PG 0907+123 , the SIMBAD biblio

PG 0907+123 , the SIMBAD biblio (34 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.20CEST01:28:36

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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.
1990A&A...239..265M 37 77 Hot sublumous stars at high galactic latitudes. II. Physical parameters and distances of 37 sdB stars. MOEHLER S., HEBER U. and DE BOER K.S.
1990A&AS...86...53M 127 101 Hot subluminous stars at high galactic latitudes. I. Spectra and Stromgren photometry. MOEHLER S., RICHTLER T., DE BOER K.S., et al.
1992AJ....104..203W 318 79 Studies of hot B subdwarfs. VIII. Stromgren photometry of hot, hydrogen-rich subdwarf candidates in the Palomar-Green and Kitt Peak-Downes surveys. WESEMAEL F., FONTAINE G., BERGERON P., et al.
1997A&A...327..577D 41 28 Hot subdwarf stars: galactic orbits and distribution perpendicular to the plane. DE BOER K.S., AGUILAR SANCHEZ Y., ALTMANN M., et al.
1998MNRAS.298..179J 46 32 The detection of binary companions to subdwarf B stars. JEFFERY C.S. and POLLACCO D.L.
2001MNRAS.326.1391M 2 54 348 The binary fraction of extreme horizontal branch stars. MAXTED P.F.L., HEBER U., MARSH T.R., et al.
2002ApJ...578..515B 73 24 A survey for pulsating hot B subdwarfs in the northern hemisphere. BILLERES M., FONTAINE G., BRASSARD P., et al.
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.
2003MNRAS.338..752M 2 22 151 Orbital periods of 22 subdwarf B stars. MORALES-RUEDA L., MAXTED P.F.L., MARSH T.R., et al.
2004A&A...414..181A 112 34 Studying the populations of our Galaxy using the kinematics of sdB stars. ALTMANN M., EDELMANN H. and DE BOER K.S.
2005MNRAS.356..753N 94 198 Reconstructing the evolution of white dwarf binaries: further evidence for an alternative algorithm for the outcome of the common-envelope phase in close binaries. NELEMANS G. and TOUT C.A.
2005MNRAS.359..648M 106 35 Six detached white-dwarf close binaries. MORALES-RUEDA L., MARSH T.R., MAXTED P.F.L., et al.
2010MNRAS.406.2701K 854 T K   D S   X C       20 15 3
PG 0907+123 and JL 194: slowly pulsating hot subdwarf stars. 		KOEN C. and GREEN E.M.
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.415.3042K 15       D               2 18 1 Two large amplitude slowly pulsating hot subdwarf stars. KOEN C.
2013A&A...551A..31D viz 16       D               3 182 26 An MK-like system of spectral classification for hot subdwarfs. DRILLING J.S., JEFFERY C.S., HEBER U., et al.
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.
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.
2015MNRAS.452..765G viz 16       D               1 1185 8 An independent test of the photometric selection of white dwarf candidates using LAMOST DR3. GENTILE FUSILLO N.P., REBASSA-MANSERGAS A., GANSICKE B.T., et al.
2016ApJ...818..202L viz 16       D               1 166 12 Hot subdwarf stars observed in LAMOST DR1–Atmospheric parameters from single-lined spectra. LUO Y.-P., NEMETH P., LIU C., 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.
2017MNRAS.466.5020H 16       D               2 113 5 Three new pulsating sdB stars discovered with SuperWASP. HOLDSWORTH D.L., OSTENSEN R.H., SMALLEY B., 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.
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.
2021A&A...650A.205V viz 17       D               2 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.
2021ApJS..256...28L viz 17       D               2 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               4 1465 4 A Robust Identification Method for Hot Subdwarfs Based on Deep Learning. TAN L., MEI Y., LIU Z., et al.
2022A&A...661A.113G viz 18       D               1 652 11 Radial velocity variability and the evolution of hot subdwarf stars. GEIER S., DORSCH M., PELISOLI I., et al.
2022A&A...662A..40C viz 18       D               3 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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