Mercurial > hgrepos > Python2 > PyMuPDF
comparison tests/resources/test_2608_expected_1.26 @ 1:1d09e1dec1d9 upstream
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| author | Franz Glasner <fzglas.hg@dom66.de> |
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| date | Mon, 15 Sep 2025 11:37:51 +0200 |
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| -1:000000000000 | 1:1d09e1dec1d9 |
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| 1 No significant gamma-ray excess above the expected background | |
| 2 is detected from the direction of FRB 20171019A, with 52 gamma | |
| 3 candidate events from the source region and 524 background event. | |
| 4 A second analysis using an independent event calibration and reconstruction (Parsons & Hinton 2014) confirms this result. A search for | |
| 5 variable emission on timescales ranging from milliseconds to several minutes with tools provided in (Brun et al. 2020) does not reveal | |
| 6 any variability above 2.2 ๐. For the total data set of 1.8 h, 95% confidence level (C. L.) upper limits on the photon flux are derived using | |
| 7 the method described by Rolke et al. (2005). The energy threshold | |
| 8 of the data is highly dependent on the zenith angle of the observations. For these observations, the zenith angles range from 15 to 25 | |
| 9 deg, which leads to an energy threshold for the stacked data set of | |
| 10 ๐ธth = 120 GeV. The upper limit on the Very High Energy (VHE) |