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Fig. 13.

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Number of GW and KN detections in the M1M2 space. The colorbar indicates the number of GW detections with sky localisation Ω90<5 deg2 (left) and the number of corresponding KN detections for the 1ep detection strategy (right) obtained assuming APR4 (top) and BLh (bottom) EOSs, Gaussian NS mass distribution, α = 1.0, and GW network ET-Δ+2 CE. The black dot shows the peak of the Gaussian mass distribution, that is M1=M2 = 1.33 M.

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