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).

(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).

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