adsabs/WIESP2022-NER huggingface dataset:
Paper: 2019A&A...622A..18S (acknowledgments)
PNB and JS are grateful for support from the UK STFC via grant ST/M001229/1. KJD acknowledges support from the ERC Advanced Investigator programme NewClusters 321271. GG acknowledges the CSIRO OCE Postdoctoral Fellowship. MJH and WLW acknowledge support from the UK Science and Technology Facilities Council (STFC) [ST/M001008/1]. APM would like to acknowledge the support from the NWO/DOME/IBM programme “Big Bang Big Data: Innovating ICT as a Driver For Astronomy”, project #628.002.001. LKM acknowledges support from Oxford Hintze Centre for Astrophysical Surveys, which is funded through generous support from the Hintze Family Charitable Foundation. This publication arises from research partly funded by the John Fell Oxford University Press (OUP) Research Fund. IP acknowledges support from INAF under PRIN SKA/CTA “FORECaST”. The LOFAR group in Leiden is supported by the ERC Advanced Investigator programme New-Clusters 321271. LOFAR, the LOw Frequency ARray designed and constructed by ASTRON, has facilities in several countries, which are owned by various parties (each with their own funding sources) and are collectively operated by the International LOFAR Telescope (ILT) foundation under a joint scientific policy. The ILT resources have benefited from the following recent major funding sources: CNRS-INSU, Observatoire de Paris, and Université d’Orléans, France; BMBF, MIWF-NRW, MPG, Germany; Department of Business, Enterprise and Innovation (DBEI), Ireland; NWO, The Netherlands; and The Science and Technology Facilities Council (STFC), UK. Part of this work was carried out on the Dutch national e-infrastructure with the support of the SURF Cooperative through grant e-infra 160022 and 160152. The LOFAR software and dedicated reduction packages on https://github.com/apmechev/GRID_LRT were deployed on the e-infrastructure by the LOFAR e-infragroup, consisting of J. B. R. Oonk (ASTRON Leiden Observatory), A. P. Mechev (Leiden Observatory), and T. Shimwell (ASTRON) with support from N. Danezi (SURFsara) and C. Schrijvers (SURFsara). This research has made use of the University of Hertfordshire high-performance computing facility ( http://uhhpc.herts.ac.uk/ ) and the LOFAR-UK computing facility located at the University of Hertfordshire and supported by STFC [ST/P000096/1]. The National Radio Astronomy Observatory is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research made use of Astropy, a community-developed core Python package for Astronomy ( Astropy Collaboration 2018 ).
Paper: 2019ApJ...881...47L (acknowledgments)
E.L. is supported by an NSF Astronomy and Astrophysics Postdoctoral Fellowship under award AST-1801937. R.D.M. acknowledges funding support from NSF AST-1714506 and NASA-NNX15AW69G. A.V.’s work was performed under contract with the California Institute of Technology (Caltech)/Jet Propulsion Laboratory (JPL) funded by NASA through the Sagan Fellowship Program executed by the NASA Exoplanet Science Institute. Thank you to R. Esselstein for helpful conversations about stellar rotation periods for this paper. Thank you also to the anonymous referee for careful and thoughtful comments on the manuscript.
Paper: 2015MNRAS.451L..25N (acknowledgments)
This research is supported by the Polish National Science Centre through grant DEC-2012/05/B/ST9/03932. Fruitful discussions with Pawel Moskalik are acknowledged. We also thank Jan Skowron for enlightening discussion about the OGLE photometry.
Paper: 2015MNRAS.453.2465P (acknowledgments)
SS acknowledges support from the Netherlands Organization for Scientific research (NWO), VENI grant 639.041.233. RS acknowledges support from the European Research Council under the European Union (FP/2007-2013)/ERC grant agreement no. 306476. DS acknowledges (i) financial support from the NWO through a Veni fellowship and (ii) funding from FCT through a FCT Investigator Starting Grant and Start-up Grant (IF/01154/2012/CP0189/CT0010) and from FCT grant PEst-OE/FIS/UI2751/2014.
Paper: 2018MNRAS.474.2116D (acknowledgments)
Acknowledgements For useful discussions in the course of this work, we would like to thank Rolf-Peter Kudritzki, Nathan Smith, Justyn Maund and Paul Crowther.
Paper: 2016A&A...587A.150U (acknowledgments)
We are thankful to Raphael Roth and Fortunate Joos for providing data on C production rates and for useful discussions on the carbon cycle. Support by the Academy of Finland to the ReSoLVE Center of Excellence (project no. 272157) and by IPGP through its invitation program is acknowledged. Y.G. and G.K. were partly financed by grant N 14.Z50.31.0017 of the Russian Ministry of Science and Education. This is IPGP contribution No. 3699.
Paper: 2016MNRAS.455.2745K (acknowledgments)
We are extremely grateful to Lyuba Slavcheva-Mihova for providing us with their HST structure map of Mrk 590. Also, we thank Sandra Raimundo for helpful discussions and the anonymous reviewer for insightful comments. We wish to thank the staff of the Nordic and Italian nodes of the European ARC, in particular Ivan Marti-Vidal, for assistance with the data reduction and imaging. We are also indebted to SMA support staff, including Mark Gurwell and Lars Kristensen, for their assistance with the preparation of the SMA proposal, scheduling of observations and data reduction. Travel to the Nordic node of the ARC was made possible through the MARCUs RadioNet3 funding from the European Commission Seventh Framework Programme (FP/2007-2013) under grant agreement no. 283393. JYK is supported by a research grant (VKR023371) from Villumfonden. MV, JYK, and DL gratefully acknowledge support from the Danish Council for Independent Research via grant no. DFF 4002-00275. The Dark Cosmology Centre is funded by the Danish National Research Foundation. The work of VC is partly supported by the Italian Ministero dell′′Istruzione, Università e Ricerca through the grant Progetti Premiali 2012 – iALMA (CUP C52I13000140001). BMP is grateful to the US National Science Foundation for support through grant AST–1008882 to The Ohio State University. This paper makes use of the following ALMA data: ADS/JAO.ALMA#2013.1.00534.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. The National Radio Astronomy Observatory (NRAO) is a facility of the National Science Foundation operated under cooperative agreement by Associated Universities, Inc. This research also makes use of data from the SMA, which is a joint project between the Smithsonian Astrophysical Observatory and the Academia Sinica Institute of Astronomy and Astrophysics and is funded by the Smithsonian Institution and the Academia Sinica. We also used data based on observations made with the NASA/ESA HST , and obtained from the Hubble Legacy Archive, which is a collaboration between the Space Telescope Science Institute (STScI/NASA), the Space Telescope European Coordinating Facility (ST-ECF/ESA) and the Canadian Astronomy Data Centre (CADC/NRC/CSA). The NVAS image used in this paper was produced as part of the NVAS, (c) AUI/NRAO. We acknowledge the use of data from the NASA Extragalactic Database (NED).
Paper: 2018MNRAS.480.2597P (acknowledgments)
ACKNOWLEDGEMENTS This work was supported by the ERC Advanced Investigator Project 267219, the UK Natural Environment Research Council and the Russian Fund for Fundamental Studies (grant 18-02-0057).
Paper: 2018MNRAS.477.1414C (acknowledgments)
Acknowledgements The authors would like to express their gratitude to the computing facilities of IATE and UNC, without which these numerical experiments would not have been possible. We also thank an anonymous referee for valuable comments and suggestions that improved the manuscript. This work was funded by research grants from SECYT/UNC, CONICET, and ANPCyT.
Paper: 2017MNRAS.470.4671R (acknowledgments)
Acknowledgements We wish to thank Jay Anderson for helping us quantify the additional uncertainty introduced by the 180° rotation between epochs. Thanks also to Bo Reipurth for helpful conversations. MR would like to thank John Bieging, Tom Haworth and Chris Miller. HH numbers are assigned by Bo Reipurth in order to correspond with the catalogue of HH objects maintained at http://ifa.hawaii.edu/reipurth/ ; see also Reipurth Reiter (2017), A General Catalog of Herbig-Haro Objects , 3rd Edition, in preparation. Support for this work was provided by NASA through grants AR-12155, GO-13390 and GO-13391 from the Space Telescope Science Institute. This work is based on observations made with the NASA/ESA Hubble Space Telescope , obtained from the Data Archive at the Space Telescope Science Institute, which is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS 5-26555. These HST observations are associated with programmes GO 10241, 10475, 13390 and 13391.
Paper: 2015MNRAS.451.4346S (acknowledgments)
Data from ESO FEROS programme ID 078.C-0493(A) and FLAMES programme 171.D-0237(B) were taken from the ESO archive. This research has made use of the simbad (Wenger et al. 2000 ) Database, operated at CDS, Strasbourg, France and the ESO Archive. JVS thanks the ESO Director General Discretionary Fund and Queen's University Belfast Visiting Scientist Fund for financial support. We would like to thank two anonymous referees whose comments significantly improved the paper.
Paper: 2019ApJ...877..104Z (acknowledgments)
The authors thank the anonymous referee for useful comments that improved this paper. We also thank Jane Lin for helpful discussions on stellar mass for the Li-rich giants. This research was supported by the National Key Basic Research Programme of China 2014CB845700, and by the National Natural Science Foundation of China under grant Nos. 11833006, 11603037, and 11473033. This work is supported by the Astronomical Big Data Joint Research Center, cofounded by the National Astronomical Observatories, Chinese Academy of Sciences and the Alibaba Cloud. K.P. acknowledges support from the Mt. Cuba Astronomical Foundation Grant and from Center for Astronomical Megascience, CAS. Guoshoujing Telescope (the Large Sky Area Multi-Object Fiber Spectroscopic Telescope LAMOST) is a National Major Scientific Project built by the Chinese Academy of Sciences. Funding for the project has been provided by the National Development and Reform Commission. LAMOST is operated and managed by the National Astronomical Observatories, Chinese Academy of Sciences. This publication makes use of data products from the Wide field Infrared Survey Explorer, which is a joint project of the University of California, Los Angeles, and the Jet Propulsion Laboratory/California Institute of Technology, funded by the National Aeronautics and Space Administration. Based on data products from observations made with ESO Telescopes at the La Silla Paranal Observatory under programme ID 188.B-3002. This research made use of Astropy, a community-developed core Python package for Astronomy. Software: Astropy (Astropy Collaboration et al. 2013 , 2018 ), PARAM (da Silva et al. 2006 ), SPECTRUM (Gray Corbally 1994 ), MARCS (Gustafsson et al. 2008 ).
Paper: 2019ApJ...873..126M (acknowledgments)
The authors are grateful to the anonymous referee for constructive comments. The authors thank Doug Gilliam (NSO) and Michiel Van Noort (MPS) for their valuable support during the acquisition and MOMFBD processing of the data. S.L.G. and F.Z. are supported by Università degli Studi di Catania (Linea di intervento 1 e Linea di intervento 2). The research leading to these results has received funding from the European Research Council under the European Union’s Horizon 2020 Framework Programme for Research and Innovation, grant agreements H2020 PRE-EST (No. 739500) and H2020 SOLARNET (No. 824135). This work was also supported by INAF Istituto Nazionale di Astrofisica (PRIN-INAF-2014). S.J. acknowledges support from the European Research Council under the European Unions Horizon 2020 research and innovation program (grant agreement No. 682462) and from the Research Council of Norway through sits Centres of Excellence scheme (project No. 262622).
Paper: 2020MNRAS.492.2535G (acknowledgments)
ACKNOWLEDGEMENTS We thank Steve Warren for helpful comments on an earlier version of this paper. This work was supported by the Science and Technology Facilities Council (STFC) grants ST/L00075X/1 and ST/P000541/1. AJG acknowledges an STFC studentship funded by STFC grant ST/N50404X/1. CDL has received funding from the ARC Centre of Excellence for All Sky Astrophysics in 3 Dimensions (ASTRO 3D), through project number CE170100013. CDL also thanks the Mobilising European Research in Astrophysics and Cosmology (MERAC) Foundation for a Postdoctoral Research Award. This work used the DiRAC Data Centric system at Durham University, operated by the Institute for Computational Cosmology on behalf of the STFC DiRAC High Performance Computing (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.
Paper: 2019MNRAS.487.1269S (acknowledgments)
ACKNOWLEDGEMENTS We thank the anonymous referee for valuable comments. M.J. acknowledges the support of the Academy of Finland Grant No. 285769. P.C. acknowledges the support of the ERC Advanced grant PALs 320620.
Paper: 2015MNRAS.451.3055B (acknowledgments)
The author is really thankful to the anonymous referee for numerous comments, which led to a significant improvement of the manuscript. The author is also grateful to C.J. Pethick and D.G. Yakovlev for discussions. This work was supported by RSF, grant no. 14-12-00316.
Paper: 2015ApJ...802...50C (acknowledgments)
We thank the anonymous referee for a careful reading of the manuscript and helpful suggestions that strengthened this paper greatly. We thank our colleagues on the AGES, ISS, SDWFS, NDWFS, and the XBoötes teams and the HerMES team for making the data publicly available. The first Spitzer MIPS survey of the Boötes region was obtained using GTO time provided by the Spitzer Infrared Spectrograph Team (PI, James Houck) and by M. Rieke. We thank the collaborators in that work for access to the 24 μ m catalog generated from those data by Emeric Le Floc’h. This work was supported under Contract NAS8-03060. R.J.A. was supported by Gemini-CONICYT Grant 32120009. K.N.H and R.C.H. were partially supported by NASA through ADAP Award NNX12AE38G and by the National Science Foundation through Grant 1211096. This work was also supported by Science and Technologies Facilities Council (STFC) grant ST/I001573/1 (D.M.A. and A.D.M.) and the Leverhulme Trust (D.M.A.). R.C.H. acknowledges support from an Alfred P. Sloan Research Fellowship and Dartmouth Class of 1962 Faculty Fellowship. C.-T.J.C was supported by a Dartmouth Fellowship and the William H. Neukom 1964 Institute for Computational Science.
Paper: 2019MNRAS.487..782L (acknowledgments)
ACKNOWLEDGEMENTS The research was supported by an Australian Research Council grant DE180101104. Funding for the Stellar Astrophysics Centre is provided by the Danish National Research Foundation (Grant DNRF106). 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: 2019ApJ...878...42E (acknowledgments)
The authors thank the anonymous reviewer for a careful reading of this manuscript and providing thoughtful feedback that improved this paper. We also thank Alis Deason for assistance in line-list vetting, Gina Duggan for useful discussions on generating grids of synthetic spectra, Raja Guha Thakurta for help with observations and insightful conversations, and Luis Vargas and Marla Geha for sharing their data for M31 outer halo RGB stars. I.E. acknowledges support from a Ford Foundation Predoctoral Fellowship and the NSF Graduate Research Fellowship under grant No. DGE-1745301, as well as the NSF under grant No. AST-1614081, along with E.N.K. K.M.G. and J.W. acknowledge support from NSF grant AST-1614569. E.C.C. was supported by an NSF Graduate Research Fellowship as well as NSF grant No. AST-1616540. The analysis pipeline used to reduce the DEIMOS data was developed at UC Berkeley with support from NSF grant AST-0071048.
Paper: 2018ApJ...856...29M (acknowledgments)
This work was supported in part by the Theoretical Astrophysics Center at UC Berkeley. D.K. is supported in part by a Department of Energy Office of Nuclear Physics Early Career Award, and by the Director, Office of Energy Research, Office of High Energy and Nuclear Physics, Divisions of Nuclear Physics, of the U.S. Department of Energy under Contract No. DE-AC02-05CH11231. Numerical computations utilized the Savio computational cluster resource provided by the Berkeley Research Computing program at the University of California, Berkeley (supported by the UC Berkeley Chancellor, Vice Chancellor of Research, and Office of the CIO).
Paper: 2015MNRAS.451L..50T (acknowledgments)
We are grateful to the referee S. Johnston for very useful comments, to A. Jessner, D. Schnitzeler and D. Riquelme for discussions, to P. Lazarus for sharing code, and to C. Ng for reading the manuscript. Partly based on observations with the 100-m telescope of the MPIfR at Effelsberg. The Nançay radio observatory is operated by the Paris Observatory, associated with the French CNRS. IRAM is supported by INSU/CNRS (France), MPG (Germany), and IGN (Spain). APEX is a collaboration between the MPIfR, the European Southern Observatory, and the Onsala Space Observatory. Financial support by the European Research Council for the ERC Synergy Grant BlackHoleCam (ERC-2013-SyG, Grant Agreement no. 610058) is gratefully acknowledged. PT is supported for this research through a stipend from the International Max Planck Research School (IMPRS) for Astronomy and Astrophysics at the Universities of Bonn and Cologne.
Paper: 2016MNRAS.460..478L (acknowledgments)
ML and AB were supported by the DOE (Grant No. DE-AC02-09CH-11466) and the NSF (Grant No. AGS-1338944) during the course of this work. ML is grateful to Gordon Ogilvie for his encouraging comments regarding a preliminary version of the manuscript. ML is thankful to Santiago Benavides and Pallavi Bhat for their insightful assistance.
Paper: 2016ApJ...817...26B (acknowledgments)
I am grateful to T. Baker and M. G. Santos for extensive discussions, and acknowledge Y. Akrami, S. Camera, P. G. Ferreira, A. Raccanelli, J.-P. Uzan, M. Viel, F. Villaescusa-Navarro, and K. Zarb-Adami for useful comments and suggestions. I was supported by European Research Council grant StG2010-257080. The code and Fisher matrices used in this paper are available from http://philbull.com/mg_ska/ .
Paper: 2018ApJ...866..134G (acknowledgments)
This project has received funding from the US Department of Energy under grant DE-FG02-04ER54742, the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 795158, the Shota Rustaveli National Science Foundation of Georgia (SRNSFG; grant number FR17-107), and the Space and Geophysics Laboratory at the University of Texas at Austin. G.M. acknowledges support from the Alexander von Humboldt Foundation (Germany). The simulations were performed at the Texas Advanced Computing Center in Austin (TX) and on the high-performance Linux cluster Hydra at the Helmholtz-Zentrum Dresden-Rossendorf (Germany).
Paper: 2016MNRAS.462.1757G (acknowledgments)
We thank the anonymous referee for helpful comments. We also thank Jarle Brinchmann, Anna Feltre, Brent Groves, Alba Vidal-García, Aida Wofford and the entire NEOGAL team for valuable discussions. We acknowledge support from the ERC via an Advanced Grant under grant agreement no. 321323-NEOGAL. GB acknowledges the hospitality and support from CNRS/IAP during different stages of this investigation, as well as support for this work from the National Autonomous University of México (UNAM) through grant PAPIIT IG100115. Funding for the creation and distribution of the SDSS Archive has been provided by the Alfred P. Sloan Foundation, the Participating Institutions, the National Aeronautics and Space Administration, the National Science Foundation, the US Department of Energy, the Japanese Monbukagakusho and the Max Planck Society. The SDSS website is http://www.sdss.org/ .
Paper: 2018MNRAS.479.2161G (acknowledgments)
ACKNOWLEDGEMENTS This work was supported in part by the bequest of William Herschel Womble in support of astronomy at the University of Denver. JG thanks the University of Denver Undergraduate Research Center for a Partners in Scholarship (PinS) grant, and the Native American Scholarship fund that helped his efforts in this research. An earlier version of this paper appeared as https://arxiv.org/abs/1612.05287 . The authors are grateful to the Astronomical Research Consortium (ARC) that operates the Apache Point Observatory 3.5 m telescopes and its ARCES and TripleSpec instruments that provided the bulk of the data reported in this paper. We thank Matthew Muterspaugh (Tennessee State University) for access to late-eclipse time-series data generated by Joel Eaton with their Automated Spectroscopy Telescope (AST), review of which led us to re-examine the ARCES data during third-contact (see section 3.4: Details of Stream Appearance). We also want to acknowledge observers and APO programme leaders including Alaina Bradley, Jack Dembicky, Suzanne Hawley, Joseph Huehnerhoff, Russet McMillan, Sarah Schmidt, Nicholas Ule, Donald G. York, George Wallerstein, the APO staff, and others for their contributions to the ARCES and TripleSpec data collection process. We appreciate helpful comments from the reviewer and editor.
Paper: 2015MNRAS.449..685H (acknowledgments)
We thank Monique Arnaud, Gabriel Pratt, Keiichi Umetsu, James Jee, Edo van Uitert, Anja von der Linden, Doug Applegate, Ken Rines and Douglas Scott for useful discussions. We are also grateful to Keiichi Umetsu and James Jee for providing some of their Subaru images, and to Anja von der Linden for sharing the WtG lensing catalogues. HH and MC were supported by the Netherlands organization for Scientific Research (NWO) Vidi grant 639.042.814; HH, RH and MV acknowledge support from the European Research Council FP7 grant number 279396. AB would like to acknowledge research funding from NSERC Canada through its Discovery Grant program. AM acknowledges support from NASA ADAP grant NNX12AE45G. This research used the facilities of the Canadian Astronomy Data Centre operated by the National Research Council of Canada with the support of the Canadian Space Agency.
Paper: 2015MNRAS.448.3731R (acknowledgments)
We thank Laura Bonavera for assisting with the C2499 ATCA observations of this project. We wish also to thank Mark Wieringa for the support on the miriad data reduction and Piero Ullio for insightful discussions during the early stages of the project. SC acknowledges support by the South African Research Chairs Initiative of the Department of Science and Technology and National Research Foundation and by the Square Kilometre Array (SKA). SP is partly supported by the US Department of Energy, Contract DE-FG02-04ER41268. MR acknowledges support by the research grant TAsP ( Theoretical Astroparticle Physics ) funded by the Istituto Nazionale di Fisica Nucleare (INFN). The ATCA is part of the Australia Telescope National Facility which is funded by the Commonwealth of Australia for operation as a National Facility managed by CSIRO.
Paper: 2016ApJ...820...97C (acknowledgments)
M.Ć. acknowledges support from NASA’s Outer Planets Research Program, awards NNX11AM48G and NNX14AOO38G. We thank an anonymous reviewer for very insightful comments that greatly improved the paper.