório Nacional de Astrofísica (LNA), Itajubá-MG, Brazil. TRAPPIST-South is funded by the Belgian Fund for Scientific Research under the grant FRFC 2.5.594.09.F. EJ is a Belgian FNRS Senior Research Associates. The work was based on observations made by MiNDSTEp from the Danish 1.54 m telescope at ESO’s La Silla observatory. This collaboration, as part of the Encelade working group ( http://www.issibern.ch/teams/encelade/ ), has been supported by the International Space Sciences Institute in Bern, Switzerland. Part of the research leading to these results has received funding from the European Research Council under the European Communitys H2020 (2014–2020/ERC grant 669416 ‘LUCKY STAR’)
Paper: 2016MNRAS.458.2870V (acknowledgments)
We are grateful to the people responsible for the Bolshoi and MultiDark simulations for making their halo catalogues publicly available, to the anonymous referee for an insightful report that greatly helped to improve the presentation, and to the following individuals for their advice and assistance: Peter Behroozi, Mike Boylan-Kolchin, Carlo Giocoli, Andrew Hearin, Anatoly Klypin, Alexander Knebe, Surhud More, Nikhil Padmanabhan, Tomomi Sunayama, and Bepi Tormen.
Paper: 2016MNRAS.462.3255C (acknowledgments)
We thank the referee for their comments and criticisms that have significantly improved this work. We are grateful to David Bacon, Bob Nichol, Dominique Sluse, Kenneth Wong and Phil Marshall for insightful comments on the original manuscript. We thank Tommaso Treu and Paul Schechter for helpful discussions. SDC acknowledges funding from the SEPNet summer placement scheme and is grateful to the ICG for hosting the placement. This project made use of the lenspop code which is freely available from github.com/tcollett/LensPop. Numerical computations were done on the Sciama High Performance Compute (HPC) cluster which is supported by the ICG, SEPNet and the University of Portsmouth.
Paper: 2019MNRAS.489L..22A (acknowledgments)
ACKNOWLEDGEMENTS It is a pleasure to thank Simon White and Adriano Agnello for inspiring discussions.
Paper: 2016MNRAS.461...79D (acknowledgments)
MGBA acknowledges the financial support from FAPESP 2011/23996-9 and from the FAPESP Thematic Project 2013/26258-4. MGBA is also grateful to the Kapteyn Astronomical Institute for the hospitality and to R. Misra, M. Linares, P. Bult and T. Strohmayer for the useful comments. DA acknowledges support from the Royal Society. The authors are grateful to the unknown referee for his/her meticulous review of this paper whose comments significantly increased the value of our work.
Paper: 2017A&A...606A.131G (acknowledgments)
This research has made use of the GOLDmine database (Gavazzi et al. 2003, 2014b) and of 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.452.1105B (acknowledgments)
We thank Martin Haehnelt, Daniel Mortlock and Steve Warren for their helpful comments on the manuscript, as well as Paul Hewett for assistance in the early stages of this work. We also thank the referee, Xiaohui Fan, for comments which helped to improve the manuscript. SEIB acknowledges a Graduate Studentship from the Science and Technology Funding Council (STFC) and is grateful for funding through the ERC grant LGAG/209 RG66659. GDB has been supported by STFC through an Ernest Rutherford Fellowship.
Paper: 2018ApJ...860..122C (acknowledgments)
We warmly thank Diana Valencia for interesting discussions on the internal composition of planets, Florentin Millour for explanations concerning the Hipparcos catalog, Georges Kordopatis, Orlagh Creevey and Mathias Schultheis for insights on stellar models and populations. R.L. is funded by the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie grant agreement n. 664931. C.D. is funded by the Swiss National Science Foundation under the Ambizione grant PZ00P2_174028.
Paper: 2018ApJ...859...59B (acknowledgments)
We thank the US National Science Foundation (AST-1505502) for support in conducting the present experiments. The authors acknowledge the W. M. Keck Foundation for financing the experimental setup.
Paper: 2017MNRAS.466..425W (acknowledgments)
Acknowledgments The authors thank Clive Dickinson and Patrick Leahy for useful discussions and comments on the manuscript. We also acknowledge useful discussions with Pascal Rideau and Joel Michaud concerning practical constraints related to data transfer and to attitude and orbit control. CGRW acknowledges the award of an STFC quota studentship the support of the Engineering and Physical Sciences Research Council (grant no. EP/M011852/1). MLB acknowledges the European Research Council for support through the award of an ERC Starting Independent Researcher Grant (EC FP7 grant no. 280127). MLB also thanks the STFC for the award of Advanced and Halliday fellowships (grant no. ST/I005129/1). Some of the results in this paper have been derived using the healpix (Grski etal. 2005 ) package.
Paper: 2015ApJ...808...16N (acknowledgments)
We would like to thank Daniel Foreman-Mackey (NYU), Morgan Fouesneau (MPIA), Jon Holtzman (NMSU), Keivan Stassun (Vanderbilt University), Jennifer Johnson (OSU), and David Sontag (NYU) for valuable discussions. D.W.H. was partially supported by the NSF (grant IIS-1124794), NASA (grant NNX08AJ48G), and the Moore–Sloan Data Science Environment at NYU. The research has received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP 7) ERC Grant Agreement No. [321035]. 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.
Paper: 2016A&A...591A.140G (acknowledgments)
This paper made use of spectroscopic data that were obtained at the FLWO-1.5 m with FAST, which is operated by Harvard-Smithsonian Centre for Astrophysics. In particular we want to thank Perry Berlind and Mike Calkins for their role in obtaining most of the FLWO-1.5 m/FAST data. The paper also makes use of data obtained as part of the INT Photometric H Survey of the Northern Galactic Plane (IPHAS) carried out at the Isaac Newton Telescope (INT). The INT is operated on the island of La Palma by the Isaac Newton Group in the Observatorio del Roque de los Muchachos of the Instituto de Astrofísica de Canarias. All IPHAS data are processed by the Cambridge Astronomical Survey Unit, at the Institute of Astronomy in Cambridge. We also acknowledge the use of data obtained at the INT and the Nordic Optical Telescope as part of a CCI International Time Programme. The work of L.G. and J.F. is supported by the Spanish Ministerio de Economía y Competitividad, and FEDER, under contracts AYA2010-18352 and AYA2013-48623-C2-2-P, and by the Generalitat Valenciana project of excellence PROMETEOII/2014/060. R.R. received funding from the European Research Council under the European Union’s Seventh Framework Programme (FP/2007-2013)/ERC Grant Agreement No. 320964 (WDTracer). N.J.W. was supported by a Royal Astronomical Society fellowship. Finally, we are grateful to Dr. Pablo Reig for his assistance in the classification in the MK system.
Paper: 2017MNRAS.469.2704H (acknowledgments)
Acknowledgments The observational data for PSR J0738-4042 (at 1375 MHz) and PSR J1022+1001 (at 728 MHz) were obtained from the EPN data base under the Creative Commons Attribution 4.0 International licence. The numerical code that supports the plots and diagrams within this paper, as well as the relevant parameters of modelling, is available from the authors upon reasonable request. We thank Ya.N. Istomin, B. Stappers and P. Weltevrede for their interest and useful discussions and the anonymous referee for instructive comments that helped us to improve the manuscript. This work was partially supported by Russian Foundation for Basic Research (Grant no. 14-02-00831). AAP is supported by Porter Ogden Jacobus Fellowship, awarded by the graduate school of Princeton University.
Paper: 2019ApJ...874...27T (acknowledgments)
We acknowledge the detailed comments from the anonymous referee. We thank K. Nakanishi, F. Egusa, R. Kawamata, Y. Harikane, M. Ouchi, P. Papadopoulos, and M. Michałowski for fruitful suggestions. This work was supported by NAOJ ALMA Scientific Research Grant Numbers 2018-09B, 2016-01A, and JSPS/MEXT KAKENHI (No. 17H06130, 17H04831, 17KK0098, 17H01110, 18H04333, 17K14252, and 17H01110). E.Z. acknowledges funding from the Swedish National Space Board. T.T.T. is supported by a Sumitomo Foundation Grant for Basic Science Projects (180923). This paper makes use of the following ALMA data: ADS/JAO.ALMA #2016.1.00117, ADS/JAO.ALMA #2013.1.00999.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. This work is also based on observations collected at the European Organisation for Astronomical Research in the Southern Hemisphere under ESO programme 0100.A-0529(A). Some of the data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. 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. IRAF is distributed by the National Optical Astronomy Observatory, which is operated by the Association of Universities for Research in Astronomy (AURA) under a cooperative agreement with the National Science Foundation.
Paper: 2018MNRAS.480.4244C (acknowledgments)
ACKNOWLEDGEMENTS The authors would like to thank the referee for their insightful comments that improved the quality of this manuscript. The authors are also grateful to Jo Bovy and Alice Quillen for useful conversations, Jacob Bauer for his assistance with the simulations, and Eugene Vasiliev for his help with an early version of agama and comments on the original manuscript. We also acknowledge the use of computational resources at Compute Canada and the Centre for Advanced Computing. This work was supported by the Natural Sciences and Engineering Research Council of Canada through the Postgraduate Scholarship Program (MHC) and Discovery Grant Program (LMW).
Paper: 2018MNRAS.478.3266M (acknowledgments)
ACKNOWLEDGEMENTS MV is supported by INFN/PD51 Indark, PRIN-INAF, PRIN-MIUR, and ERC-StG (European Research Council-Starting Grant) ‘cosmoIGM’ grants under ERC Grant agreement 257670-cosmoIGM. TSK is supported by ERC-StG ‘cosmoIGM’. TSK also acknowledges the support from ‘NSF-AST118913’. CM wishes to thank D. Goz, E. Munari, and A. Zoldan for useful discussion. We are grateful to an anonymous referee who provided very useful comments that allowed us to clarify several points in the paper.
Paper: 2019MNRAS.489..196M (acknowledgments)
ACKNOWLEDGEMENTS The Atmospheric Chemistry Experiment (ACE), also known as SCISAT, is a Canadian-led mission mainly supported by the Canadian Space Agency. EJRM is funded by a McGill Science Undergraduate Research Award. The authors thank Yi Huang for his insight on the ACE-FTS data and on stratospheric clouds, Mark Swain for the idea of investigating Earth’s sodium layer, and Emily Pass for her helpful comments on this work. We also thank Yan Bétrémieux, Tyler Robinson, and an anonymous referee for their comments, which significantly improved this work. NBC acknowledges funding from NSERC and FRQNT.
Paper: 2019ApJ...885..162X (acknowledgments)
We would like to thank the anonymous referee for very helpful comments, which help to improve the paper significantly. This work is partially supported by the National Key RD Program of China 2018YFA0404203 and 2018YFA0404204, NSFC grants U1738122, U1931204 and 11761131007, the Natural Science Foundation for Young Scholars of Jiangsu Province, China (No. BK20191109), and by the International Partnership Program of Chinese Academy of Sciences, grant No.114332KYSB20170008.
Paper: 2018MNRAS.478.2291C (acknowledgments)
ACKNOWLEDGEMENTS I thank P. Behroozi and C. Pacifici for the inspiring discussions to work on this, to B. Diemer, G. Lemson, Y. Feng for help in various steps of obtaining and analysing the data, and many others for conversations, comments, and questions, including S. Alam, M. van Daalen, N. Dalal, R. Dave, and A. Kravtsov. I also thank other participants at the Santa Barbara Galaxy-Halo connection workshop in June 2017, members of the Royal Observatory of Edinburgh, and participants at the Berkeley Center for Cosmological physics workshop and Nordita workshop in July 2017 for the opportunity to talk on this work and for their feedback and suggestions, and the Royal Observatory and Nordita for their kind hospitality. B. Diemer and C. Pacifici generously provided many helpful suggestions and criticisms of an earlier draft. I am especially grateful to M. White for innumerable discussions and suggestions, as well as encouragement. I also thank the referee for many helpful suggestions and questions. The Millennium simulation data bases used in this paper and the web application providing online access to them were constructed as part of the activities of the German Astrophysical Virtual Observatory (GAVO).