Cumulative histograms and the Kolmogorov-Smirnow tests between the microlensed dwarf sample and the giant star samples shown in Fig. 12. The solid thicker red line shows the microlensed bulge dwarfs, (b) the RGB sample from Hill et al. (2011), (c) the red clump sample from Hill et al. (2011), (d) the red clump sample from ARGOS (Ness et al., submitted), and (e) the RGB sample from Uttenthaler et al. (2012).