Ton S 185 , the SIMBAD biblio

Ton S 185 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST15:23:02


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Title First 3 Authors
1962BOTT....3...37H viz 233 109 Faint blue stars in the region near the South Galactic Pole. HARO G. and LUYTEN W.J.
1968ApJ...153..723E 226 17 Stellar-population samples at the galactic poles. I. Proper-motion stars, blue objects, and eclipsing binaries near the south pole. EGGEN O.J.
1981RMxAA...6...23T 8 2 Objetos con exceso ultravioleta en la vecindad del polo galactico sur. TORRES C. and CAMPUSANO L.E.
1983AJ.....88.1304C 373 16 The Cerro el Roble sample of faint ultraviolet excess objects in the South Galactic Pole. CAMPUSANO L.E. and TORRES C.
1986MNRAS.223..629M viz 14       D               1 6120 20 A survey of trigonometric parallaxes and proper motions with the UK Schmidt telescope - II. Astrometric and photometric data for a complete sample of 6125 stars brighter than B=17.5, V=17.0 in the South Galactic Cap. MURRAY C.A., ARGYLE R.W. and CORBEN P.M.
1988ApJS...68..463L 305 30 Young, high-velocity A stars. I. Rotational velocities and a catalog of early-type stars at the South Galactic Pole. LANCE C.M.
1992AJ....103..267B viz 14       D               1 754 66 Spectroscopy of hot stars in the galactic halo. BEERS T.C., PRESTON G.W., SHECTMAN S.A., et al.
1995A&AS..112..347C viz 567 40 The ESO key-programme "A homogeneous bright QSO survey". I. The methods and the "deep" fields. CRISTIANI S., LA FRANCA F., ANDREANI P., et al.
2000AJ....119..241L viz 190 29 The Montreal-Cambridge-Tololo survey of southern subluminous blue stars: the south Galactic cap. LAMONTAGNE R., DEMERS S., WESEMAEL F., et al.
2005A&A...430..223L viz         O           78 137 Hot subdwarfs from the ESO Supernova Ia Progenitor Survey. I. Atmospheric parameters and cool companions of sdB stars. LISKER T., HEBER U., NAPIWOTZKI R., et al.
2011MNRAS.415.1105S viz 15       D               1 393 10 Distance limits to intermediate- and high-velocity clouds. SMOKER J.V., FOX A.J. and KEENAN F.P.
2012A&A...543A.149G 15       D               1 114 34 Hot subdwarf stars in close-up view. II. Rotational properties of single and wide binary subdwarf B stars. GEIER S. and HEBER U.
2013A&A...549A.110G viz 207       D     X C       5 112 46 Hot subdwarf stars in close-up view. III. Metal abundances of subdwarf B stars. GEIER S.
2016MNRAS.459.4343K viz 16       D               389 6 The Edinburgh-Cape Blue Object Survey - V. The end: Partial Zones 4-6: Galactic latitudes -50deg > b > -90deg. KILKENNY D., WORTERS H.L., O'DONOGHUE D., 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.
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.
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.
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.
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.
2022A&A...664A.113T 17       D               1 368 ~ A search for transiting planets around hot subdwarfs. II. Supplementary methods and results from TESS Cycle 1. THUILLIER A., VAN GROOTEL V., DEVORA-PAJARES M., et al.
2024A&A...691A.223V viz 18       D               1 2819 ~ Advanced classification of hot subdwarf binaries using artificial intelligence techniques and Gaia DR3 data. VISCASILLAS VAZQUEZ C., SOLANO E., ULLA A., et al.

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