The detection of possible -ray quasi-periodic modulation with 600 days from the blazar S2 0109+22
arXiv:2306.11579 · doi:10.1088/1538-3873/acdf1f
Abstract
In this work, we analyzed the long term gamma-ray data by a Fermi Large Area Telescope (Fermi-LAT) of blazar S2 0109+22, ranging from 2008 to 2023. The quasi-periodic oscillations (QPOs) of blazars aided in investigating the physical properties of internal supermassive black holes, the nature of variability, and the underlying radiation mechanism. We employed four different methods--Weighted Wavelet Z-transform, Lomb-Scargle periodogram, REDFIT and phase folded light curve analysis, for searching QPO signals. Our analysis identified a possible QPO behavior with a periodicity of 600 days in November 2013 to January 2023 at a significance level of 3.5 . This QPO signal sustained 9 years, corresponding to 5.6 cycles, which was in good agreement with the previously observed of periodicity 657 days in radio. We explained this phenomenon based on the accretion model and the lighthouse effect, in a binary black hole system.
arXiv comment12 pages, 8 figures,3 tables,accepted for publication in PASP
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