Table A.4.
Spectral fitting parameters of the ten time windows of the XMM-Newton observation, using tbabs×zashift×(bbody+diskbb), with their 90% confidence intervals.
| Time window | kTDiskbb(eV) | NormDiskbb | kTBbody | NormBbody | L0.2-2 keV | Radius |
|---|---|---|---|---|---|---|
| (eV) | ((Rin/D10)2) | (eV) |
 |
(×1042 erg s−1) | (×106 km) | |
| 0 (1-4 combined) |
 |
 |
N/A | N/A | N/A | N/A |
| 1 |
 |
 |
||||
| 2 | " | " | ||||
| 3 | " | " | ||||
| 4 | " | " | ||||
| 5 | " | " | 45.1 |
17.1 |
26.4 |
8.5 |
| 6 | " | " | 68.0 |
13.8 |
24.3 |
3.1 |
| 7 | " | " | 86.3 |
25.3 |
46.1 |
2.6 |
| 8 | " | " | 107.1 |
37.8 |
70.1 |
2.1 |
| 9 | " | " | 113.5 |
57.7 |
107.1 |
2.3 |
| 10 | " | " | 114.2 |
63.3 |
117.5 |
2.3 |
Notes. The Time window 0 results from the merging of the time windows 1-4, and corresponds to the quiescent state; we removed the bbody parameter from this specific time window only, to better estimate the quiescent diskbb. For the other time windows, the diskbb parameters are tiedn but the bbody is independent. The luminosity is for the bbody only, and it is extrapolated to the 0.2-2 keV band from the fitted data in the 0.3-0.9 keV band. It was not computed in the first four time windows, where the bbody was not constrained. The radius is computed by replacing bbody with bbodyrad, which allows us to retrieve the emitting area from the normalisation factor. The spectral fitting of the time windows 1–10 yields a fit statistic of CStat = 339.4 with 339 degrees of freedom. The combined quiescent state fit resulted in a fit statistic of CStat = 32.7 with 33 degrees of freedom.
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.