Figure 5
From: AEDGE: Atomic Experiment for Dark Matter and Gravity Exploration in Space
The SNR (upper left panel), the sky localization uncertainty ΔΩ (upper middle panel), the polarization uncertainty Δψ (upper right panel), and the uncertainties in the luminosity distance \(D_{L}\) (lower left panel), the time remaining before merger \(t_{c}\) (lower middle panel) and the chirp mass \(M_{\mathrm{chirp}}\) (lower right panel), calculated for three merging binaries of different BH mass combinations as functions of their redshifts