Bolometric luminosity estimated from SED-fitting ($L_{\mathrm{bol}}^{\mathrm{SED}}$) vs. bolometric luminosity derived from the broad Hα luminosity following (Stern & Laor 2012) ($L_{\mathrm{bol}}^{\mathrm{H}\alpha }$). Left panel: $L_{\mathrm{bol}}^{\mathrm{H}\alpha }$ when using the observed L_Hα (green squares) and the extinction corrected one (yellow squares) for SEAMBHs. Central panel: the BASS AGN (blue crosses). Right panel: NLS1s galaxies from Jin et al. (2012b) (cyan diamonds). The dashed black line indicates the one-to-one relation in each panel.