Fig. D.1
EPIC pn spectra for the annuli defined in Fig. 1. The various components used for the fit are shown in red for the source; in blue for the NXB; in magenta for the CXB; in cyan for the Galactic halo emission; and in green for the local hot bubble. The fit was performed jointly on all 3 EPIC instruments, but here only the pn is shown for clarity. The results of the fit are listed in Table 3.
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