Confirmation of the 62 Day X-Ray Periodicity from M82
Philip Kaaret, Hua Feng

TL;DR
This study confirms a 62-day X-ray periodicity in M82 using extensive monitoring data, supporting the hypothesis that it results from orbital motion in an X-ray binary system.
Contribution
It provides the first confirmation of the 62-day periodicity with high significance and coherence, strengthening the orbital motion interpretation.
Findings
Confirmed the 62-day periodicity with high significance
Observed a sinusoidal light curve with consistent amplitude
Estimated a very low probability of chance occurrence (6E-7)
Abstract
Using 400 days of new X-ray monitoring of M82, we confirm the 62 day periodicity previously reported. In the full data set spanning 1124 days, we find a period of 62.0 +/- 0.3 days and a coherence, Q = 22.3, that is consistent with a strictly periodic signal. We estimate that the probability of chance occurrence of our observed signal is 6E-7. The light curve folded at this period is roughly sinusoidal and has a peak to peak amplitude of (0.99 +/- 0.10) x 10^-11 erg cm^-2 s^-1. Confirmation of the periodicity strengthens our previous suggestion that the 62 day modulation is due to orbital motion within an X-ray binary.
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