--- /dev/null	Thu Jan 01 00:00:00 1970 +0000
+++ b/tests/resources/test_2608_expected	Mon Sep 15 11:44:09 2025 +0200
@@ -0,0 +1,14 @@
+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 recon-
+struction (Parsons & Hinton 2014) confirms this result. A search for
+variable emission on timescales ranging from milliseconds to sev-
+eral 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% confi-
+dence 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 observa-
+tions. 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)