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Table 1
Dense stellar fields observed to model the photometric flat-field correction.
| Name | RA | Dec | E(B − V)a |
| (mag) | |||
|
|
|||
| Grid-1 (winter field) | 6h30m00 | 14d20m00 | 0.45 ± 0.08 |
| Grid-2 (summer field) | 21h00m00 | 10d00m00 | 0.12 ± 0.03 |
Notes.
(a)
Average value of the dust extinction derived from the analysis of the stellar locus displacement, assuming extinction follows Cardelli et al. (1989) law with Rv = 3.1.
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