期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 486, 期 2, 页码 2169-2183出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stz960
关键词
catalogues; subdwarfs; white dwarfs; stars: fundamental parameters; cataclysmic variables
资金
- Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior - Brasil (CAPES) [001]
- Conselho Nacional de Desenvolvimento Cientifico e Tecnologico - Brasil (CNPq)
- Fundacao de Amparo a Pesquisa do Rio Grande do Sul (FAPERGS) - Brasil
- Deutsche Forschungsgemeinschaft [GE2506/12-1]
- Alfred P. Sloan Foundation
- U.S. Department of Energy Office of Science
- Center for High-Performance Computing at the University of Utah
- Brazilian Participation Group
- Carnegie Institution for Science, Carnegie Mellon University
- Chilean Participation Group
- French ParticipationGroup
- Harvard-Smithsonian Center for Astrophysics
- Instituto de Astrofisica de Canarias
- Johns Hopkins University
- Kavli Institute for the Physics and Mathematics of the Universe (IPMU)/University of Tokyo
- Lawrence Berkeley National Laboratory
- Leibniz Institut fur Astrophysik Potsdam (AIP)
- Max-Planck-Institut fur Astronomie (MPIA Heidelberg)
- Max-Planck-Institut fur Astrophysik (MPA Garching)
- Max-Planck-Institut fur Extraterrestrische Physik (MPE)
- National Astronomical Observatories of China
- New Mexico State University
- New York University
- University of Notre Dame
- Observatario Nacional/MCTI
- Ohio State University
- Pennsylvania State University
- Shanghai Astronomical Observatory
- United Kingdom Participation Group
- Universidad Nacional Autonoma de Mexico
- University of Arizona
- University of Colorado Boulder
- University of Oxford
- University of Portsmouth
- University of Utah
- University of Virginia
- University of Washington
- University of Wisconsin
- Vanderbilt University
- Yale University
- Algerian Centre de Recherche en Astronomie, Astrophysique et Geophysique of Bouzareah Observatory
- Austrian Fonds zur Forderung der wissenschaftlichen Forschung (FWF) Hertha Firnberg Programme [T359, P20046, P23737]
- BELgian federal Science Policy Office (BELSPO) through various PROgramme de D'eveloppement d'Experiences scientifiques (PRODEX) grants
- Polish Academy of Sciences -Fonds Wetenschappelijk Onderzoek [VS.091.16N]
- Brazil-France exchange programme Fundacao de Amparo a Pesquisa do Estado de Sao Paulo (FAPESP)
- Chilean Direccion de Gestion de la Investigacion (DGI) at the University of Antofagasta
- Comite Mixto ESO-Chile
- National Science Foundation of China (NSFC) [11573054, 11703065]
- Czech-Republic Ministry of Education, Youth, and Sports [LG 15010]
- Czech Space Office through ESA PECS [98058]
- Charles University Prague [PRIMUS/SCI/17]
- Danish Ministry of Science
- Estonian Ministry of Education and Research [IUT40-1]
- European Commission's Sixth Framework Programme through the European Leadership in Space Astrometry (ELSA) Marie Curie Research Training Network [MRTN-CT-2006-033481]
- European Commission's Sixth Framework Programme through Marie Curie project [PIOF-GA-2009-255267]
- European Commission's Sixth Framework Programme through a Marie Curie Transfer-of-Knowledge (ToK) fellowship [MTKD-CT-2004-014188]
- European Commission's Seventh Framework Programme [FP7-606740, 264895]
- European Research Council (ERC) [320360, 647208]
- European Research Council (ERC) through the European Union's Horizon 2020 research and innovation programme [670519, 687378]
- European Science Foundation (ESF) of the Gaia Research for European Astronomy Training Research Network Programme (GREAT-ESF)
- European Union (EU) through a European Regional Development Fund (ERDF) for Galicia, Spain
- Academy of Finland
- Magnus Ehrnrooth Foundation
- French Centre National de la Recherche Scientifique (CNRS) through action 'Defi MASTODONS' the Centre National d'Etudes Spatiales (CNES)
- L'Agence Nationale de la Recherche (ANR) 'Investissements d'avenir' Initiatives D'EXcellence (IDEX) programme Paris Sciences et Lettres (PSL**) [ANR-10-IDEX-0001-02]
- ANR D'efi de tous les savoirs' (DS10) programme [ANR-15-CE31-0007]
- Region Aquitaine
- Universite de Bordeaux
- Utinam Institute of the Universite de Franche-Comte
- Region de Franche-Comte
- Institut des Sciences de l'Univers (INSU)
- German Aerospace Agency (Deutsches Zentrum fur Luft-und Raumfahrt e.V., DLR) [50QG0501, 50QG0601, 50QG0602, 50QG0701, 50QG0901, 50QG1001, 50QG1101, 50QG1401, 50QG1402, 50QG1403, 50QG1404]
- European Space Agency (ESA) through the Plan for European Cooperating States (PECS) programme [C98090, 4000106398/12/NL/KML, 4000115263/15/NL/IB]
- Hungarian Academy of Sciences through the Lendulet Programme [LP2014-17]
- Janos Bolyai Research Scholarship
- Hungarian National Research, Development, and Innovation Office [NKFIH K-115709, PD-116175, PD-121203]
- Science Foundation Ireland (SFI) through a Royal Society -SFI University Research Fellowship
- Israel Science Foundation (ISF) [848/16]
- Agenzia Spaziale Italiana (ASI) [I/037/08/0, I/058/10/0, 2014-025-R.0, 2014-025-R.1.2015, 2014-049-R.0/1/2, I/008/10/0, 2013/030/I.0, 2013-030-I.0.1-2015, 2016-17-I.0]
- Netherlands Organisation for Scientific Research (NWO) [NWO-M-614.061.414]
- Netherlands Organisation for Scientific Research (NWO) through a VICI grant
- Netherlands Research School for Astronomy (NOVA)
- Polish National Science Centre through HARMONIA grant [2015/18/M/ST9/00544]
- Polish National Science Centre through ETIUDA grants [2016/20/S/ST9/00162, 2016/20/T/ST9/00170]
- Portugese Fundacao para a Ciencia e a Tecnologia (FCT) [SFRH/BPD/74697/2010]
- Slovenian Research Agency [P10188]
- Spanish Ministry of Economy (MINECO/FEDER, UE) [ESP2014-55996-C2-1-R, ESP2014-55996-C2-2-R, ESP2016-80079-C2-1-R, ESP2016-80079-C2-2-R]
- Spanish Ministerio de Economia, Industria y Competitividad [AyA2014-55216]
- Spanish Ministerio de Educacion, Cultura y Deporte (MECD) [FPU16/03827]
- Institute of Cosmos Sciences University of Barcelona (ICCUB, Unidad de Excelencia 'Maria de Maeztu') [MDM-2014-0369]
- Xunta de Galicia
- Centros Singulares de Investigacion de Galicia for the period 2016-2019 through the Centro de Investigacion en Tecnologias de la Informacion y las Comunicaciones (CITIC)
- Red Espanola de Supercomputacion (RES) computer resources at MareNostrum
- Barcelona Supercomputing Centre - Centro Nacional de Supercomputacion (BSC-CNS) [AECT-2016-1-0006, AECT-2016-2-0013, AECT-2016-3-0011, AECT-2017-1-0020]
- Swedish National Space Board (SNSB/Rymdstyrelsen)
- Swiss State Secretariat for Education, Research, and Innovation through the ESA PRODEX programme
- Mesures d'Accompagnement
- Swiss Activites Nationales Complementaires
- Swiss National Science Foundation
- United Kingdom Rutherford Appleton Laboratory
- United Kingdom Science and Technology Facilities Council (STFC) [ST/L006553/1]
- United Kingdom Space Agency (UKSA) [ST/N000641/1, ST/N001117/1]
- Particle Physics and Astronomy Research Council [PP/C503703/1]
- Brazil-France exchange programme Coordenacao de Aperfeicoamento de Pessoal de Nivel Superior (CAPES) - Comite Francais d'Evaluation de la Cooperation Universitaire et Scientifique avec le Bresil (COFE-CUB)
- [UID/FIS/00099/2013]
- [UID/EEA/00066/2013]
- STFC [ST/L006553/1, ST/S002103/1] Funding Source: UKRI
- Fundação para a Ciência e a Tecnologia [UID/EEA/00066/2013] Funding Source: FCT
- Austrian Science Fund (FWF) [P20046] Funding Source: Austrian Science Fund (FWF)
White dwarfs carry information on the structure and evolution of the Galaxy, especially through their luminosity function and initial-to-final mass relation. Very cool white dwarfs provide insight into the early ages of each population. Examining the spectra of all stars with 3 sigma proper motion in the Sloan Digital Sky Survey Data Release 14, we report the classification for 20 088 spectroscopically confirmed white dwarfs, plus 415 hot subdwarfs, and 311 cataclysmic variables. We obtain T-eff, log g, and mass for hydrogen atmosphere white dwarf stars (DAs), warm helium atmosphere white dwarfs (DBs), hot subdwarfs (sdBs and sdOs), and estimate photometric T-eff for white dwarf stars with continuum spectra (DCs). We find 15 793 sdAs and 447 dCs between the white dwarf cooling sequence and the main sequence, especially below T-eff similar or equal to 10 000 K; most are likely low-mass metal-poor main-sequence stars, but some could be the result of interacting binary evolution.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据
分享论文
