Constraints on the merging binary neutron star mass distribution and equation of state based on the incidence of jets in the population

Open Access

Fig. A.2.

f_j, GW inference with multiple GW-detected BNS mergers. The coloured bands show the evolution of the posterior 90% and 50% credible range on f_j, GW after N_events simulated GW detections (see text), while the red solid line shows the median of the posterior. The horizontal black dashed line shows the true value.

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