Table 4.
Normalization factors (K) of the XSPEC model zgauss used to simulate possible emission lines in XMM-Newton/EPIC-pn and Chandra/ACIS-S X1 and X2 data in Fig. 7.
| Line | El(keV) | XMM-pn | CXO-X1 | CXO-X2 |
|---|---|---|---|---|
| N VI Heα | 0.426 | 8.0 | 1.0 | 0.2 |
| O VII Heα | 0.569 | 8.0 | 1.0 | 0.2 |
| O VIII Lyα | 0.653 | 8.0 | 1.0 | 0.2 |
| Ne Kα | 0.849 | 8.0 | 1.0 | 0.2 |
| Ne X Lyα | 1.021 | 8.0 | 1.0 | 0.2 |
| Mg XII Lyα | 1.471 | 8.0 | 1.0 | 0.2 |
| Al XIII Lyα | 1.727 | 8.0 | 1.0 | 0.2 |
| Si XIII Heα | 1.865 | 8.0 | 1.0 | 0.2 |
| S Kα | 2.308 | 4.0 | 0.5 | 0.1 |
| Ar Kα | 2.958 | 4.0 | 0.5 | 0.1 |
| Ar XVIII Lyα | 3.318 | 4.0 | 0.5 | 0.1 |
| Ca Kα | 3.691 | 4.0 | 0.5 | 0.1 |
| Fe Kα | 6.404 | 4.0 | 0.1 | 0.02 |
Notes. The zgauss components are shifted with vout = −290 km s−1 in the rest frame (z = 0.020598) and have a line width (σ) of 10 eV. The normalization factor unit is in 10−6 photons cm−2 s−1 in the line energy (El).
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