FBS 1715+424 , the SIMBAD biblio

FBS 1715+424 , the SIMBAD biblio (21 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.16CEST18:19:56

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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
1991Afz....34...13A viz 105 4 First Byurakan spectral sky survey. Blue stellar objects. IV. The region +41<delta<45. ABRAMYAN G.V., LIPOVETSKII V.A., MIKAELYAN A.M., et al.
1993Afz....36..203E 33 6 Polarimetric observations of blue FBS stellar objects. II. ERITSYAN M.A. and MIKAELYAN A.M.
1999Ap.....42....1M viz 112 13 On the nature of the FBS blue stellar objects and the completeness of the bright quasar survey. MICKAELIAN A.M., GONCALVES A.C., VERON-CETTY M.-P., et al.
2003A&A...406..535Z viz 10257 80 The Hamburg/RASS Catalogue of optical identifications. Northern high-galactic latitude ROSAT Bright Source Catalogue X-ray sources. ZICKGRAF F.-J., ENGELS D., HAGEN H.-J., et al.
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.
2006Ap.....49..333S 101 1 Spectral observations of blue stellar objects from FBS in the zone delta = +43 ° . SINAMIAN P.K. and 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.
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.
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 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.
2019ApJ...881....7L viz 16       D               1 926 24 Hot subdwarf stars observed in Gaia DR2 and LAMOST DR5. LUO Y., NEMETH P., DENG L., et al.
2019PASJ...71...41L 16       D               1 77 ~ Searching for hot subdwarf stars from the LAMOST Spectra. II. Pure spectroscopic identification method for hot subdwarfs. LEI Z., BU Y., ZHAO J., 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               1 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               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 17       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...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.
2023ApJS..264...17Z viz 17       D               3 31380 1 Stellar Parameters and Spectroscopic Properties of TESS Objects Observed in the LAMOST Low- and Medium-resolution Spectral Survey. ZHANG L.-Y., SU T., MISRA P., et al.
2024A&A...686A..25D viz 18       D               1 401 ~ A 500 pc volume-limited sample of hot subluminous stars I. Space density, scale height, and population properties. DAWSON H., GEIER S., HEBER U., 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.
2025AJ....169..275G 112       D         F     5 81 ~ The Lyα Sky as Observed by New Horizons at 57 au. GLADSTONE G.R., SHULL J.M., PRYOR W.R., et al.

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