Fig. 13.
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Top panel: Multi-dimensional grids of emission models of plasma in collisionally ionisation equilibrium for the combined RGS (0.4–2 keV) and EPIC (2–10 keV) spectra. Middle and bottom panels: Grids of models of photoionised plasma in emission and absorption, respectively. Both scans adopted a line broadening of 100 km s−1 and solar abundances. The best-fit CIE model is also shown in Fig. 11.
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