PG 2230+121 , the SIMBAD biblio

PG 2230+121 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.17CEST07:58:58


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Title First 3 Authors
1986ApJS...61..305G viz 1882 923 The Palomar-Green catalog of ultraviolet-excess stellar objects. GREEN R.F., SCHMIDT M. and LIEBERT J.
2003AJ....126.1455S viz 15       D               1 593 46 Single and composite hot subdwarf stars in the light of 2MASS photometry. STARK M.A. and WADE R.A.
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.
2011MNRAS.417.1210G viz 15       D               1 16849 120 DA white dwarfs in Sloan Digital Sky Survey Data Release 7 and a search for infrared excess emission. GIRVEN J., GANSICKE B.T., STEEGHS D., et al.
2015MNRAS.448.2260G viz 16       D               1 32939 53 A photometric selection of white dwarf candidates in Sloan Digital Sky Survey Data Release 10. GENTILE FUSILLO N.P., GANSICKE B.T. and GREISS S.
2017A&A...600A..50G viz 16       D               5613 59 The population of hot subdwarf stars studied with Gaia. I. The catalog of known hot subdwarf stars. GEIER S., OSTENSEN R.H., NEMETH P., 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.491.2280S viz 16       D               1 48782 ~ Application of convolutional neural networks for stellar spectral classification. SHARMA K., KEMBHAVI A., KEMBHAVI A., et al.
2020A&A...635A.193G viz 16       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.
2022A&A...662A..40C viz 17       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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