Detection rate as a function of detection limit threshold for our fiducial BHNS population. In the top panel we assume the LVK O4 detectors network (colored lines) and a network consisting of only two aLIGO (gray lines). In the lower panel we assume the LVKI O5 detectors network (colored lines) and the same network without LIGO–India (black lines). Every network is assumed with a 70% duty cycle for each detector. The blue and red colors indicate respectively the kilonova+GW (g band) and the GRB afterglow+GW (radio band) detectable binaries. The solid line indicates all the detectable binaries, the dashed and dotted lines the detectable binaries with ΔΩ_90% < 100 deg² and the ones with ΔΩ_90% < 10 deg², respectively.