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Table 2.
Typical radial velocity error of observed stars in the faintest 0.5 mag bin as derived from Eq. 2 for [Fe/H] = −1 dex (MP) and [Fe/H] = +0.5 dex (MR).
| Field | S/N | ɛ RV (MP) km s−1 | ɛ RV (MR) km s−1 |
|---|---|---|---|
| p0m2 | 20 | 6.3 | 4.5 |
| m1p2 | 15 | 8.4 | 6.1 |
| p0p2 | 10 | 12.8 | 9.2 |
| p1m1 a | 10 | 7.4 | 6.8 |
Notes.
(a)
For this field the faintest stars are giants, therefore we have used Eq. (1).
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