The population of hot subdwarf stars studied with Gaia IV. Catalogues of hot subluminous stars based on Gaia EDR3
In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the Gaia mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars cont...
Saved in:
Published in | Astronomy and astrophysics (Berlin) Vol. 662; p. A40 |
---|---|
Main Authors | , , , , , |
Format | Journal Article |
Language | English |
Published |
United States
EDP Sciences
14.06.2022
|
Subjects | |
Online Access | Get full text |
Cover
Loading…
Summary: | In light of substantial new discoveries of hot subdwarfs by ongoing spectroscopic surveys and the availability of the
Gaia
mission Early Data Release 3 (EDR3), we compiled new releases of two catalogues of hot subluminous stars: The data release 3 (DR3) catalogue of the known hot subdwarf stars contains 6616 unique sources and provides multi-band photometry, and astrometry from
Gaia
EDR3 as well as classifications based on spectroscopy and colours. This is an increase of 742 objects over the DR2 catalogue. This new catalogue provides atmospheric parameters for 3087 stars and radial velocities for 2791 stars from the literature. In addition, we have updated the
Gaia
Data Release 2 (DR2) catalogue of hot subluminous stars using the improved accuracy of the
Gaia
EDR3 data set together with updated quality and selection criteria to produce the
Gaia
EDR3 catalogue of 61 585 hot subluminous stars, representing an increase of 21 785 objects. The improvements in
Gaia
EDR3 astrometry and photometry compared to
Gaia
DR2 have enabled us to define more sophisticated selection functions. In particular, we improved hot subluminous star detection in the crowded regions of the Galactic plane as well as in the direction of the Magellanic Clouds by including sources with close apparent neighbours but with flux levels that dominate the neighbourhood. |
---|---|
Bibliography: | Science and Technology Facilities Council (STFC) National Aeronautics and Space Administration (NASA) USDOE Office of Science (SC) National Science Foundation (NSF) Australian Research Council (ARC) ST/T000406/1; NNX13AC07G; NAS5-26555; NAS5-98034; NNX08AR22G; AST-1238877; LE130100104 |
ISSN: | 0004-6361 1432-0746 |
DOI: | 10.1051/0004-6361/202243337 |