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GUVV J120136.9-033328.1 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.19CEST23:27:17 |
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 |
---|---|---|---|---|---|---|---|---|---|
2008AJ....136..259W | 15 | D | 1 | 413 | 15 | The second GALEX ultraviolet variability (GUVV-2) catalog. | WHEATLEY J.M., WELSH B.Y. and BROWNE S.E. | ||
2013ApJ...763...32D | 16 | D | 1 | 12288 | 202 | Probing the outer galactic halo with RR Lyrae from the Catalina surveys. | DRAKE A.J., CATELAN M., DJORGOVSKI S.G., et al. | ||
2013AJ....146...21S | 16 | D | 1 | 5702 | 98 | Exploring the variable sky with LINEAR. II. Halo structure and substructure traced by RR Lyrae stars to 30 kpc. | SESAR B., IVEZIC Z., STUART J.S., et al. | ||
2014ApJ...781...22Z | 16 | D | 1 | 1393 | 41 | La Silla QUEST RR Lyrae star survey: region I. | ZINN R., HOROWITZ B., VIVAS A.K., et al. | ||
2014A&A...566A.118D | 16 | D | 9 | 116 | 25 | A comprehensive view of the Virgo stellar stream. | DUFFAU S., VIVAS A.K., ZINN R., et al. | ||
2014AJ....148..121K | 16 | D | 1 | 255 | 3 | The identification of RR Lyrae and δ Scutti stars from variable Galaxy Evolution Explorer ultraviolet sources. | KINMAN T.D. and BROWN W.R. | ||
2016ApJ...831..165V | 16 | D | 1 | 469 | 11 | Disentangling the Virgo overdensity with RR Lyrae stars. | VIVAS A.K., ZINN R., FARMER J., 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. | ||
2019A&A...622A..60C | 17 | 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. | ||
2022ApJS..261...33D | 18 | 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. |