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Fig. 2


a) Spectra (100 eV bins) of the background expected on X-IFUin all the cases analyzed. The black line is the expected background without an anticoincidence system, the red line is the level expected with an ACD, and the blue line is the final background level. b) Spectra (500 eV bins) expected on X-IFUin L2 and in LEO orbit, in the nominal configuration (dashed lines), and in the reduced configuration (continuous lines).

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