Morphological class fraction of BASS AGNs, before (above) and after (below) redshift debiasing, as a function of redshift (left), 14–195 keV luminosity (middle left), black hole mass (middle), Eddington ratio (middle right), and absolute i-magnitude for Sy 1.8-2 types only (right). Shaded regions correspond to 1σ confidence. No attempt was made to debias the other-uncertain class. A small percentage of sources lie beyond the limits of the plots, but subsequently have poorly constrained class fractions and were thus cropped out.