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| Cl* NGC 7092 PLAT 6931 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST12:40:23 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
1994BICDS..44....9P |
7931 | 7 | Catalogue of proper motions, UBV-photometry and spectral classification in the region of NGC 7092 (M39) | PLATAIS I. | |||||
|
2011MNRAS.417.1210G |
15 | D | 1 | 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. | ||
|
2019A&A...621A..38G |
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. | ||
|
2019MNRAS.482.4570G |
16 | D | 1 | 486646 | 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. | ||
|
2021A&A...650A.205V |
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. | ||
|
2022A&A...662A..40C |
17 | D | 1 | 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...663A..45K |
17 | D | 3 | 159 | 4 | Discovery of new TESS pulsating hot subdwarfs. | KRZESINSKI J. and BALONA L.A. | ||
|
2024A&A...684A.118U |
18 | D | 1 | 345 | ~ | A comprehensive search for hot subdwarf stars using Gaia and TESS I. Pulsating hot subdwarf B stars. | UZUNDAG M., KRZESINSKI J., PELISOLI I., et al. | ||
|
2024A&A...686A..25D |
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. |