Table 1
Characteristics of the three Rubin DP1 fields and the selection process.
| Field | Coordinates | The number of exposures per band | Selected sample sizes | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| RA | Dec | l | b | u | g | r | i | z | y | Total | r < 24 | Unresolved | Blue MS | |
| ECDFS | 53.13 | −28.10 | 224.07 | −54.47 | 43 | 230 | 237 | 162 | 153 | 30 | 494 851 | 81 622 | 6874 | 786 |
| EDFS | 59.10 | −48.73 | 256.98 | −48.48 | 20 | 61 | 87 | 42 | 42 | 20 | 375 663 | 83 868 | 8454 | 1010 |
| SV 95–25 | 95.00 | −25.00 | 232.53 | −17.64 | 33 | 82 | 84 | 23 | 60 | 10 | 348 913 | 128 130 | 30 393 | 5767 |
Notes. Table summarizes basics characteristics of the DP1 fields analyzed in this work, as well as counts of objects after successive selection steps. Equatorial and galactic coordinates are listed in degrees. The ugrizy columns list the number of exposures in each band. The last four columns list the number of objects after successive selection steps. Each field covers about 2 deg2.
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