CPD-55 10148 , the SIMBAD biblio

CPD-55 10148 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST15:43:05

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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
2014ASPC..485..223B viz 15       D               1 465820 45 The JMMC stellar diameters catalog v2 (JSDC): a new release based on SearchCal improvements BOURGES L., LAFRASSE S., MELLA G., 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.
2019MNRAS.490.3158C viz 16       D               1 465839 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., et al.
2020MNRAS.499.5508S viz 16       D               1 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.
2022A&A...663A..45K viz 145       D     X         4 159 4 Discovery of new TESS pulsating hot subdwarfs. KRZESINSKI J. and BALONA L.A.
2024A&A...684A.118U viz 18       D               1 345 ~ A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars. UZUNDAG M., KRZESINSKI J., PELISOLI I., 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.

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