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Fig. 3.


Left: differential distribution of distances (normalized to the sky-position-averaged horizon) of events in total GW population (full line), and detectable jointly in O2-VLA (dotted line) and O3-VLA (dashed line) configurations. Right: cumulative distribution of same events. Distributions have been normalized to the fraction of jointly detected events among all GW-detected events, see text for details.

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