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Table 1
Fields observed: coordinates, distance to Galactic centre, reddening as adopted in Zoccali et al. (2008), number of stars observed, and typical signal-to-noise ratios.
| Field | l | b | RGC | E(B-V) | Nstars | S∕N/pixel |
|---|---|---|---|---|---|---|
| (°) | (°) | (pc) | @620 nm | |||
| Baade’s window | 1. °14 | −4. °18 | 604 | 0.55 | 204 | 40–60 |
| b = − 6° | 0. °21 | −6. °02 | 850 | 0.48 | 213 | 60–90 |
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