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Fig. 12.

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Updated probabilities distribution of the merger rates after the inclusion of J1208−5936 and the MMGPS-L survey. Top: individual contributions from each DNS population, derived from the values in Table 4 and Eq. (13). The 90% credible intervals are quoted in Table 4. Bottom: galactic merger rate probability distribution from the convolution of individual DNS distributions, with a highlighted 90% credible interval.

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