{ "id": "2206.10269", "version": "v1", "published": "2022-06-21T11:36:33.000Z", "updated": "2022-06-21T11:36:33.000Z", "title": "About 300 days optical quasi-periodic oscillations in the long-term light curves of the blazar PKS 2155-304", "authors": [ "Qi Zheng", "Xueguang Zhang", "Qirong Yuan" ], "comment": "13 pages, 9 figures, accepted to be published in RAA", "categories": [ "astro-ph.HE", "astro-ph.GA" ], "abstract": "Based on the long-term light curves collected from the Catalina Sky Survey (CSS) (from 2005 to 2013) and the All-Sky Automated Survey for Supernovae (ASAS-SN) (from 2014 to 2018), optical quasi-periodic oscillations (QPOs) about 300 days can be well determined in the well-known blazar PKS~2155-304 through four different methods: the generalized Lomb-Scargle periodogram (GLSP) method, the weighted wavelet Z-transform (WWZ) technique, the epoch-folded method and redfit method. The GLSP determined significance level for the periodicity is higher than 99.9999\\% based on a false alarm probability. The redfit provided confidence level for the periodicity is higher than 99\\% in ASAS-SN light curve, after considering the effects of red noise. Based on continuous autoregressive (CAR) process created artificial light curves, the probability of detecting fake QPOs is lower than 0.8\\%. The determined optical periodicity of 300 days from CSS and ASAS-SN light curves is well consistent with the reported optical periodicity in the literature. Moreover, three possible models are discussed to explain the optical QPOs in PKS 2155-304: the relativistic Frame-dragging effect, the binary black hole (BBH) model and the jet precession model.", "revisions": [ { "version": "v1", "updated": "2022-06-21T11:36:33.000Z" } ], "analyses": { "keywords": [ "long-term light curves", "days optical quasi-periodic oscillations", "blazar pks", "asas-sn light curve", "process created artificial light curves" ], "note": { "typesetting": "TeX", "pages": 13, "language": "en", "license": "arXiv", "status": "editable" } } }