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Fig. 6


Left panel: interstellar flux (multiplied by E3.3) of secondary positrons computed with all propagation effects (ΦII, solid lines) and with the high-energy approximation (, dotted lines) for the Min (blue), Med (red), and Max (green) models. Right panel: relative error above 10 GeV of the high-energy approximation for secondary positrons compared to the exact result.

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