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| ATO J100.4017+33.7742 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.18CEST10:07:59 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2018AJ....156..241H 
|
16 | D | 1 | 311106 | 199 | A first catalog of variable stars measured by the Asteroid Terrestrial-impact Last Alert System (ATLAS). | HEINZE A.N., TONRY J.L., DENNEAU L., 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. | ||
|
2019ApJ...881....7L
|
16 | D | 1 | 926 | 24 | Hot subdwarf stars observed in Gaia DR2 and LAMOST DR5. | LUO Y., NEMETH P., DENG L., 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. | ||
|
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
|
17 | D | 2 | 1465 | 4 | A Robust Identification Method for Hot Subdwarfs Based on Deep Learning. | TAN L., MEI Y., LIU Z., et al. | ||
|
2022ApJ...928...20B
|
17 | D | 1 | 1219 | 10 | New Variable Hot Subdwarf Stars Identified from Anomalous Gaia Flux Errors, Observed by TESS, and Classified via Fourier Diagnostics. | BARLOW B.N., CORCORAN K.A., PARKER I.M., et al. | ||
|
2022A&A...661A.113G
|
17 | D | 1 | 652 | 11 | Radial velocity variability and the evolution of hot subdwarf stars. | GEIER S., DORSCH M., PELISOLI I., 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. |
