Fig. 3.
(a) Scatterplot of MBH and Mgas for our sample of PG (squares), IR (circles), and HE (triangles) quasars. Colors indicate the Eddington ratio: λEdd > 1 (red), 1 ≥ λEdd > 0.1 (green), and 0.1 ≥ λEdd (blue). The dashed diagonal lines indicate that Mgas is 1, 10, 100, and 1000 times MBH. One can estimate Mgas/Mbulge from these lines by assuming the local co-evolutionary relationship such as MBH ≃ 0.005 × Mbulge (Kormendy & Ho 2013). The black cross shows the typical uncertainty (0.3 dex for both MBH and Mgas). (b) As (a), but for the subsample (see subsection 3.1 for details).