Upper row: membership probability as a function of magnitude for the bulge, disk and cluster, color coded by point density. The blue and red dashed lines depict the p = 0.66 and p = 0.90 levels used to select likely members of the respective components of the mixture. Middle row: VPD of the whole sample is displayed identically in each panel, color coded by density. The blue and red points stand for subsamples of bulge, disk, and cluster stars selected as those with membership probabilities to the respective component larger than p = 0.66 and p = 0.90 (and with error in their probabilities smaller than 0.35). Lower row: CMD for the most probable members of the bulge, disk and cluster, color coded as above.