Table 2 GRB candidates for the four PeV neutrinos

From: Lorentz violation from gamma-ray burst neutrinos

Event

E (PeV)

GRB

z

Δtobs (103 s)

#14

1.04

110725Ac

2.15b

1320.217

110730A

2.15b

907.885

110731A

2.83

782.096

110808B

0.5b

74.303

110905A

2.15b

−2309.121

#20

1.14

111229A

1.3805

384.970

120119Cc

2.15b

−1940.176

120210A

0.5b

−3304.901

#35

2.0

120919A

2.15b

6539.722

121229A

2.707

−2091.621

130121Ac

2.15b

−4046.519

ATel

2.6

140427Ac

2.15b

3827.439

#7856

140516B

2.15b

2185.942

  1. The GRB candidates here are selected by the time and direction criteria (detailed in Methods). For every one of the four events, there exists a candidate marked by c that satisfy the strict time criterion and is consistent with the regularity of TeV neutrinos. The mark b represents a “best guess” value of the redshift, i.e., z = 2.15 for “long bursts” and z = 0.5 for “short bursts”.
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