Fig. 1.
Distribution of photometric errors as a function of magnitude (black dots) in the Ks band of detector #12 for the bulge field b249. With the exception of the magnitude range 15 ≳ Ks ≳ 11, the photometric errors are well below the dispersion calculated from simulations (red line). Also worth noticing is the effect from saturation for stars with Ks ≲ 12.
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