Fig. 4
Best fit of the UVOT white-band data (black triangles, taken from De Pasquale et al. 2010, their Fig. 1) for two models that require a second break in the UVOT light curve at 22 ks (see Sect. 3.3). Also shown are the X-ray data, shifted in flux density by a factor of 104. The two vertical lines highlight the time interval in which GROND was observing.
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