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Fig. 8.

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Posterior obtained by fixing H0 to 70 km s−1 Mpc−1 and d ̂ L thr = 4250 $ \hat{d}_L^\mathrm{{thr}} = 4250 $ Mpc for 500 detected GWs, for a sky area of 10 deg2 and considering different LOSs when reconstructing the posterior.

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