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Table 5
Comparison of the derived upper limit with the estimated photon flux derived using the publicly available spectral information preliminarily reported by GCN Circulars.
| GRB | UL (× 10-3) ph cm-2 s-1 | Expected (× 10-3) ph cm-2 s-1 |
|
|
||
| 071010B | 1.21 |
|
| 080721 | 3.33 |
|
| 080723B | 0.95 |
|
| 090131 | 1.99 |
|
| 090222 | 4.05 |
|
| 090618 | 0.65 |
|
| 090620 | 2.88 |
|
| 090709 | 0.40 |
|
| 090904B | 0.77 |
|
| 091010 | 0.30 |
|
|
|
||
| 070724B | 0.69 |
|
| 070824 | 4.09 |
|
| 080413A | 1.13 |
|
| 080413B | 2.49 |
|
| 080613B | 0.75 |
|
| 080714 | 1.19 |
|
| 080916A | 2.02 |
|
| 081001 | 5.48 |
|
| 081130B | 3.89 |
|
| 081203A | 2.38 |
|
| 081224 | 2.68 |
|
| 090319 | 0.52 |
|
| 090326 | 2.32 |
|
| 090410 | 0.64 |
|
| 090418B | 0.33 |
|
| 090516 | 0.33 |
|
| 090516B | 0.80 |
|
| 090715B | 0.10 |
|
Notes. Upper (lower) rows refer to events where the prompt spectrum is well fit by a Band (cutoff power law) model.
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