The most distant optically polarised GRB afterglow: GRB 240419A at z = 5.178

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Table 1.

GRBs with detected early-time (t − t₀ ≲ 10 000 s) polarised optical light from the afterglow phase.

GRB	z	P [%]	t − t₀ [s]	Rest frame t − t₀ [s]	Reference
090102	1.55	10.2 ± 1.3	190	74.5	Steele et al. (2009)
091208B	1.063	10.4 ± 2.5	149–706	72–342	Uehara et al. (2012)
101112A	≲3.5	$6_{- 2}^{+ 3}$ $6^{+3}_{-2}$	176–355	–	Steele et al. (2017)
		$6_{- 3}^{+ 4}$ $6^{+4}_{-3}$	715–893	–
110205A	2.22	$13_{- 9}^{+ 13}$ $13^{+13}_{-9}$	240–840	74.5–291	Steele et al. (2017)
120308A	2.2	$28_{- 4}^{+ 4}$ $28^{+4}_{-4}$	240	75	Mundell et al. (2013)
		$16_{- 4}^{+ 5}$ $16^{+5}_{-4}$	800	250
121024A	2.298	4.09 ± 0.20	9698	2854	Wiersema et al. (2014)
180720B	0.654	∼0.5 − 8	80–2000	48.4–1209	Arimoto et al. (2024)
190114C	0.4245	7.7 ± 1.1	52	36.5	Jordana-Mitjans et al. (2020)
		∼2 − 4	108–2000	76–1375
191016A	3.3	4.7 ± 4.1	3987–4587	927–1067	Shrestha et al. (2022)
		11.2 ± 6.6	4587–5187	1067–1206
		14.6 ± 7.2	5787–6387	1346–1485
191221B	1.148	1.4 ± 0.1	10454	4867	Urata et al. (2023)
210610B	1.1341	4.27 ± 1.45	10411	4878.5	Agüí Fernández et al. (2024)
210619B	1.937	2.2 ± 0.7	6537	2225.7	Mandarakas et al. (2023)
		2.6 ± 0.8	6751	2298.6

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