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 | ΓPL (Γ1, 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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