Table 2.
Completeness of Datasets A, B, and C with respect to the samples of variable stars published in dedicated Gaia DR2 catalogues of variable stars.
| Variability type | Total | 5.5 < G/mag < 19, Aproxy, G > 0.06 |
Reference | ||||
|---|---|---|---|---|---|---|---|
| in DR2 | in DR2 | Dataset A | Dataset B | Dataset C | |||
| LPV (SOS) | 151 761 | 138 193 | 138 150 | 111 941 | 76 527 | Mowlavi et al. (2018) | |
| 81% | 68% | ||||||
| RR Lyr (classif) | 195 780 | 127 123 | 127 103 | 74 189 | 48 891 | Rimoldini et al. (2019) | |
| 58% | 66% | ||||||
| RR Lyr (SOS) | 140 784 | 90 024 | 89 976 | 59 824 | 39 977 | Clementini et al. (2019) | |
| 66% | 67% | ||||||
| Cep (classif) | 8550 | 8367 | 8362 | 5403 | 3887 | Rimoldini et al. (2019) | |
| 65% | 72% | ||||||
| Cep (SOS) | 9575 | 9197 | 9194 | 5685 | 4131 | Clementini et al. (2019) | |
| 62% | 73% | ||||||
| δ Sct, SX Phe (classif) | 8882 | 3328 | 3310 | 3183 | 2016 | Rimoldini et al. (2019) | |
| 96% | 63% | ||||||
| Rot. modul. (SOS) | 147 535 | 2181 | 2129 | 692 | 463 | Lanzafame et al. (2018) | |
| 33% | 67% | ||||||
| Short time-scale (SOS) | 3018 | 2641 | 2640 | 129 | 60 | Roelens et al. (2018) | |
| 5% | 47% | ||||||
Notes. The origin of the samples in DR2 (i.e. either classification table or SOS table, see Holl et al. 2018, in particular their Fig. 3) is indicated in parenthesis. Reference to the paper describing the specific catalogue is given in the last column. The numbers in italics denote the percentages of sources present in Datasets B and C compared to Datasets A and B, respectively.
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