Fig. 7.

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Light curves from our highest-likelihood theoretical model shown for each observing band, spanning X-ray, optical, and radio frequencies. Only data points after 0.3 days were used in the modelling, and we show these as filled-in data points, in contrast to the earlier time data points shown as empty circles. Upper limits are shown as upside-down triangles. The shaded regions surrounding the three radio bands (X, C, and L) represent the effects of Galactic scintillation at the 1σ level. The optical g- and r-band model fits plateau towards the measured host-galaxy flux levels at 285 days, shown as diamonds.
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