Fig. 2
Our best fit to the X-ray (solid line) and R-band optical (dashed line) afterglow light curves of GRB 051016B by using the ring-shaped jet model. The square data points are observed X-ray afterglow by Swift-XRT (see the Swift website) and the triangle data points are observed R-band afterglow (Chen et al. 2005; Sharapov et al. 2005).
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