Predicted 90th percentile of the cumulative MM detection rates for our four population model variations, assuming a jet core half-opening angle θ_j = 3.4° for the jet-related emissions. Different marker shapes indicate different adopted EoSs (triangle: SFHo; circle: DD2). Filled markers are for χ_BH = 0, while empty markers are for a uniform spin parameter distribution between 0 and 0.5. The error bars indicate the uncertainty on the local merger rate. For GRB afterglow and prompt they also take into account a variation on the jet core half-opening angle (θ_j = 15°, corresponding to the minimum and maximum value reported in Table 1). Similarly as in Fig. 2, the left-hand panel assumes an LVK GW-detector network and the O4 projected sensitivities, while the right-hand panel assumes an LVKI network and the O5 sensitivities. EM bands and detection thresholds are the same as in Fig. 2.