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Table C.6.

Results from the spectral analyses of the Swift-XRT data from the B2 1811+31 high state.

Start time Exposure CPL/dof CBPL/dof F-statistic/p-value ΓPL1, BPL, Γ2, BPL) Ebreak Flux [0.3 - 10 keV]
[MJD] [s] [keV] [10−12 erg cm−2 s−1]
59125.442 2476 221/245 220/243 0.55/0.58 2.54±0.06 - 21.3±0.8
59128.283 1303 125/153 124/151 0.61/0.54 2.50±0.11 - 11.0±0.6
59132.286 1171 126/149 126/147 0.58/0.56 2.58±0.10 - 11.4±0.6
59134.853 1489 171/201 171/199 0.58/0.56 2.56±0.08 - 23.5±1.1
59136.848 2003 246/271 235/269 6.30/2.1×10−3 2.09±0.09, 2.83±0.26 1.9±0.4 24.5±2.7
59138.851 1841 253/271 237/269 9.08/1.5×10−4 2.14±0.08, 4.72±1.13 3.0±0.4 18.4±3.5
59156.828 1948 277/322 276/320 0.57/0.56 2.22±0.04 - 73.0±2.1
59157.823 1839 242/248 241/246 0.51/0.60 2.36±0.06 - 26.4±1.0

Notes. Cash statistic values assuming PL and BPL models for the source intrinsic spectrum are reported, as well as the corresponding F-statistic values and p-values for the spectral curvature test. The BPL model was preferred over the single PL model if p−value <2.7×10−3, corresponding to the 3σ confidence level. For the observations with BPL model favored over the PL one, the BPL best-fit spectral indices Γ1, BPL, Γ2, BPL and energy break Ebreak are indicated rather than the PL index ΓPL. The normalization energy E0 of the PL and BPL functional forms in Equations 1 and 2 was set to E0 = 1 keV.

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