Table 1
Spectral analysis results of H.E.S.S. II mono observations.
| Source | Year | MJD | Livetime | E 0 | Φ0 | Γ | β |
| [h] | [GeV] | [10-9 cm-2 s-1 TeV-1] | |||||
|
|
|||||||
| PKS 2155−304 | 2013 | 56 403–56 601 | 43.7 | 151 | 0.530 ± 0.018stat | 2.65 ± 0.09stat | 0.22 ± 0.07stat |
| 2014 | 56 805–56 817 | 12.3 | 177 | 0.532 ± 0.029stat | 2.82 ± 0.13stat | 0.16 ± 0.10stat | |
| 2013+2014 | 56 403–56 817 | 56.0 | 156 | 0.511 ± 0.015stat | 2.63 ± 0.07stat | 0.24 ± 0.06stat | |
|
|
|||||||
| PG 1553+113 | 2013 | 56 441–56 513 | 16.8 | 141 | 1.48 ± 0.07stat | 2.95 ± 0.23stat | 1.04 ± 0.31stat |
Notes.For both blazars, the observational period is provided along with the spectral parameters: decorrelation energy E0; differential flux at the decorrelation energy Φ0; photon index Γ; and curvature parameter β. These three parameters describe the log-parabola fit to the spectra.
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