PG 2254+067 , the SIMBAD biblio

PG 2254+067 , the SIMBAD biblio (20 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:57:34

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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
1986ApJS...61..305G viz 1882 923 The Palomar-Green catalog of ultraviolet-excess stellar objects. GREEN R.F., SCHMIDT M. and LIEBERT J.
1988SAAOC..12....1K viz 1210 56 A catalogue of spectroscopically identified hot subdwarf stars. KILKENNY D., HEBER U. and DRILLING J.S.
2010A&A...513A...6O viz 15       D               1 343 51 A survey for pulsating subdwarf B stars with the Nordic Optical Telescope. OSTENSEN R.H., OREIRO R., SOLHEIM J.-E., et al.
2011A&A...526A..39G 362       D     X C       9 10 30 Massive unseen companions to hot faint underluminous stars from SDSS (MUCHFUSS). Analysis of seven close subdwarf B binaries. GEIER S., MAXTED P.F.L., NAPIWOTZKI R., et al.
2011A&A...530A..28G viz 15       D               2 161 79 The MUCHFUSS project - searching for hot subdwarf binaries with massive unseen companions. Survey, target selection and atmospheric parameters. GEIER S., HIRSCH H., TILLICH A., et al.
2011MNRAS.417.1210G viz 15       D               2 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.
2015A&A...576A..44K viz 16       D               1 145 87 Hot subdwarf binaries from the MUCHFUSS project. Analysis of 12 new systems and a study of the short-period binary population. KUPFER T., GEIER S., HEBER U., et al.
2015A&A...577A..26G viz 16       D               1 200 27 The catalogue of radial velocity variable hot subluminous stars from the MUCHFUSS project. GEIER S., KUPFER T., HEBER U., et al.
2015MNRAS.450.3514K 16       D               2 218 19 New binaries among UV-selected, hot subdwarf stars and population properties. KAWKA A., VENNES S., O'TOOLE S., et al.
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.
2017ApJ...845..171B viz 16       D               1 1444 3 A search for rapidly pulsating hot subdwarf stars in the GALEX survey. BOUDREAUX T.M., BARLOW B.N., FLEMING S.W., et al.
2018ApJ...868...70L viz 16       D               1 294 25 New hot subdwarf stars identified in Gaia DR2 with LAMOST DR5 spectra. LEI Z., ZHAO J., NEMETH P., 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.
2019MNRAS.482.4570G viz 17       D               1 486647 296 A Gaia Data Release 2 catalogue of white dwarfs and a comparison with SDSS. GENTILE FUSILLO N.P., TREMBLAY P.-E., GANSICKE B.T., 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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