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Table 3.

Events with the highest energy of Fermi-LAT GRBs for which ≥10 GeV photons arrive both within T90 and thereafter.

GRB properties Photon properties

Name . T90(a)of T90(b)sf Redshift (c) Energy (d)of Arrival time (e)of Energy (f)sf Arrival time (g)sf P (h)
160509A 369.7 170.4 1.17 51.90 55.7 112.6 25.7 1
41.51 221.4 90.1 102.0 1
28.90 69688.6 62.7 32114.6 1
130427A 138.2 103.1 0.34 94.12 243.6 126.1 181.8 1
77.11 19.1 103.3 14.2 1
57.42 256.7 76.9 191.6 1
38.67 78.8 51.8 58.8 1
38.19 3410.3 51.2 2545.2 1
33.65 34366.6 45.1 25648.6 1
28.41 48.0 38.1 35.8 1
26.90 85.2 36.1 63.6 1
25.36 141.5 34.0 105.6 1
19.27 6063.0 25.8 4524.9 1
17.08 217.9 22.9 162.6 1
14.90 119.7 20.0 89.4 1
12.87 80.9 17.2 60.4 1
12.18 64.9 16.3 48.4 1
12.00 23.9 16.1 17.8 1
11.74 214.4 15.7 160.0 1
10.85 23.7 14.5 17.6 1
090902B 19.3 6.8 1.82 21.72 332.2 61.3 117.7 1
18.11 26.5 51.1 9.4 1
15.40 45.9 43.5 16.3 1
14.22 14.5 40.1 5.1 1
12.66 42.7 35.7 15.1 1
11.89 12.0 33.6 4.2 1

Notes. The unit of energy is GeV, T90 and arrival times are in seconds.

(a,d,e)

Observation frameof;

(b,f,g)

source framesf;

(h)

probability of the photon being associated with that GRB.

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