Extended Data Fig. 2: The relation between MBH and M* for zâ¤0.35 type 1 AGNs without smoothing.
From: Evolutionary paths of active galactic nuclei and their host galaxies
Colours represent (a) rest-frame optical colour \({({g}^{{\prime} }-{r}^{{\prime} })}_{0}\), (b) Eddington ratio (λE), and (c) relative Fe II strength. Best-fit relations from ref. 5 for local early-type galaxies (black dashed line), late-type galaxies (black dotted line), and both types combined (black solid line; intrinsic scatter of 0.81 dex indicated as shaded gray region). This figure shows the version of Fig. 2 without smoothing to demonstrate that the trends are still present in the original data.
