Fig. B.1

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The black data show the e12 spectrum fitted with the best fit model shift-LHB-CGM-Coro2-CXB (same spectrum and color scheme as in Fig. 5). The red data show the e12 spectrum obtained after filtering the events with the FLAREGTI tool. The two spectra are consistent with each other. Notable background flares are not detected during the observation of the eFEDS region during e1 and e2.
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