Table 2
General properties of the prompt emission of the high-redshift GRBs.
| Identifier | T90 | Epeak | Fluence | Eiso | Ref. |
|---|---|---|---|---|---|
| (s) | (keV) | (×107 erg/cm2) | (×1052 erg) | ||
| GRB 050904A | 225 ±10 | >150 | 54±2 | 34 | [1,2] |
| GRB 080913A | 8 ± 1 | 93 ± 56 | 5.6 ± 0.6 | 7 | [3] |
| GRB 090429B | 5.5±1 | 42 ± 5.6 | 3.1 ± 0.3 | 3.5 | [4,5] |
| GRB 090709A | 89±3 | 439 ± 58 | 257 ± 3 | 31 | [6,7,8] |
| GRB 100205A | 26 ± 8 | … | 4.0 ± 0.7 | … | [9] |
| GRB 120521C | 26.7 ± 4.4 | … | 11 ± 1 | 19±8 | [10] |
| GRB 120923A | 27.2 ± 3 | 44±11 | 3.2 ± 0.8 | 4.8 ± 1.6 | [11,12] |
| GRB 140515A | 23.4 ± 2.1 | 51 ± 15 | 5.9 ± 0.6 | 5.8 ± 0.6 | [13,14] |
| GRB 210905A | 870 | 144 ± 56 | 182 ± 29 | 127 ± 20 | [15] |
Notes. [1] Sakamoto et al. (2005); [2] Tagliaferri et al. (2005); [3] Greiner et al. (2009); [4] Stamatikos et al. (2009); [5] Cucchiara et al. (2011); [6] Sakamoto et al. (2009); [7] Ohno et al. (2009); [8] Cenko et al. (2010); [9] Sakamoto et al. (2010); [10] Markwardt et al. (2012a); [11] Markwardt et al. (2012b); [12] Tanvir et al. (2018); [13] Stamatikos et al. (2014); [14] Melandri et al. (2015); [15] Rossi et al. (2022).
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