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Fig. 6

image

Spectral energy distribution (solid line) obtained with X-Shooter (red) and XRT data (black), corrected for the rest-frame AV and NH respectively. We also included the radio detection (green) of Laskar et al. (2014). The dashed blue line represents the extinction uncorrected best-fit. Dashed lines indicate the position of the injection frequency (νi = 2 × 1012 Hz) and the cooling frequency (νc ~ 2 × 1016 Hz) expected for a pure synchrotron model.

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