Similar to Fig. 7, but zoomed into the optical and NIR regime (the full plot is displayed in Fig. C.1). In the left inset we show the SEDs for the 10 GRBs that show evidence for a medium amount of dust (AV> 0.1 mag) fitted with the SN extinction curve. For comparison, in the right inset we show again the best result when performing the fit with local extinction curves. The goodness of fit is comparable in both scenarios (see Table 2 and Sect. 4).
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