M_• − σ_e relation for local type 1 AGNs, as in Figure 8, highlighting the best-fit relations for classical bulges (Kormendy & Ho 2013) and pseudo bulges (Ho & Kim 2014). We differentiate the systems by bulge type. The shaded regions represent the intrinsic scatter for both relations, 0.29 dex and 0.46 dex, respectively. The dashed line indicates the extrapolation of the best-fit relation for pseudo bulges at high BH masses. We also show the RM AGNs presented in Ho & Kim (2014, 2015) and the local AGN sample of Bennert et al. (2021).