Could the "Wow" signal have originated from a stochastic repeating beacon?
David Kipping, Robert Gray

TL;DR
This study explores whether the 1977 'Wow' signal could have originated from a stochastic, non-periodic repeating beacon, using likelihood modeling and additional observational data to assess its plausibility.
Contribution
It introduces a likelihood emulator approach to evaluate the stochastic repeater hypothesis for the 'Wow' signal, extending previous analyses to include new observational data.
Findings
Maximum a-posteriori likelihood of 32.3% for the stochastic repeater hypothesis.
Additional observations reduce the likelihood to 1.78%, indicating tension with the hypothesis.
Approximately 62 days of further data are needed to reach 3 sigma confidence in excluding the hypothesis.
Abstract
The famous "Wow" signal detected in 1977 remains arguably the most compelling SETI signal ever found. The original Big Ear data requires that the signal turned on/off over the span of ~3 minutes (time difference between the dual antennae), yet persisted for 72 seconds (duration of a single beam sweep). Combined with the substantial and negative follow-up efforts, these observations limit the allowed range of signal repeat schedules, to the extent that one might question the credibility of the signal itself. Previous work has largely excluded the hypothesis of a strictly periodic repeating source, for periods shorter than 40 hours. However, a non-periodic, stochastic repeater remains largely unexplored. Here, we employ a likelihood emulator using the Big Ear observing logs to infer the probable signal properties under this hypothesis. We find that the maximum a-posteriori solution has a…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
