Gamma-ray Flux Distribution and Non-linear behavior of Four LAT Bright AGNs
Pankaj Kushwaha (1, 2), Atreyee Sinha (2), Ranjeev Misra (2), K. P., Singh (3), E. M. de Gouveia Dal Pino (1) ((1) IAG-USP, Sao Paulo, Brazil (2), IUCAA, Pune, India (3) TIFR, Mumbai, India)

TL;DR
This study statistically characterizes gamma-ray emission from four bright AGNs, revealing non-linear variability patterns and suggesting a multiplicative process, with implications for jet physics and central engine connections.
Contribution
It provides the first detailed statistical analysis of gamma-ray flux distributions and variability in four bright AGNs, highlighting non-linear behavior and potential physical models.
Findings
Blazars' flux distributions are consistent with a lognormal, indicating non-linear variability.
Flux-rms relation is linear for three blazars, supporting multiplicative variability.
Power spectra suggest scale-free shot noise with possible break points.
Abstract
We present a statistical characterization of the -ray emission from the four \emph{Fermi}-LAT sources: FR I radio galaxy NGC 1275, BL Lac Mrk 421, FSRQs B2 1520+31 and PKS 1510-089 detected almost continuously over a time integration of 3-days between August 2008 - October 2015. The observed flux variation is large, spanning orders of magnitude between the extremes except for Mrk~421. We compute the flux distributions and compare with Gaussian and lognormal ones. We find that the 3 blazars have distribution consistent with a lognormal, suggesting that the variability is of a non-linear, multiplicative nature. This is further supported by the computation of the flux-rms relation, which is observed to be linear for the 3 blazars. However, for NGC 1275, the distribution does not seem to be represented either by a lognormal or a Gaussian, while its flux-rms relation is…
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