Table 5
C-statistic values for fitting the O VII triplet, and the whole RGS spectrum, with WA absorption of narrow emission lines (and RRCs when looking at the whole data range).
| C-stat value for | C-stat value for | |
| Absorption applieda | O VII tripletb | all RGS datac |
|
|
||
| None | 104 | 1865 |
| A | 103 | 1864 |
| B | 93 | 1856 |
| C | 102 | 1861 |
| D | 114 | 1882 |
| E | 94 | 1879 |
| F | 100 | 1863 |
|
|
||
| B and E | 83 | 1870 |
| B, E and D | 85 | 1878 |
| B, E and F | 78 | 1871 |
| A, B and C | 90 | 1853 |
| A, B, C and D | 96 | 1864 |
| A, B, C, D and E | 80 | 1866 |
| A, B, C, D, E and F | 78 | 1868 |
Notes. The parameters of all the WA components were fixed to the best-fit values from Kaastra et al. (2014), as they are for all the analysis within this work. For each of these fits, all three O VII triplet lines had fixed outflow velocities of −300 km s-1 and the widths of all three triplet lines were coupled and fitted together. ;
Letters refer to Kaastra et al. (2014) WA components;
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