Fig. 8.
Radio luminosity of the afterglow of GRB 111005A (circles), compared with cosmological GRBs (region marked by black lines; Chandra & Frail 2012), GRB 980425 (small stars; Kulkarni et al. 1998), GRB 031203 (small squares; Soderberg et al. 2004), GRB 060218 (small triangles; Soderberg et al. 2006), and GRB 100316D (small diamonds; Margutti et al. 2013). Datapoints are colour-coded by frequency.
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