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Table 1.

Highest energy events of Fermi-LAT GRBs for which ≥10 GeV photons arrive after T90 only.

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)
190114C 116.0 81.4 0.43 18.94 8849.2 27.0 6210.0 1
171210A 143.1 12.49 1374.6 1
171022A 13.3 13.98 4582.8 1
171010A 107.3 80.7 0.33 19.00 2891.0 25.3 2173.7 1
160623A 107.8 78.9 0.37 18.21 12039.8 24.9 8807.5 1
160521B 2.8 12.69 423.7 1
160422A 12.3 12.29 771.4 1
160310A 25.6 26.99 5886.0 1
150902A 13.6 10.59 98.9 1
140928A 17.9 51.76 2555.2 1
38.62 3100.9 1
140810A 81.7 15.38 1490.3 1
140416A 31.7 10.08 2208.3 1
140206B 27.3 10.96 6736.7 1
29.39 75494.0 1
131231A 31.2 19.0 0.64 48.29 110.4 79.3 67.2 1
17.14 844.0 28.1 514.0 1
173.17 57071.0 284.4 34757.0 0.97
130907A 115.0 51.4 1.24 50.96 17161.0 114.1 7668.0 1
130502B 24.3 31.10 222.1 1
120919B 118.0 12.70 605.0 1
120916A 53.0 21.57 13004.8 1
120526A 43.6 14.30 1354.3 1
101014A 449.4 13.60 2750.7 1
11.20 2962.0 1
100511A 42.4 46.00 161.9 1
18.00 179.8 1
100414A 26.5 11.1 1.37 29.80 34.4 70.6 14.5 1
25.13 359.5 59.5 151.8 1
100213C 60.0 34.00 3389.0 1
100116A 102.5 32.64 379.2 1
13.35 296.7 1
090926A 20.0 6.4 2.11 19.46 25.8 60.5 8.3 1
10.42 3786.0 32.4 1217.4 1
090510A 1.0 0.5 0.90 29.91 1.8 56.8 0.9 1
090427A 12.3 14.10 422.9 1

Notes. 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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