Table 3.
Fit parameters to the Swift-XRT spectra in each given epoch.
| State | Time | Texp | OBS ID | Model | F-test | χred2/ndf | ΓLP | F2 − 10 keV | F0.3 − 10 keV |
|---|---|---|---|---|---|---|---|---|---|
| [MJD] | [ks] | [%] | [×10−11 erg cm−2 s−1] | ||||||
| A | 58904.12262 | 1.04 | 00031531058 | LP | 0.02 | 0.97/266 | 2.23 ± 0.09 | 4.30 ± 0.34 | 6.25 ± 0.38 |
| B | 58906.36604 | 1.43 | 00031531061 | LP | 0.03 | 1.16/88 | 2.15 ± 0.05 | 4.57 ± 0.20 | 6.43 ± 0.22 |
| C | 58907.84000 | 0.59 | 00031531064 | LP | 0.14 | 0.87/196 | 2.32 ± 0.11 | 4.84 ± 0.53 | 7.29 ± 0.50 |
| D | 58908.83296 | 0.90 | 00031531063 | LP | 0.00 | 0.79/242 | 2.26 ± 0.10 | 5.84 ± 0.54 | 8.57 ± 0.55 |
Notes. Columns: (1) State. (2) Time of the observation. (3) Exposure. (4) Swift observation ID. (5) Preferred spectral model. (6) F-test (LP over PWL). (7) Reduced χ2 and number of degrees of freedom for the LP. (8) Spectral index. (9) Integral flux between 2 keV and 10 keV. (10) Integral flux between 0.3 keV and 10 keV.
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