# Variability studies and modeling of the blazar PKS 2155-304 in the light   of a decade of multi-wavelength observations

**Authors:** J. Chevalier, D.A. Sanchez, P. D. Serpico, J.-P. Lenain, G. Maurin

arXiv: 1901.01743 · 2019-01-16

## TL;DR

This study analyzes a decade of multi-wavelength data on blazar PKS 2155-304, revealing log-normal variability, potential periodicity, and modeling its behavior with a synchrotron self-Compton approach.

## Contribution

It provides a comprehensive variability analysis over ten years and introduces a successful time-dependent model to explain observed behaviors and potential periodicity.

## Key findings

- Optical and X-ray variability follow a log-normal distribution.
- A tentative 700-day periodicity is identified.
- A one-zone synchrotron self-Compton model reproduces variability evolution.

## Abstract

The variability of the high-frequency peaked BL Lac object PKS 2155-304 is studied using almost 10 years of optical, X-ray and gamma-rays data. Publicly available data have been gathered and analyzed with the aim to characterize the variability and to search for log-normality or periodic behavior. The optical and X-ray range follow a log-normal process; a hint for a periodicity of about 700 days is found in optical and in the high energy (100 MeV <E<300 GeV) range. A one zone, time-dependent, synchrotron self-Compton model is successfully used to reproduce the evolution with energy of the variability and the tentatively reported periodicity.

## Full text

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## Figures

23 figures with captions in the complete paper: https://tomesphere.com/paper/1901.01743/full.md

## References

56 references — full list in the complete paper: https://tomesphere.com/paper/1901.01743/full.md

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Source: https://tomesphere.com/paper/1901.01743