CD-39 14181 , the SIMBAD biblio

CD-39 14181 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST04:01:28

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1992ApJS...81..795G 1543 77 An Einstein Observatory SAO-based catalog of B-type stars. GRILLO F., SCIORTINO S., MICELA G., et al.
2015MNRAS.453.1879K viz 16       D               1 715 9 The Edinburgh-Cape Blue Object Survey - IV. Zone 3: Galactic latitudes -40° > b > -50°. KILKENNY D., O'DONOGHUE D., WORTERS H.L., et al.
2018A&A...620A.172Z viz 16       D               1 127610 99 3D mapping of young stars in the solar neighbourhood with Gaia DR2. ZARI E., HASHEMI H., BROWN A.G.A., et al.
2019A&A...621A..38G viz 16       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.
2020MNRAS.499.5508S viz 99       D         F     3 1808 ~ A search for variable subdwarf B stars in TESS full frame images - I. Variable objects in the southern ecliptic hemisphere. SAHOO S.K., BARAN A.S., SANJAYAN S., et al.
2021A&A...650A.205V viz 17       D               1 1932 14 A search for transiting planets around hot subdwarfs. I. Methods and performance tests on light curves from Kepler, K2, TESS, and CHEOPS. VAN GROOTEL V., POZUELOS F.J., THUILLIER A., et al.
2022A&A...662A..40C viz 17       D               1 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.
2024A&A...686A..25D viz 18       D               1 401 ~ A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties. DAWSON H., GEIER S., HEBER U., et al.
2026A&A...707A...6D viz 50           X         1 49 ~ A 500 pc volume-limited sample of hot subluminous stars II. Atmospheric parameters, mass distribution, and kinematics. DAWSON H., DORSCH M., GEIER S., et al.

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