Table 2
Best-fit parameters and confidence intervals for the relativistic reflection model applied to the full observations, including both eROSITA and XMM-Newton data.
| Parameter | Value and confidence |
|---|---|
| spina |  |
| θ [°] |  |
| Γ |  |
| h [rg] |  |
 |
 |
 |
 |
 |
 |
| logξe |  |
| CMOS2 | 1.14 ± 0.07 |
| CeROSITA |  |
| C-statistic/d.o.f. | 353.3∕291 |
Notes. This is not our final model. (a)Dimensionless spin parameter cJ∕GM2 where M is the black hole mass and J is the angular momentum. (b) See Dauser et al. (2016). (c) Reflection fraction, see Dauser et al. (2014). (d) Iron abundance with respect to solar values (Grevesse et al. 1996). (e)Ionisation parameter, defined as ξ = 4πF∕n where F is the incident flux and where n is the particle density.
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.