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Only run tests on recent mupdf which have fixed the underlying bug. Test failed in optimised rebased; have fixed.
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No significant gamma-ray excess above the expected background | ||
is detected from the direction of FRB 20171019A, with 52 gamma | ||
candidate events from the source region and 524 background event. | ||
A second analysis using an independent event calibration and reconstruction (Parsons & Hinton 2014) confirms this result. A search for | ||
variable emission on timescales ranging from milliseconds to several minutes with tools provided in (Brun et al. 2020) does not reveal | ||
any variability above 2.2 𝜎. For the total data set of 1.8 h, 95% confidence level (C. L.) upper limits on the photon flux are derived using | ||
the method described by Rolke et al. (2005). The energy threshold | ||
of the data is highly dependent on the zenith angle of the observations. For these observations, the zenith angles range from 15 to 25 | ||
deg, which leads to an energy threshold for the stacked data set of | ||
𝐸th = 120 GeV. The upper limit on the Very High Energy (VHE) |
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