Optical quasi-periodic oscillation of the BL Lacertae object S5 0716+714 during the faint state
arXiv:1711.08641 · doi:10.3847/1538-3881/aa9d89
Abstract
In order to search for the evidence of quasi-periodic oscillation (QPO) in blazar, multicolor optical observations of the BL Lacertae object S5 0716+714 were performed from 2005 to 2012. For band on March 19 2010 with low variability amplitude and low flux level, the same quasi-periodic oscillation minutes with 99% significance levels is confirmed by ZDCF method, Lomb-Scargle method, REDFIT and fitting sinusoidal curves. The observed QPO is likely to be explained by accretion disk variability. If the observed QPO indicates an innermost stable orbital period from the accretion disk, the QPO min corresponds to a black hole mass of for a non-rotating Schwarzschild black hole and for a maximally rotating Kerr black hole.
arXiv comment29 pages, 3 figures, 6 tables, accepted for publication in AJ
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