Black hole mass distributions for galaxies with bulge masses 10 < log M_bulge < 10.5 (left panel) and 10.5 < log M_bulge < 11 (right panel) predicted by the Guo et al. (2011) and Bower et al. (2006) models (red and blue lines, respectively), and for classical and pseudo bulges (dotted and solid lines, respectively). The solid, black lines in both panels are the data collected in Table 1. The grey stripes are the black hole mass intervals (median plus scatter) inferred from the Sani et al. M_bh-M_bulge relation for the corresponding bulge masses.