Large-scale bias evolution as a function of host galaxy stellar mass (left panel) and specific BHAR (right panel) for CCL Type 2 AGN and mock AGN. These are matched to have the same host galaxy properties of CCL Type 2 AGN, for Q = 1 and = 2 (according to the legend), which correspond to a relative fraction of satellite AGN = 0.1 and = 0.15, respectively. The error bars on x-axis represent the typical error on the stellar mass and specific BHAR estimates in COSMOS. For comparison, the red dotted lines show the large-scale bias as a function of M_star and λ_BHAR for mock matched normal galaxies.