Fig. 8.
Observed mean Ks (left panel) and reddening-corrected Ks0 (right) magnitude of stars with ∼50% completeness level (p = 0.50 ± 0.03) across the whole bulge area studied in this work. Each measurement comes from the average magnitude per individual detector per tile, where the position in the sky is set to be the middle of each detector field of view.
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