Table 1
Five GRBs used for the determination of the slope parameter γ of the correlation.
| GRB | z | Ep,i (keV) | F0 (erg cm-2 s-1) | τ (s) | α X |
|
|
|||||
| 060729 | 0.54 | 104 ± 24 | (2.32 ± 0.05) × 10-11 | 61462 ± 2844 | −1.71 ± 0.03 |
| 081007 | 0.5295 | 61 ± 15 | (4.48 ± 0.64) × 10-11 | 2178 ± 457 | −1.17 ± 0.04 |
| 090424 | 0.544 | 273 ± 5 | (4.20 ± 0.26) × 10-9 | 204 ± 16 | −1.20 ± 0.01 |
| 090618 | 0.54 | 257 ± 41 | (1.18 ± 0.03) × 10-9 | 1206 ± 47 | −1.46 ± 0.01 |
| 100621A | 0.542 | 146 ± 23 | (1.75 ± 0.22) × 10-10 | 3613 ± 746 | −1.05 ± 0.03 |
Notes. In the Col. 1 is shown the GRB name, in Col. 2 the redshift z, in Col. 3 the intrinsic peak energy of the burst, in Col. 4 the initial flux of the afterglow additional component F0 in the common rest-frame energy range (0.3–10) keV, in Col. 5 the time parameter (τ), in Col. 6 the late power-law decay index (αX).
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