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Table 2.
Fitting parameters of the HE γ-ray and X-ray spectra from Fermi-LAT and Swift-XRT during the highest VHE-flux nights 2016.
| Time | Flux (a) in 0.3–300 GeV | Flux (b) at 1.96 GeV | Γ | ||
|---|---|---|---|---|---|
| (cm−2 ⋅ s−1) | (MeV−1 ⋅ cm−2 ⋅ s−1) | ||||
| Fermi-LAT | 21:00 12th–09:00 14th June | ||||
| (MJD 57551.875–57553.375) | (9.6 ± 3.0)×10−8 | (9.7 ± 2.9)×10−12 | 1.56 ± 0.20 | ||
| Time | Flux (c) in 2–10 keV | Flux (c) in 0.5–5 keV | Γ | χ2/d.o.f | |
| (erg ⋅ cm−2 ⋅ s−1) | (erg ⋅ cm−2 ⋅ s−1) | ||||
| 02:47–03:57 13th June | |||||
| Swift-XRT | (MJD 57552.116–57552.165) |
 |
 |
 |
0.921 |
| 02:18–02:33 14th June | |||||
| (MJD 57553.096–57553.106) |
 |
 |
 |
1.11 | |
Notes. The fit function is PL defined in Sect. 2.1. The normalization energy is fixed at 1.96 GeV for the LAT and at 1 keV for the XRT.
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