Table 2
Continuum parameters of the spectral fit of the baseline model to the relatively unabsorbed 2006 XMM-Newton observation.
| [pow+xillver] ∗ | ||
| zxipcf(wa 1 ) ∗ zxipcf(wa 2 ) ∗ zxipcf(wa 3 ) ∗ tbnew_simple(local) | ||
|
|
||
| Mod. comp. | Parameter | Value ± uncert. |
|
|
||
| 0400270101: χ2 (d.o.f.) = 1341.1 (953) | ||
|
|
||
| SXPL | norm |
|
| Γ | 1.57∗ | |
| HXPL | norm |
|
| Γ |
|
|
| Ion. Refl. | norm |
|
| log ξ (erg cm s-1) |
|
|
| Z Fe |
|
|
| z (absolute) | 0.00386∗ | |
| WA 1 | NH (1022cm-2) |
|
| log ξ (erg cm s-1) |
|
|
| f cvr | 1∗ | |
| z (absolute) | 0.00386∗ | |
| WA 2 | NH (1022cm-2) | 2.75 ± 0.29 |
| log ξ (erg cm s-1) |
|
|
| f cvr |
|
|
| z (absolute) | 0.00386∗ | |
| WA 3 | NH (1022cm-2) |
|
| log ξ (erg cm s-1) |
|
|
| f cvr | 1∗ | |
| z (absolute) | –0.00302∗ | |
| CA | NH,Gal (1022cm-2) | 0.0199 |
Notes. Fixed parameters are marked with an asterisk. We assume that the incident hard X-ray power law (HXPL) of the ionized reflection and the continuum power law are identical. To reduce model degeneracies, we freeze the photon index to the value found by Markowitz et al. (2009), who find WA3 to be outflowing. We therefore also freeze the absolute redshift of WA3 to the according value in our model. The soft excess is modeled by a power law (SXPL).
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.