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| V* V1862 Oph , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2024.04.27CEST19:37:41 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
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 |
|---|---|---|---|---|---|---|---|---|---|
| 1968BANS....2..293P | 919 | 5 | Variable stars in a field centred at l(II) = 4deg, b(II) = +12deg (field 2 of the Palomar-Groningen variable-star survey). Part 1: Introduction and RR Lyrae-type variables. | PLAUT L. | |||||
| 1970IBVS..480....1K | 2217 | 35 | 57th Name-list of variable stars | KUKARKIN B.V., KHOLOPOV P.N. and PEROVA N.B. | |||||
2014MNRAS.441..715G 
|
16 | D | 1 | 13079 | 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. | ||
|
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. | ||
|
2017ApJ...850...96H
|
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. | ||
|
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. | ||
|
2019AcA....69..321S
|
17 | 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 | 17 | 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. |
