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Following the procedure described in Pol et al., we update the Galacticdouble neutron star (DNS) merger rate by including the new, highly eccentricDNS system J0509+3801 (Lynch et al.). This leads to a new Galactic DNS mergerrate of $\mathcal{R}_{\rm MW} = 37^{+24}_{-11}$ Myr$^{-1}$, where the errorsrepresent 90% confidence intervals. The corresponding DNS merger detection ratefor Advanced LIGO is $\mathcal{R} = 1.9^{+1.2}_{-0.6} \times \left( D_{\rm r} /100 \ \rm Mpc \right)^3 \rm yr^{-1},$ where $D_{\rm r}$ is the range distance.Using the LIGO O3 range distance of 130 Mpc (Abbott et al.), we predict thatLIGO will detect anywhere between three and seven DNS mergers per year ofobserving at O3 sensitivity.

An Updated Galactic Double Neutron Star Merger Rate Based on Radio Pulsar Populations