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Fig. 3.

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Simulated spectrum (black crosses), with an exposure of 100 ks, in half of the Resolve FoV with the best-fit bapec model overplotted. The thermal model only is shown with the green line, the instrumental background in blue, and the thermal model plus the instrumental and cosmic background in red. The most prominent lines are the Fe XXV and Fe XXVI complexes in the range 6−7 keV.

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