Characterizing the Optical Variability of Bright Blazars: Variability-Based Selection of Fermi AGN

TL;DR

This study demonstrates that optical variability analysis using a damped random walk model effectively identifies blazars and associates them with gamma-ray sources, providing insights into jet physics and improving source classification in large surveys.

Contribution

The paper introduces a variability-based method for selecting blazars using optical light curves, achieving high efficiency and completeness even with shallow survey data.

Findings

High efficiency (>88%) in recovering known Fermi AGN counterparts.

Optical variability timescale in blazars is approximately 3 years in the jet rest frame.

Blazar variability is stochastic and influenced by relativistic beaming.

Abstract

We investigate the use of optical photometric variability to select and identify blazars in large-scale time-domain surveys, in part to aid in the identification of blazar counterparts to the ~30% of gamma-ray sources in the Fermi 2FGL catalog still lacking reliable associations. Using data from the optical LINEAR asteroid survey, we characterize the optical variability of blazars by fitting a damped random walk model to individual light curves with two main model parameters, the characteristic timescales of variability (tau), and driving amplitudes on short timescales (sigma). Imposing cuts on minimum tau and sigma allows for blazar selection with high efficiency E and completeness C. To test the efficacy of this approach, we apply this method to optically variable LINEAR objects that fall within the several-arcminute error ellipses of gamma-ray sources in the Fermi 2FGL catalog. Despite the extreme stellar contamination at the shallow depth of the LINEAR survey, we are able to recover previously-associated optical counterparts to Fermi AGN with E > 88% and C = 88% in Fermi 95% confidence error ellipses having semimajor axis r < 8'. We find that the suggested radio counterpart to Fermi source 2FGL J1649.6+5238 has optical variability consistent with other gamma-ray blazars, and is likely to be the gamma-ray source. Our results suggest that the variability of the non-thermal jet emission in blazars is stochastic in nature, with unique variability properties due to the effects of relativistic beaming. After correcting for beaming, we estimate that the characteristic timescale of blazar variability is ~3 years in the rest-frame of the jet, in contrast with the ~320 day disk flux timescale observed in quasars. The variability-based selection method presented will be useful for blazar identification in time-domain optical surveys, and is also a probe of jet physics.