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Fig. 7.


Predicted samples of GW-detected (dots) and jointly detected (crosses) mergers in planes of various pairs of observables, for O3-VLA configuration. Upper left: distance and viewing angle, and maximum distance at which the proper motion can be measured (Dmax(θv), see Eq. (18), green dotted line). Upper right: peak flux and viewing angle. Lower left: time of radio afterglow peak (assuming lateral expansion of jet) and viewing angle. Lower right: maximum remnant proper motion and distance, and limiting proper motion μlim (green dotted line).

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