Table 1.
Sample of GRBs with redshift z, jet half-opening angle θj – both in the homogeneous interstellar medium (ISM) and wind profile (W) –, the Lorentz factor Γ0, and the minimum variability timescale (MVT).
GRB | z |
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Γ0 | MVT | m | q | σint | N | (log(Ep, i/keV))c |
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(10−2 rad) | (10−2 rad) | (s) | ||||||||
090102 | 1.547 | n.a. | n.a. |
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18 | 2.52 ± 0.08 |
090323 | 3.5832 | 10.3 ± 4.3 | 4.5 ± 1.2 |
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32 | 2.59 ± 0.21 |
090328 | 0.736 | n.a. | n.a. |
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24 | 3.07 ± 0.11 |
090424 | 0.544 | < 23.1 | < 16.1 |
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34 | 2.27 ± 0.03 |
091208B | 1.0633 | < 14.8 | < 13.8 |
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13 | 2.32 ± 0.05 |
100414A | 1.368 | n.a. | n.a. |
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16 | 2.58 ± 0.24 |
100728A | 1.567 | n.a. | n.a. |
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46 | 2.77 ± 0.03 |
100906A | 1.727 | 2.9 ± 0.1 | 3.0 ± 0.1 | < 369 |
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9 | 2.32 ± 0.08 |
120711A | 1.405 | n.a. | n.a. |
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27 | 2.72 ± 0.08 |
140508A | 1.027 | n.a. | n.a. |
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32 | 2.51 ± 0.08 |
140512A | 0.725 | 4.7 ± 0.1 | 5.2 ± 0.1 |
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21 | 2.98 ± 0.12 |
151027A | 0.81 | 7.9 ± 0.9 | 8.3 ± 0.6 |
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15 | 2.82 ± 0.32 |
160509A | 1.17 | 9.2 ± 0.7 | 5.4 ± 0.3 |
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50 | 2.63 ± 0.04 |
160625B | 1.406 | 14.8 ± 1.0 | 6.0 ± 0.3 |
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73 | 2.53 ± 0.06 |
170405A | 3.510 | 2.0 ± 0.1 | 2.8 ± 0.1 | n.a. |
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23 | 2.76 ± 0.16 |
171010A (a) | 0.3285 | < 11.0 | n.a. |
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162 | 2.46 ± 0.05 |
180720B | 0.654 | 7.2 ± 0.7 | 5.3 ± 0.3 | n.a. |
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93 | 2.66 ± 0.03 |
181020A | 2.938 | 2.1 ± 0.3 | 2.0 ± 0.2 | n.a. |
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10 | 2.66 ± 0.21 |
190114C | 0.4245 | 3.2 ± 0.5 | 3.2 ± 0.3 | n.a. |
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64 | 2.53 ± 0.04 |
221010A (b) | 4.615 |
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n.a. | n.a. | n.a. |
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31 | 2.56 ± 0.10 |
Notes. Values of z and θj are from Zhao et al. (2020), Γ0 from Ghirlanda et al. (2018), and MVT from Camisasca et al. (2023). Also reported are the best-fit parameters of the Ep, i–Liso correlation (90% confidence), the number of spectra N, and the representative value of log Ep, i computed at a common reference luminosity (see Sect 3.2).
is taken from Chand et al. (2019).
z and are taken from Zhu et al. (2023).
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