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Fig. 3.

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Light curves for GRB 160131A of visible and X-ray data modelled with DBPL (Eq. (4)). We observe the plateau, probably ascribable to the energy injection between ∼104 and ∼7 × 104 s (∼0.1 and 0.8 d), and the achromatic break at ∼9 × 104 s (∼1 d), typical of jetted emission. Bottom panel: residuals of the fit.

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