Fig. 7
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Same spectrum and color scheme as in Fig. 5. Left panel: Best fit result with a recombining plasma emission model (RNEI in XSPEC) for the Galactic corona (solid green) in addition to the components considered in the bottom left panel of Fig. 5 (shiſt-LHB-CGM-Coro2-CXB in Table 2). Right panel: Same as left panel, but with the addition of the SWCX component (shiſt-LHB-CGM-CXB-Coro2-SWCX model).
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