| GRB | z | Ep,o (keV) |
|
band (keV) | GCN | |||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| 090516 | 4.109 | 190 |
-1.5 |
[-2.2] |
15 |
20-1200 | 9422 | |
| 090715B | 3.00 | 134 |
-1.1 |
[-2.2] |
9.3 |
20-2000 | 9679 | |
| 090812 | 2.452 | 586 |
-1.03 |
[-2.2] |
26.1 |
15-1400 | 9821 | |
| 090926B | 1.24 | 91 |
-0.13 |
[-2.2] |
8.7 |
10-1000 | 9957 | |
| 091018 | 0.971 | 28 |
-1.53 |
[-2.2] |
1.44 |
10-1000 | 10 045 | |
| 091029 | 2.752 | 61.4 |
-1.46 |
[-2.2] |
2.4 |
15-150 | 10 103 | |
| 090618 | 0.54 | 155.5 |
-1.26 |
-2.50 |
270 |
8-1000 | 9535 | |
| 090902B | 1.822 | 775 |
-0.696 |
-3.85 |
374 |
50-10 000 | 9866 | |
| 090926 | 2.1062 | 314 |
-0.75 |
-2.59 |
145 |
8-1000 | 9933 | |
| 091003 | 0.8969 | 486.2 |
-1.13 |
-2.64 |
37.6 |
8-1000 | 9983 | |
| 091020 | 1.71 | 103 |
-0.93 |
-1.9 |
10.4 |
20-2000 | 10 057 | |
| 091127 | 0.49 | 36 |
-1.27 |
-2.20 |
18.7 |
8-1000 | 10 204 | |
| 091208B | 1.0633 | 124 |
-1.44 |
-2.32 |
5.8 |
8-1000 | 10 266 |
Notes. In this table we show (1) the name of GRB, (2) the spectral model used for the fitting of the spectra, (3) the redshift, (4) the peak energy observed, (5) the softer spectral index, absent for the cut-off power law spectral model, (6) the higher spectral index, (7) the observed fluence and (8) the detector band considered for the estimate of the fluence, (9) the GCN reference for the GRB, where we took the spectral data.
References. (Sakamoto et al. 2009a), (McBreen 2009a), (Golenetskii et al. 2009a), (Sakamoto et al. 2009b), (Bissaldi & Connaughton 2009), (Bissaldi 2009), (Briggs 2009), (Rau 2009), (Golenetskii et al. 2009b), (Golenetskii 2009), (Barthelmy et al. 2009), (Wilson-Hodge & Preece 2009), (McBreen 2009b).
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