Fig. D.1
Rest frame 1–10 000 keV light curve for GRB 130603B. The red data are Swift observations, with the first 2 data points being from the BAT observations and the remainder are XRT observations. The blue data are the XMM observations obtained by Fong et al. (2014). The Swift XRT data are fitted using the magnetar model, as described in Rowlinson et al. (2013), shown by the black line.
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