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| OGLE BLG-RRLYR-47019 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST10:17:00 |
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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 |
|---|---|---|---|---|---|---|---|---|---|
2013MNRAS.434.1220A 
|
822 | D | X C F | 20 | 43 | 27 | A detailed census of variable stars in the globular cluster NGC 6333 (M9) from CCD differential photometry. | ARELLANO FERRO A., BRAMICH D.M., FIGUERA JAIMES R., 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. | ||
|
2022ApJS..261...33D
|
17 | D | 1 | 104673 | 3 | Photometric Metallicity Prediction of Fundamental-mode RR Lyrae Stars in the Gaia Optical and Ks Infrared Wave Bands by Deep Learning. | DEKANY I. and GREBEL E.K. | ||
|
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. | ||
|
2019AcA....69..321S
|
16 | D | 2 | 80178 | 56 | Over 78 000 RR Lyrae stars in the Galactic bulge and disk from the OGLE survey. | SOSZYNSKI I., UDALSKI A., WRONA M., et al. | ||
| 2020AcA....70..121P | 16 | D | 1 | 80166 | ~ | Properties of the Milky Way's old populations based on photometric metallicities of the OGLE RR Lyrae stars. | PIETRUKOWICZ P., UDALSKI A., SOSZYNSKI I., 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...689A.189F
|
18 | D | 1 | 1324 | ~ | Validation of the RR Lyrae period determination in the Pan-STARRS PS1 3π survey with K2. | FORRO A., MOLNAR L., PLACHY E., et al. | ||
|
2024A&A...690L..17L
|
18 | D | 1 | 11379 | ~ | An 'alien' called the Oosterhoff dichotomy? | LUONGO E., RIPEPI V., MARCONI M., et al. |
