arXiv Analytics

Sign in

arXiv:1901.01743 [astro-ph.HE]AbstractReferencesReviewsResources

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

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

Published 2019-01-07Version 1

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.

Related articles: Most relevant | Search more
arXiv:2308.11317 [astro-ph.HE] (Published 2023-08-22)
Quasi-periodic oscillation detected in $γ$-rays in blazar PKS 0346-27
arXiv:1401.1386 [astro-ph.HE] (Published 2014-01-07)
Multi-wavelength observations of the binary system PSR B1259-63/LS 2883 around the 2010-2011 periastron passage
arXiv:1210.4552 [astro-ph.HE] (Published 2012-10-16)
Herschel PACS and SPIRE observations of blazar PKS 1510-089: a case for two blazar zones