Intrinsic $\gamma$-ray luminosity, black hole mass, jet and accretion in Fermi blazars

Understand

We have analyzed a large sample of clean blazars detected by Fermi Large Area Telescope (LAT).

• Using literature and calculation, we obtained intrinsic $\gamma$-ray luminosity excluding beaming effect, black hole mass, broad-line luminosity (used as a proxy for disk luminosity), jet kinetic power from "cavity" power and bulk Lorentz factor for parsec-scale radio emission, and studied the distributions of these parameters and relations between them.
• Our main results are as follows.
• (i) After excluding beaming effect and redshift effect, intrinsic $\gamma$-ray luminosity with broad line luminosity, black hole mass and Eddington ratio have significant correlations.