Left: cumulative log N–log S distribution of the MOJAVE-1 sample excluding radio galaxies, omitting all upper limits (flux for 20–100 keV, blue squares) and log N–log S for the beamed AGN sub-sample of the BAT 105-month source catalog (flux for 14 keV–195 keV, red circles) and the same sub-sample excluding all MOJAVE-1 sources (14 keV–195 keV, purple x). Right: log N–log S for 15 GHz flux density VLBI measurements from Lister et al. (2015) of all blazars in the MOJAVE-1 sample (black circles) and MOJAVE-1 blazars from left graph (blue squares, norm with a factor of 0.1 for better readability). The black lines represent power-law fits, the gray area shows the corresponding error range. The radio data have been fit for all fluxes higher than 2.5 Jy. The dashed lines indicate a slope of −1.5.