OGLE BLG-RRLYR-36651 , the SIMBAD biblio

OGLE BLG-RRLYR-36651 , the SIMBAD biblio (10 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST22:46:55


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Title First 3 Authors
1994PAZh...20..403K 45 ~ New variable stars in the globular cluster M 22 = NGC 6656. KRAVTSOV V.V., SAMUS N.N., ALCAINO G., 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.
2017AJ....153..204S viz 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.
2017ApJ...850...96H viz 16       D               1 13727 30 The geometry of the Sagittarius stream from Pan-STARRS1 3π RR Lyrae. HERNITSCHEK N., SESAR B., RIX H.-W., 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.
2021A&A...651A..47A viz 17       D               1 735 11 Variable stars in the VVV globular clusters. II. NGC 6441, NGC 6569, NGC 6626 (M 28), NGC 6656 (M 22), 2MASS-GC 02, and Terzan 10. ALONSO-GARCIA J., SMITH L.C., CATELAN M., et al.
2022MNRAS.510.3575H viz 17       D               1 71780 1 Identifying RR Lyrae in the ZTF DR3 data set. HUANG K.-W. and KOPOSOV S.E.
2022ApJS..261...33D viz 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.
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.

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