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Fig. A.1.

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Flux distribution in log10 of sGRB afterglows associated with BHNS mergers detected in GWs with a 3G detector network that includes ET. The distributions are shown for different average BH spins: χBH = 0 (purple), 0.2 (red), 0.4 (green), 0.6 (orange), and 0.8 (blue). The vertical dashed line shows the SKA1-Mid 5σrms detection limit.

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