Fig. 12.

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Distribution of GRX GWs emitted in (f, h)-space where MSMBH = 4 × 106 M⊙. Each dot represents an event at a given snapshot emerging from a hard binary. The detectable regions for the Square Kilometer Array (SKA; Smits et al. 2009), μAres (Sesana et al. 2021) and LISA (Amaro-Seoane et al. 2017) are shown on the plot using code developed by Campeti et al. (2021). Calculations assume a luminosity distance of DL = 1 Gpc.
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