Table 2.
Results of the time-resolved spectral analysis of the Swift data.
| Interval | Γ1 | Γ2 | Ecross | Flow | Fhigh | Synchrotron contribution | α | β |
|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| 1 | 3.65 ± 0.05 | 0.82 ± 0.03 | 1.62 | 0.37 ± 0.01 | 1.26 ± 0.03 | 23% | 2.59 ± 0.06 | −0.82 ± 0.01 |
| 2 | 3.76 ± 0.06 | 1.06 ± 0.03 | 1.52 | 0.39 ± 0.01 | 1.28 ± 0.03 | 23% | 2.73 ± 0.05 | −0.85 ± 0.01 |
| 3 | 3.27 ± 0.04 | 1.85 ± 0.04 | 1.91 | 0.80 ± 0.02 | 1.10 ± 0.02 | 45% | 2.78 ± 0.03 | −0.35 ± 0.01 |
| 4 | 3.38 ± 0.05 | 1.68 ± 0.03 | 1.52 | 0.52 ± 0.01 | 1.97 ± 0.01 | 21% | 2.72 ± 0.06 | −0.42 ± 0.01 |
| 5 | 2.87 ± 0.04 | 1.61 ± 0.04 | 2.10 | 1.77 ± 0.03 | 2.75 ± 0.03 | 39% | 2.46 ± 0.05 | −0.33 ± 0.01 |
| 6 | 3.02 ± 0.05 | 1.71 ± 0.04 | 1.85 | 1.01 ± 0.02 | 1.79 ± 0.02 | 36% | 2.60 ± 0.04 | −0.41 ± 0.01 |
| 7 | 3.08 ± 0.05 | 1.71 ± 0.05 | 1.32 | 0.52 ± 0.01 | 2.11 ± 0.02 | 12% | 2.51 ± 0.04 | −0.42 ± 0.01 |
| 8 | 2.73 ± 0.05 | 1.62 ± 0.03 | 1.31 | 0.31 ± 0.01 | 1.67 ± 0.01 | 16% | 2.27 ± 0.04 | −0.36 ± 0.01 |
| 9 | 2.76 ± 0.08 | 1.51 ± 0.07 | 1.36 | 0.30 ± 0.01 | 2.45 ± 0.02 | 11% | 2.27 ± 0.04 | −0.45 ± 0.01 |
| 10 | 3.00 ± 0.08 | 1.81 ± 0.06 | 1.76 | 1.11 ± 0.03 | 2.44 ± 0.01 | 31% | 2.61 ± 0.03 | −0.38 ± 0.01 |
Notes. The columns are as follows: (2) and (3) photon indices for a double power law fit with Galactic absorption; (4) energy value for the crossing point in keV of two power law lines; (5) and (6) flux of the low- and high-energy components in 10−11 erg cm−2 s−1; (7) relative contribution of the synchrotron component; (8) photon index of a logparabola fit; (9) curvature parameter of a logparabola fit.
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