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| PHL 1539 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:11:50 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
|
2017A&A...600A..50G |
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 |
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 |
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 |
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. | ||
|
2022ApJS..258...16P |
17 | D | 1 | 4582 | 43 | TESS Eclipsing Binary stars. I. Short-cadence observations of 4584 eclipsing binaries in sectors 1-26. | PRSA A., KOCHOSKA A., CONROY K.E., et al. | ||
|
2022A&A...662A..40C |
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 | 43 | X | 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. | ||
| 2019RNAAS...3...81B | 325 | X C | 7 | 2 | ~ | A Hot Subdwarf B Star Eclipsed by a Low-mass White Dwarf in TESS Data. | BELL K.J., KOSAKOWSKI A., KILIC M., et al. | ||
|
2024A&A...691A.223V |
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. |