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Fig. 5

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Multiwavelength spectral energy distribution fitted with a one zone synchrotron self Compton model (Maraschi & Tavecchio 2003). MAGIC observations (red butterfly), have been corrected for the extragalactic background light absorption using the model of Domínguez et al. (2011). The data used for the fit are: optical from KVA (red square), archival UV and optical from Swift/UVOT and archival X-ray from Swift/XRT (blue triangles), HE γ rays from Fermi-LAT (red triangles, three months centred around the MAGIC observing period) and VHE γ rays from MAGIC. We also show the three year LAT data (light blue triangles) and archival data (grey) from the ASI/ASDC archive (http://tools.asdc.asi.it/).

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