Comparing next-generation detector configurations for high-redshift gravitational wave sources with neural posterior estimation

Open Access

Fig. 5.

Cumulative distributions of events as a function of the optimal S/N (ρ; Eq. (D.4)), the relative variations in detector-frame chirp mass ( $Δ M_{d} / M_{d}^{inj}$ $Mathematical equation: $ \Delta \mathcal{M}_{\mathrm{d}}/\mathcal{M}^{\mathrm{inj}}_{\mathrm{d}} $$ ), mass ratio (q), first (Δχ₁) and second (Δχ₂) aligned spins, and inclination angle (Δθ_jn) for all considered XG detector configurations. See Sect. 3.3 for details.

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