Dense stellar fields observed to model the photometric flat-field correction.
|Name||RA||Dec||E(B − V)a|
|Grid-1 (winter field)||6h30m00||14d20m00||0.45 ± 0.08|
|Grid-2 (summer field)||21h00m00||10d00m00||0.12 ± 0.03|
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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