Fast radio bursts: the observational case for a Galactic origin
Dan Maoz, Abraham Loeb, Yossi Shvartzvald, Monika Sitek, Michael, Engel, Flavien Kiefer, Marcin Kiraga, Amir Levi, Tsevi Mazeh, Michal Pawlak,, R. Michael Rich, Lev Tal-Or, Lukasz Wyrzykowski

TL;DR
This paper presents observational evidence supporting the hypothesis that fast radio bursts originate from nearby flare stars, challenging the cosmological origin theory and suggesting a local stellar source based on optical and radio data analysis.
Contribution
It provides new optical observations of potential flare star counterparts in FRB fields and re-evaluates the likelihood of a Galactic origin for FRBs, including the case of repeating bursts.
Findings
Possible flare star associations in multiple FRB fields.
High probability that two FRBs are from the same repeating source.
Dispersion measures are inconsistent with a cosmological origin.
Abstract
There are by now ten published detections of fast radio bursts (FRBs), single bright GHz-band millisecond pulses of unknown origin. Proposed explanations cover a broad range from exotic processes at cosmological distances to atmospheric and terrestrial sources. Loeb et al. have previously suggested that FRB sources could be nearby flare stars, and pointed out the presence of a W-UMa-type contact binary within the beam of one out of three FRB fields that they examined. Using time-domain optical photometry and spectroscopy, we now find possible flare stars in additional FRB fields, with one to three such cases among eight FRB fields studied. We evaluate the chance probabilities of these possible associations to be in the range 0.1% to 9%, depending on the input assumptions. Further, we re-analyze the probability that two FRBs recently discovered 3 years apart within the same radio beam…
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