V* SS Pav , the SIMBAD biblio

V* SS Pav , the SIMBAD biblio (12 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.15CEST12:47:50


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Title First 3 Authors
1970BamVe...8...90S 43 0 Mitteilungen uber veranderliche der Bamberger liste. SHAW S. and SIEVERS J.
1994IBVS.4006....1L 94 3 Improved positions of southern NSV stars. III. LOPEZ C.E. and MIRA H.
2009OEJV..101....1M 2 0 Recovery of W Dor & SS Pav. MOREL M.
2009OEJV..116....1P 180 8 A list of minima and maxima timings PASCHKE A.
2014MNRAS.441..715G viz 15       D               1 13086 14 A mid-infrared study of RR Lyrae stars with the Wide-field Infrared Survey Explorer all-sky data release. GAVRILCHENKO T., KLEIN C.R., BLOOM J.S., et al.
2015MNRAS.446.2251T viz 16       D               1 10532 100 Discovery of ∼9,000 new RR Lyrae in the southern Catalina surveys. TORREALBA G., CATELAN M., DRAKE A.J., et al.
2019A&A...622A..60C viz 16       D               1 150347 194 Gaia Data Release 2. Specific characterisation and validation of all-sky Cepheids and RR Lyrae stars. CLEMENTINI G., RIPEPI V., MOLINARO R., et al.
2021MNRAS.502.4074M viz 17       D               1 858 ~ Kinematics and multiband period-luminosity-metallicity relation of RR Lyrae stars via statistical parallax. MUHIE T.D., DAMBIS A.K., BERDNIKOV L.N., et al.
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.
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.
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.
2024A&A...690L..17L viz 18       D               1 11379 ~ An 'alien' called the Oosterhoff dichotomy? LUONGO E., RIPEPI V., MARCONI M., et al.

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