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Fig. 9

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Residuals of the SN 1993J flux densities between days 1000 and 3000 after explosion, using the model of Weiler et al. (2007): a) all the residuals (1.4 GHz residuals have been joined with a solid line for clarity); b) zoomed, the residuals at 5 and 8.4 GHz (the solid line now marks the zero mJy level).

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