Fig. 3
Optical and near-infrared spectral energy distributions of the afterglow (top) taken on October 30, 2007, at 01:50 UT (T0 + 2.0 d) and host galaxy (bottom) of GRB 071028B. Using HyperZ, the data points are best fit by a single power law with a spectral index of 
(see Table 5) and a model of an Sb galaxy with a photometric redshift of 
(see Table 4).
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