US 3977 , the SIMBAD biblio

US 3977 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.18CEST10:03:21


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Bibcode/DOI Score in Title|Abstract|
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Title First 3 Authors
1990ApJS...74..885U 14       D               23 10 Faint blue objects at high galactic latitude. VI. Palomar Schmidt field centered on selected area 82. USHER P.D. and MITCHELL K.J.
1998MNRAS.295..225M 50 13 A new, complete sample of faint B stars in the Galactic halo. MITCHELL K.J., SAFFER R.A., HOWELL S.B., et al.
2004ApJS..153..119M viz 15       D               654 2 Faint blue objects at high galactic latitude. VIII. Performance characteristics of the US survey. MITCHELL K.J. and USHER P.D.
2007ApJ...671.1708B viz 15       D               396 76 Hypervelocity stars. III. The space density and ejection history of main-sequence stars from the Galactic Center. BROWN W.R., GELLER M.J., KENYON S.J., et al.
2019A&A...621A..38G viz 17       D               1 39805 85 The population of hot subdwarf stars studied with Gaia. II. The Gaia DR2 catalogue of hot subluminous stars. GEIER S., RADDI R., GENTILE FUSILLO N.P., et al.
2019ApJ...881....7L viz 17       D               1 926 24 Hot subdwarf stars observed in Gaia DR2 and LAMOST DR5. LUO Y., NEMETH P., DENG L., et al.
2020A&A...635A.193G viz 17       D               2 6177 44 The population of hot subdwarf stars studied with Gaia. III. Catalogue of known hot subdwarf stars: Data Release 2. GEIER S.
2021ApJS..256...28L viz 17       D               1 2206 16 Hot subdwarf atmospheric parameters, kinematics, and origins based on 1587 hot subdwarf stars observed in Gaia DR2 and LAMOST DR7. LUO Y., NEMETH P., WANG K., et al.
2022ApJS..259....5T viz 18       D               2 1465 4 A Robust Identification Method for Hot Subdwarfs Based on Deep Learning. TAN L., MEI Y., LIU Z., et al.
2022A&A...662A..40C viz 18       D               2 62976 9 The population of hot subdwarf stars studied with Gaia. IV. Catalogues of hot subluminous stars based on Gaia EDR3. CULPAN R., GEIER S., REINDL N., et al.

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