Investigating the impact of galaxies’ compact binary hosting probability for gravitational wave cosmology

Open Access

Fig. 6.

Posterior obtained by fixing H₀ to 70 km s⁻¹ Mpc⁻¹ and ${\hat{d}}_{L}^{thr} = 1550$ $\hat{d}_L^\mathrm{{thr}} = 1550$ Mpc for 200 detected GWs, for the same LOS and a sky area of 10 deg².

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