Table 1.
Spectral energy distribution in the VHE band.
| Energy | Energy low | Energy high | 95% flux UL |
|---|---|---|---|
| (TeV) | (TeV) | (TeV) | (10−13 TeV cm−2 s−1) |
| 0.162 (0.169) | 0.095 | 0.300 | 9.0 (8.9) |
| 0.510 (0.533) | 0.300 | 0.949 | 3.0 (3.2) |
| 1.613 (1.685) | 0.949 | 3.000 | 2.8 (3.1) |
| 5.103 (5.332) | 3.000 | 9.487 | 2.1 (2.4) |
Notes. Differential flux ULs with a spectral index of Γ = 2.83 (Γ = 2.0) for four logarithmic energy bins between 0.095 and 9.5 TeV. First column: average energy of the bin, reweighed according to the assumed spectral slope and the detected number of excesses in that bin (Lafferty & Wyatt 1995). Central columns: lower and upper boundaries of the energy bins. Last column: flux ULs computed in each energy bin at a 95% confidence level.
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