Fig. 3.
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Distributions of the binary parameters for a sampling of the BH binary population with 0 < z < 3, 1 nHz < f < 30nHz and 
. The symmetric mass ratio is integrated with the lower bound η > 0.001. In the right panel, the black curve shows the NANOGrav 95% CL constraint on continuous GW sources (Arzoumanian et al. 2023) and the projected sensitivity of IPTA30 at SNR = 8.
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