期刊
ASTRONOMY & ASTROPHYSICS
卷 635, 期 -, 页码 -出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361/202037526
关键词
subdwarfs; stars: horizontal-branch; catalogs
资金
- Heisenberg program of the Deutsche Forschungsgemeinschaft (DFG) [GE 2506/8-1, GE 2506/9-1]
- NASA [NAS5-26555, NAS5-98034]
- NASA O ffice of Space Science [NNX13AC07G]
- National Aeronautics and Space Administration [NAS5-26555, NNX08AR22G]
- National Science Foundation
- Robert Martin Ayers Sciences Fund
- Italian Council for Research in Astronomy
- European Southern Observatory
- International GEMINI project
- European Space Agency Astrophysics Division
- ESO Program [179.A2010]
- ESO Paranal Observatory [179.A2004]
- ESO Telescopes at the La Silla Paranal Observatory [177.A 3011(A), 177.A 3011(B), 177.A 3011(C), 177.A 3011(D), 177.A 3011(E), 177.A 3011(F), 177.A-3016, 177.A-3017, 177.A-3018]
- NOVA
- NWO-M grants
- Department of Physics & Astronomy of the University of Padova
- Department of Physics of Univ. Federico II (Naples)
- National Science Foundation [AST-1238877]
- Max Planck Institute for Extraterrestrial Physics
- ARC LIEF grant from the Australian Research Council [LE130100104]
- Astronomy Australia Limited (AAL)
- Australian Government through the Commonwealth's Education Investment Fund (EIF)
- National Collaborative Research Infrastructure Strategy (NCRIS)
- National eResearch Collaboration Tools and Resources (NeCTAR)
- Australian National Data Service Projects (ANDS)
- National Development and Reform Commission
- Alfred P. Sloan Foundation
- US Department of Energy
- National Aeronautics and Space Administration
- Japanese Monbukagakusho
- Max Planck Society
- Higher Education Funding Council for England
- American Museum of Natural History
- Astrophysical Institute Potsdam
- University of Basel
- University of Cambridge
- Case Western Reserve University
- University of Chicago
- Drexel University
- Fermilab
- Institute for Advanced Study
- Japan Participation Group
- Johns Hopkins University
- Joint Institute for Nuclear Astrophysics
- Kavli Institute for Particle Astrophysics and Cosmology
- Korean Scientist Group
- Chinese Academy of Sciences (LAMOST)
- Los Alamos National Laboratory
- Max-PlanckInstitute for Astronomy (MPIA)
- Max-Planck-Institute for Astrophysics (MPA)
- New Mexico State University
- Ohio State University
- University of Pittsburgh
- University of Portsmouth
- Princeton University
- United States Naval Observatory
- University of Washington
- US Department of Energy Office of Science
- University of Arizona
- Brazilian Participation Group
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- French Participation Group
- German Participation Group
- Harvard University
- Instituto de Astrofisica de Canarias
- Michigan State/Notre Dame/JINA Participation Group
- Lawrence Berkeley National Laboratory
- Max Planck Institute for Astrophysics
- New York University
- Pennsylvania State University
- Spanish Participation Group
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- Yale University
- Space Telescope European Coordinating Facility
- Max Planck Institute for Astronomy, Heidelberg
- Max Planck Institute for Extraterrestrial Physics, Garching
- Durham University
- University of Edinburgh
- Queen's University Belfast
- Harvard-Smithsonian Center for Astrophysics
- Las Cumbres Observatory Global Telescope Network Incorporated
- National Central University of Taiwan
- Space Telescope Science Institute
- University of Maryland
- Eotvos Lorand University (ELTE)
- Gordon and Betty Moore Foundation
In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of new all-sky data from ground-based photometric surveys and the Gaia mission Data Release 2, we compiled an updated catalogue of the known hot subdwarf stars. The catalogue contains 5874 unique sources including 528 previously unknown hot subdwarfs and provides multi-band photometry, astrometry from Gaia, and classifications based on spectroscopy and colours. This new catalogue provides atmospheric parameters of 2187 stars and radial velocities of 2790 stars from the literature. Using colour, absolute magnitude, and reduced proper motion criteria, we identified 268 previously misclassified objects, most of which are less luminous white dwarfs or more luminous blue horizontal branch and main-sequence stars.
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
