OGLE BLG-RRLYR-30509 , the SIMBAD biblio

OGLE BLG-RRLYR-30509 , the SIMBAD biblio (9 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST11:29:39

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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
2001AJ....122.2600P 85 54 Variable stars in the unusual, metal-rich, globular cluster NGC 6441. PRITZL B.J., SMITH H.A., CATELAN M., et al.
2015A&A...573A.103S viz 211       D     X C       5 202 11 Searching for variable stars in the cores of five metal-rich globular clusters using EMCCD observations. SKOTTFELT J., BRAMICH D.M., FIGUERA JAIMES R., et al.
2014AcA....64..177S viz 15       D               1 38315 193 Over 38 000 RR Lyrae stars in the OGLE Galactic Bulge Fields. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2017AcA....67..297S viz 16       D               1 40131 79 The OGLE Collection of Variable Stars. Classical, Type II, and Anomalous Cepheids toward the Galactic Center. SOSZYNSKI I., UDALSKI A., SZYMANSKI M.K., et al.
2022A&A...657A.123O viz 17       D               1 247 4 Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters. OLIVEIRA R.A.P., ORTOLANI S., BARBUY B., et al.
2023ApJ...944...88L viz 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 viz 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 viz 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.

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