FBS 1654+352 , the SIMBAD biblio

FBS 1654+352 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST01:21:35

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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
1993Afz....36..517A viz 97 2 First Byurakan spectral sky survey. Blue stellar objects. VI. Zone +33 <delta< +37. ABRAHAMIAN H.V. and MICKAELIAN A.M.
2004A&A...426..367M viz 1102 9 DSS1/DSS2 astrometry for 1101 First Byurakan Survey blue stellar objects: Accurate positions and other results. MICKAELIAN A.M.
2008AJ....136..946M viz 15       D               1103 15 Revised and updated catalogue of the First Byurakan Survey blue stellar objects. MICKAELIAN A.M.
2008Ap.....51..226S 15       D               1 66 0 Spectral observations of FBS blue stellar objects in the zone delta = + 35 deg. SINAMYAN P.K. and MICKAELIAN A.M.
2010MNRAS.407..681M viz 15       D               1 640 15 Proper motions and natures of First Byurakan Survey blue stellar objects. MICKAELIAN A.M. and SINAMYAN P.K.
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.
2019MNRAS.490.3158C viz 17       D               1 465834 28 A catalogue of stellar diameters and fluxes for mid-infrared interferometry. CRUZALEBES P., PETROV R.G., ROBBE-DUBOIS S., 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.
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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