The hidden population of long gamma-ray bursts from compact object mergers

Open Access

Table 1.

Type-I GRB candidates identified in this work (referred to as sample S₀).

GRB	Fermi ID	T₉₀	FWHM_min	Fluence	E_p	ℒ_*
		(s)	(ms)	(10⁻⁶ erg/cm²)	(keV)
GRB 090831	bn090831317	39.4 ± 0.6	$69_{- 18}^{+ 24}$ $Mathematical equation: $ 69^{+24}_{-18} $$	9.44 ± 0.07	256 ± 137	0.08
GRB 140306A	bn140306146	51.7 ± 0.8	$78_{- 20}^{+ 27}$ $Mathematical equation: $ 78^{+27}_{-20} $$	57.80 ± 0.09	1937 ± 209	4.84
GRB 150510A	bn150510139	51.9 ± 0.5	$84_{- 22}^{+ 29}$ $Mathematical equation: $ 84^{+29}_{-22} $$	98.62 ± 0.09	1270 ± 50	2.29
GRB 170527A	bn170527480	49.2 ± 1.6	$140_{- 36}^{+ 48}$ $Mathematical equation: $ 140^{+48}_{-36} $$	84.30 ± 0.03	1095 ± 47	1.94
GRB 190415A	bn190415173	52.5 ± 0.8	$15_{- 4}^{+ 5}$ $Mathematical equation: $ 15^{+5}_{-4} $$	60.13 ± 0.03	1834 ± 126	4.60
GRB 211019A	bn211019250	47.4 ± 0.6	$86_{- 22}^{+ 30}$ $Mathematical equation: $ 86^{+30}_{-22} $$	107.06 ± 0.05	1169 ± 40	1.90
GRB 220408B	bn220408311	32.5 ± 1.1	$110_{- 28}^{+ 38}$ $Mathematical equation: $ 110^{+38}_{-28} $$	34.60 ± 0.07	225 ± 5	−0.38
GRB 221121A	bn221121274	40.7 ± 1.6	$110_{- 37}^{+ 27}$ $Mathematical equation: $ 110^{+27}_{-37} $$	14.93 ± 0.03	889 ± 57	3.41
GRB 230304B	bn230304608	34.8 ± 0.6	$93_{- 24}^{+ 32}$ $Mathematical equation: $ 93^{+32}_{-24} $$	37.62 ± 0.03	301 ± 11	−0.25

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