The Low-Mass End of the 𝑀_BH/𝑀_host Relation in Quasars

Figure 1

Comparison among the 𝑀_BH distributions in the SDSS quasars at 𝑧<0.5 [27] (a), in our 2010 study (b) and in the present work (c). The latter is clearly more representative of the general quasar population at low redshift.

(a)

(b)

(c)