Comparison of the SMBHs mass and bolometric luminosity with local (Shangguan et al. 2018) and distant quasars (Circosta et al. 2021). The dashed lines represent the constant Eddington ratios. The black hole masses and bolometric luminosities are corrected for magnification. The black hole mass of our sample is distributed between the local PG quasars and luminous quasars at cosmic noon, and the distribution of the bolometric luminosities is similar.