Table 1
Relative source counts for sources with ≥2 G-band FoV transits, illustrating the decrease in relative completeness for source sets with ≥12 and ≥20 G-band FoV transits, as applied in our processing.
| Direction | ≥ 2 FoV | ≥12 FoV | ≥20 FoV | |||
|---|---|---|---|---|---|---|
| ALL | 100% | (1607) | 80% | (1283) | 51% | (826) |
| Galactic plane | 100% | (778) | 85% | (665) | 68% | (532) |
| Galactic centre | 100% | (351) | 67% | (236) | 14% | (50.0) |
| High Galactic latitudes | 100% | (50.4) | 76% | (38.4) | 48% | (24.4) |
| LMC region | 100% | (23.5) | 76% | (17.9) | 59% | (13.9) |
| SMC region | 100% | (3.4) | 78% | (2.6) | 66% | (2.2) |
| Catalina DR2 | 100% | (400) | 80% | (320) | 53% | (210) |
| Catalina DR1 | 100% | (200) | 80% | (160) | 50% | (100) |
| OGLE-IV Bulge | 100% | (305) | 66% | (200) | 10% | (29) |
| OGLE-IV MCs | 100% | (33) | 77% | (25) | 62% | (20) |
| Kepler | 100% | (8.4) | 87% | (7.4) | 78% | (6.6) |
| Rebull et al. (2016) (K2 Pleiades) | 100% | (0.38) | 85% | (0.32) | 66% | (0.25) |
| Hartman et al. (2010) (Pleiades) | 100% | (0.87) | 84% | (0.73) | 51% | (0.44) |
Notes. The top part specifies the numbers for some generic directions in the Galaxy, as defined in Sect. 2.1 and illustrated in Fig. 1. The bottom part specifies the numbers for several external catalogues, listing the Gaia source counts in their approximate sky footprints (not their source cross-match counts). In parenthesis, we provide the actual Gaia source counts in millions. Estimates of the absolute completeness of the published variable samples are presented in Tables 2 and 3.
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