Table 2.
Best fit-value of the parameters for the model TBabs*(zpowerlw+relxill).
| Parameter | Value | Units |
|---|---|---|
| Galactic absorption | ||
| NH* | 3.50 | ×1020 cm−2 |
| Relativistic effects | ||
| Γ | 1.91 ± 0.02 | – |
| z* | 0.412 | – |
| Nrel | 4.77 ± 0.11 |
 |
| logξ |
 |
erg s−1 cm |
| a* | 0.998 | – |
| Rin | > 38 | Rg |
| Rout* | 103 | Rg |
| Rf | 0.09 ± 0.04 | – |
| i* | 30 | ° |
| β* | 3 | – |
| Ecut* | 300 | keV |
| AFe* | 1 | A⊙ |
| Power-law 2 (jet) | ||
| Γ* | 1.29 | – |
| Npl* | 8.15 |
 |
| z* | 0.412 | – |
Notes. Nrel is the normalization in relxill (Dauser et al. 2016). Ecut is the energy of the observed cut-off; AFe is the reflector iron abundance in solar units; β is the coronal emissivity slope, which is parameterized as a single power law. The starred parameters are the ones kept frozen during the fit. Upper and lower limits are calculated at a 90% confidence level.
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