Fig. 7.
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Posterior distribution of the radio light curves at νobs = 3 GHz for the “SSC (with KN)” fit of the afterglow of GW 170817. The solid lines represent the median value at each observing time, the dark contours are the 68% confidence interval, and the light contours show the 97.5% confidence interval. Late-time observations that were not used in the fit are shown in blue.
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