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Table B.1.

Measured values for the linear polarisation and PA of GRB afterglows from the literature.

GRB Redshift Tmid PLin θ Ref
(days) (%) (°)
GRB 990510 1.62 0.7708 1.7 ± 0.2 101 ± 3 [1]
0.8583 1.6 ± 0.2 96 ± 4 [2]
1.8083 2.2 − 0.9 + 1.1 $ _{-0.9}^{+1.1} $ 112 − 17 + 15 $ _{-17}^{+15} $
GRB 990712 0.43 0.44 2.9 ± 0.4 121.1 ± 3.5 [3]
0.70 1.2 ± 0.4 116.2 ± 10.1 [3]
1.45 2.2 ± 0.7 139.1 ± 10.4
GRB 020405 0.695 1.2292 1.50 ± 0.40 172 ± 8 [4]
1.3208 9.89 ± 1.30 180 ± 4 [5]
2.2682 1.96 ± 0.33 154 ± 5 [6]
3.8792 1.47 ± 0.43 168 ± 9
GRB 020813 1.35 0.21528 2.22 ± 0.07 157.6 ± 1.0 [7]*
0.26181 1.98 ± 0.04 153.4 ± 1.7
0.34167 1.96 ± 0.07 152.0 ± 1.2
0.89792 1.07 ± 0.22 154.3 ± 5.9 [8]
0.93750 1.42 ± 0.25 137.0 ± 4.4
0.97542 1.11 ± 0.22 150.5 ± 5.5
1.01625 1.05 ± 0.23 146.4 ± 6.2
1.11667 1.43 ± 0.44 155.8 ± 8.5
1.97958 1.26 ± 0.34 164.7 ± 7.4
GRB 021004 2.33 0.37 1.72 ± 0.56 187.7 ± 8.3 [9]
0.38 2.09 ± 0.60 173.0 ± 7.9
GRB 030329 0.17 0.5321 0.92 ± 0.10 86.13 ± 2.43 [10]**
0.5492 0.86 ± 0.09 86.74 ± 2.40
0.5671 0.87 ± 0.09 88.60 ± 2.64
0.5850 0.80 ± 0.09 91.12 ± 2.88
0.6921 0.66 ± 0.07 78.52 ± 2.94
0.7129 0.66 ± 0.07 76.69 ± 2.89
0.7342 0.56 ± 0.05 74.37 ± 3.11
1.5204 1.97 ± 0.48 83.20
1.5500 1.37 ± 0.11 61.65 ± 2.38
1.5800 1.50 ± 0.12 62.29 ± 2.44
1.6700 1.07 ± 0.09 59.41 ± 2.51
1.7000 1.09 ± 0.08 66.07 ± 2.45
1.7200 1.02 ± 0.08 67.05 ± 2.60
1.7400 1.13 ± 0.08 70.56 ± 2.51
2.6800 0.52 ± 0.06 30.76 ± 5.04
2.7000 0.52 ± 0.12 12.55 ± 4.63
2.7200 0.31 ± 0.07 24.50 ± 6.94
3.5400 0.57 ± 0.09 53.85 ± 4.08
3.5600 0.53 ± 0.08 57.08 ± 4.06
3.5800 0.42 ± 0.10 62.21 ± 6.10
5.6600 1.68 ± 0.18 66.32 ± 3.38
7.6400 2.22 ± 0.28 75.16 ± 3.32
9.5900 1.33 ± 0.14 70.91 ± 3.31
13.6000 2.04 ± 0.57 1.16 ± 7.64
22.5000 0.58 ± 0.10 42.7 ± 9.26
37.5000 1.48 ± 0.48 25.42 ± 9.41
XR 080109 0.007 3.6416 0.95 ± 0.20 114.9 ± 5.9 [11]
5.5552 0.85 ± 0.28 106.1 ± 9.4
20.6279 1.05 ± 0.06 135.3 ± 1.7
20.6443 1.28 ± 0.06 132.5 ± 1.4
52.5578 1.42 ± 0.46 139.0 ± 9.1
GRB 080928 1.6919 1.7 4.49 − 0.96 + 1.16 $ ^{+1.16}_{-0.96} $ 41.3 ± 6.3 [12]
GRB 090102 1.55 0.0025 10.1 ± 1.3 – [13]
GRB 091208B 1.063 0.0042 10.4 ± 2.5 92 ± 6 [14]
GRB 091018 0.971 0.2461 1.07 ± 0.30 179.2 ± 16.1 [15]
0.4548 1.44 ± 0.32 2.2 ± 12.6
1.1394 1.73 ± 0.36 69.8 ± 11.7
1.1552 3.25 ± 0.35 57.6 ± 6.1
1.1735 1.99 ± 0.35 27.6 ± 10.0
1.1893 1.42 ± 0.36 114.6 ± 14.0
1.3918 0.97 ± 0.32 32.8 ± 17.8
1.4493 1.08 ± 0.35 88.7 ± 17.9
2.3902 1.45 ± 0.37 169.0 ± 14.3
GRB 120308 2.22 0.0033 28 − 4 + 4 $ ^{+4}_{-4} $ 34 ± 4 [16]
0.0042 23 − 4 + 4 $ ^{+4}_{-4} $ 44 ± 6
0.0052 17 − 4 + 5 $ ^{+5}_{-4} $ 51 ± 9
0.0062 16 − 4 + 7 $ ^{+7}_{-4} $ 40 ± 10
0.0081 16 − 4 + 5 $ ^{+5}_{-4} $ 55 ± 9
GRB 121024A 2.298 0.2194 4.09 ± 0.2 163.7 ± 2.8 [17]
0.2302 4.83 ± 0.2 160.3 ± 2.3
0.2782 3.82 ± 0.2 182.7 ± 3.0
0.2928 3.12 ± 0.19 175.3 ± 3.5
0.3088 3.39 ± 0.18 178.0 ± 2.9
0.3252 3.49 ± 0.18 180.3 ± 3.0
0.3412 3.2 ± 0.18 174.5 ± 3.3
1.2995 2.66 ± 0.6 83.0 ± 12.6
GRB 191221B 1.148 0.121 1.4 ± 0.1 68 ± 5 [18]
0.417 1.0 ± 0.1 57 ± 5
2.525 1.3 ± 0.1 62 ± 6
GRB 210610B 1.1345 0.0973 4.27 ± 1.45 183 ± 9 This work
0.2407 0.22 ± 0.20 267 ± 19
0.2688 0.03 ± 0.17 –
0.2793 0.15 ± 0.28 –
1.2655 2.27 ± 0.22 237 ± 3
1.2829 1.69 ± 0.27 238 ± 5
GRB 210619B 1.937 0.1057 2.2 ± 0.7 22.0 ± 10.0 [19]
0.1070 2.6 ± 0.8 2.0 ± 8.0

Notes. We include only the values from literature for which we calculate P/σP > 3.0 with Tmid in observer frame. (*) From the spectropolarimetric measurements in (Barth et al. 2003), since we do not consider chromaticity in the polarisation, we show the median value of the measured polarisation on the different wavelength bins, for the three epochs they presents. (**) For GRB 030329 we made use of the data presented in Covino & Gotz (2016) and, specifically, the results presented in this review taken from Greiner et al. (2003) and Magalhaes et al. (2003). References for values from literature are: [1] (Covino et al. 1999), [2] (Wijers et al. 1999), [3] (Rol et al. 2000), [4] (Masetti et al. 2003), [5] (Bersier et al. 2003), [6] (Covino et al. 2003), [7] (Barth et al. 2003), [8] (Gorosabel et al. 2004), [9] (Rol et al. 2003), [10] (Covino & Gotz 2016), [11] (Gorosabel et al. 2010), [12] (Brivio et al. 2022), [13] (Steele et al. 2009), [14] (Uehara et al. 2012), [15] (Wiersema et al. 2012), [16] (Mundell et al. 2013), [17] (Wiersema et al. 2014), [18] (Urata et al. 2023), [19] (Mandarakas et al. 2023)

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