Table 2
Best fit spectral parameters.
| Parameter | Power law | Units |
|
|
||
| n H |
|
cm-2 |
| Γ |
|
|
| N |
|
ph/(keVcm2s) @ 1 keV |
| CV0 |
|
|
| CBAT |
|
|
| CEPIC |
|
|
| F 0.2−10 keV |
|
erg s-1 cm-2 |
| F 15−150 keV |
|
erg s-1 cm-2 |
| χ 2 | 158.4 (182) | |
Notes. CV0, CEPIC, and CBAT are the constant factors to be multiplied to the model to match the Swift-XRT data that are collected with a CCD substrate voltage set to 0 Volt, EPIC data and BAT data, respectively. The constant factors relevant to the three EPIC detectors are set to the same best fit value for the three datasets. We report unabsorbed fluxes for the characteristic Swift-XRT (0.2–10 keV) and BAT (10–150 keV) energy bands.
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