Image Details
Caption: Figure 10.
AGN occurrence rate FAGN(L(Hβ)corr > 1039 erg s−1), 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.
© 2026. The Author(s). Published by the American Astronomical Society.