Table D.4.
Model C–flux-resolved.
| Parameter | F1 | F2 | F3 | F4 | F5 |
|---|---|---|---|---|---|
| Relativistic reflection | |||||
| log ξ | ![]() |
![]() |
![]() |
![]() |
![]() |
| Γ | ![]() |
![]() |
![]() |
![]() |
![]() |
| log10Lcont (erg/s) | ![]() |
![]() |
![]() |
![]() |
![]() |
| Rrefl | > 90 | > 85 | > 44 | > 18 | ![]() |
| ΔW/ν | 164.37/2 | 143.63/2 | 80.54/2 | 72.68/2 | 17.23/2 |
| P0 | 1.5 × 10−35 | 4.8 × 10−31 | 2.4 × 10−17 | 1.2 × 10−15 | 1.3 × 10−3 |
| Ionized absorber | |||||
| NH (1023 cm−2) | ![]() |
![]() |
> 142 | ![]() |
![]() |
| log ξ | < 3.01 | ![]() |
![]() |
![]() |
![]() |
| vturb (km/s) | ![]() |
![]() |
![]() |
> 8000 | < 4000 |
| vout (c) | ![]() |
![]() |
![]() |
![]() |
![]() |
| ΔW/ν | 52.26/4 | 45.25/4 | 23.16/4 | 13.60/4 | 6.80/4 |
| P0 | 2.5 × 10−10 | 8.2 × 10−9 | 5.1 × 10−4 | > 0.05 | > 0.05 |
| W-Stat/d.o.f. | 111.966/96 = 1.17 | 58.3485/93 = 0.63 | 110.809/93 = 1.19 | 126.047/99 = 1.27 | 104.672/99 = 1.06 |
Notes. Best-fit parameters for model C (relxill) applied to the five flux-resolved spectra (F1–F5). Ionized Absorber parameters are shown where required by the fit. The relativistic reflection section includes spin (a), inclination (i), ionization (log ξ), iron abundance (AFe), photon index (Γ), continuum luminosity, and reflection fraction. For each fit, the W-Stat/d.o.f. and the reduced statistic are shown. Missing parameters are indicated by −. The ΔW/ν and P0 rows report the fit improvement and AIC evidence ratio for the relxill component (vs. bare power law) and for the absorber (vs. relxill alone); see Table D.2 caption for details.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.































