AGN occurrence rate F_AGN(λ > 10⁻³), based on model fits (i.e., corrected for selection effects), as a function of stellar mass and sSFR. The bands are ±1σ uncertainties based on the posterior distribution. For this plot we use the M–σ relation of J. Kormendy & L. C. Ho (2013) and bolometric luminosities based on dust-corrected Hβ and the conversion of H. Netzer (2019).