Abstract:
We present a catalog of central engine properties, i.e., black hole mass (MBH) and accretion luminosity (Ldisk), for a
sample of 1077 blazars detected with the Fermi Large Area Telescope. This includes broad emission-line systems
and blazars whose optical spectra lack emission lines but are dominated by the absorption features arising from the
host galaxy. The average MBH for the sample is (log MBH,all Msun) = 8.60, and there is evidence suggesting the
association of more massive black holes with absorption-line systems. Our results indicate a bimodality of Ldisk in
Eddington units (Ldisk/LEdd) with broad-line objects tend to have a higher accretion rate (Ldisk/LEdd > 0.01). We
have found that Ldisk/LEdd and Compton dominance (CD; the ratio of the inverse Compton to synchrotron peak
luminosities) are positively correlated at the >5σ confidence level, suggesting that the latter can be used to reveal
the state of accretion in blazars. Based on this result, we propose a CD-based classification scheme. Sources with
CD > 1 can be classified as high-Compton-dominated or HCD blazars, whereas those with CD ≤ 1 are low-
Compton-dominated (LCD) objects. This scheme is analogous to that based on the mass accretion rate proposed in
the literature; however, it overcomes the limitation imposed by the difficulty in measuring Ldisk and MBH for objects
with quasi-featureless spectra. We conclude that the overall physical properties of Fermi blazars are likely to be
controlled by the accretion rate in Eddington units.
