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| LAMOST J060806.00+461001.4 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST19:47:04 |
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More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
2019A&A...621A..38G 
|
17 | 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
|
17 | D | 1 | 486647 | 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. | ||
|
2020ApJ...889..117L
|
17 | D | 1 | 183 | 16 | Hot subdwarf stars identified in Gaia DR2 with spectra of LAMOST DR6 and DR7. I. Single-lined spectra. | LEI Z., ZHAO J., NEMETH P., et al. | ||
|
2020A&A...635A.193G
|
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. | ||
|
2020ApJ...898...64L
|
17 | D | 1 | 183 | ~ | Hot subdwarf stars identified in Gaia DR2 with spectra of LAMOST DR6 and DR7. II. Kinematics. | LUO Y., NEMETH P. and LI Q. | ||
|
2021ApJS..256...28L
|
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
|
18 | D | 2 | 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
|
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. | ||
| 2024ApJS..271...21L | 20 | D | 1 | 204 | ~ | He-rich Hot Subdwarf Stars Observed in Gaia DR3 and LAMOST DR7: Carbon and Nitrogen Abundances and Kinematics. | LUO Y., NEMETH P., WANG K., et al. |
