A repeating X-ray signal with a period of about 28 minutes is claimed in two independent observations of NGC 4151, with uncorrected combined significance 5.2 sigma that falls to 3.2 sigma under the paper's strictest trial correction.
A $\gamma$-ray Quasi-Periodic modulation in the Blazar PKS 0301$-$243?
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abstract
We report a nominally high-confidence $\gamma$-ray quasi-periodic modulation in the blazar PKS 0301$-$243. For this target, we analyze its \emph{Fermi}-LAT Pass 8 data covering from 2008 August to 2017 May. Two techniques, i.e., the maximum likelihood optimization and the exposure-weighted aperture photometry, are used to build the $\gamma$-ray light curves. Then both the Lomb-Scargle Periodogram and the Weighted Wavelet Z-transform are applied to the light curves to search for period signals. A quasi-periodicity with a period of $2.1\pm0.3$ yr appears at the significance level of $\sim5\sigma$, although it should be noted that this putative quasi-period variability is seen in a data set barely four times longer. We speculate that this $\gamma$-ray quasi-periodic modulation might be evidence of a binary supermassive black hole.
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Detection and Characterization of Quasi-Periodic Oscillations in Seyfert Galaxy NGC 4151
A repeating X-ray signal with a period of about 28 minutes is claimed in two independent observations of NGC 4151, with uncorrected combined significance 5.2 sigma that falls to 3.2 sigma under the paper's strictest trial correction.