Combined X-ray and optical analysis to probe the origin of the plateau emission in γ-ray burst afterglows

Open Access

Fig. 8.

Comparison between the isotropic equivalent energy E_iso and the X-ray luminosity at 24 h after the trigger. The blue solid line and the yellow band represent the best fit and 3σ dispersion, respectively, of the same relation reported by D’Avanzo et al. (2012) for a complete sample of GRBs observed by Swift.

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