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Table C.1.
Upper limits in the 0.1 − 1 GeV range at the 3σ level.
| Duration [s] | Analysis period (T-t0) | Γ = −2 [erg cm−2 s−1] | Γ = −2.5 [erg cm−2 s−1] |
|---|---|---|---|
| 100 | -4800, -4700 | 6.8×10−9 | 6.7×10−9 |
| 300 | -4800, -4500 | 3×10−9 | 3.1×10−9 |
Notes. Given that DBE was not covered with LAT during the burst periods, we estimated these upper limits one orbit before at the same position of the sky for two different exposures of 100 s and 300 s.
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