Fig. 8
Double RC in the magnitude distribution of bulge stars as a function of metallicity. Upper panel: generalized histograms (Gaussian kernel of 0.09 mag) of the extinction corrected Ks magnitudes for stars with [Fe/H] ≳ + 0.1 dex. Lower panel: generalized histograms (Gaussian kernel of 0.09 mag) of the extinction corrected Ks magnitudes for stars with [Fe/H] ≲ + 0.1 dex. The same color-coding is used to identify the different fields in both panels.
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