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| BPS CS 22944-0002 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST20:47:26 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
1991ApJS...76.1001P 
|
1762 | 52 | Photoelectric UBV photometry of stars selected in the HK objective-prism survey. | PRESTON G.W., SHECTMAN S.A. and BEERS T.C. | |||||
|
1992AJ....103.1987B
|
1024 | 532 | A search for stars of very low metal abundance. II. | BEERS T.C., PRESTON G.W. and SHECTMAN S.A. | |||||
|
1995ApJS...96..175B
|
1810 | 175 | Kinematics of metal-poor stars in the Galaxy. | BEERS T.C. and SOMMER-LARSEN J. | |||||
|
2000AJ....119.2866B
|
2011 | 171 | Kinematics of metal-poor stars in the Galaxy. II. Proper motions for a large nonkinematically selected sample. | BEERS T.C., CHIBA M., YOSHII Y., et al. | |||||
|
2017AJ....153..204S
|
16 | D | 1 | 46977 | 123 | Machine-learned identification of RR Lyrae stars from sparse, multi-band data: the PS1 sample. | SESAR B., HERNITSCHEK N., MITROVIC S., et al. | ||
|
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. | ||
|
2022MNRAS.510.3575H
|
17 | D | 1 | 71780 | 1 | Identifying RR Lyrae in the ZTF DR3 data set. | HUANG K.-W. and KOPOSOV S.E. | ||
|
2023ApJ...944...88L
|
17 | D | 1 | 135907 | 6 | Photometric Metallicity and Distance Estimates for ∼136,000 RR Lyrae Stars from Gaia Data Release 3. | LI X.-Y., HUANG Y., LIU G.-C., et al. | ||
|
2023A&A...674A..18C
|
17 | D | 1 | 271810 | 30 | Gaia Data Release 3 Specific processing and validation of all-sky RR Lyrae and Cepheid stars: The RR Lyrae sample. | CLEMENTINI G., RIPEPI V., GAROFALO A., et al. | ||
|
2024A&A...690L..17L
|
18 | D | 1 | 11379 | ~ | An 'alien' called the Oosterhoff dichotomy? | LUONGO E., RIPEPI V., MARCONI M., et al. |
