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Table 1.

Short GRB rest-frame energetics and prompt emission peak energy.

GRB z Ep Eiso
[keV] [1051 erg]
050509B (a)(b) 0.2248
050709 (a) 0.16 0.033 ± 0.001
050724 (a) 0.2570
051221A 0.547 621.5 ± 127 2.6 ± 0.35
060614 (a) 0.125 2.4 ± 0.4
061006 (a) 0.4377 2.0 ± 0.3
070714B 0.92 2150 ± 1045 9.8 ± 2.4
080123 0.495 105 ± 21.5 0.13 ± 0.015
080905A (b) 0.122 579 ± 77.5 0.032 ± 0.003
090426 2.609 177 ± 72 5.4 ± 0.65
090510 (b) 0.903 8090 ± 594 74.3 ± 3.2
100117A (b) 0.92 549 ± 84.5 0.81 ± 0.10
100206A (b) 0.41 639 ± 131 0.74 ± 0.50
100625A (b) 0.452 701 ± 115 0.75 ± 0.03
100816A 0.805 247 ± 8.5 7.3 ± 0.25
101219A (b) 0.718 842 ± 155 4.9 ± 0.7
101224A (b) 0.72 568 ± 475 0.34 ± 0.07
110717A 0.92 937 ± 297 1.87 ± 0.23
111117A (b) 2.221 663 ± 70 8.3 ± 0.9
130603B 0.356 895 ± 136 2.12 ± 0.23
150120A 0.46 190 ± 146 0.21 ± 0.05
160410A 1.717 4660 ± 1445 40.0 ± 4.00
160624 0.483 1247 ± 531 4.5 ± 0.4
160821B 0.16 98 ± 22 0.12 ± 0.015
170428A 0.454 1428 ± 573 2.1 ± 0.45

Notes. GRB 090426 and 100816 (in italics) are suspected long GRBs (see discussion in D14).

(a)

Belongs to the Type I Gold Sample of Z09.

(b)

Has fNC ≥ 0.5 in the sample of B13.

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