Fig. 5.
Spectral energy distributions (SED) for 8 observations between MJD 56009 and MJD 57046. The markers match the following experiments; the green open triangle OVRO (radio 15 GHz), blue open square Metsähovi (radio 37 GHz), red open circle (R-band optical, corrected for host galaxy), blue open triangles Swift/UVOT (UV), black filled circles Swift/XRT (X–ray), pink open triangles Swift/BAT (X–ray), blue open circles Fermi-LAT (gamma rays) and red/green filled squares/triangles MAGIC/VERITAS (VHE gamma rays). VHE data are EBL–corrected using Franceschini et al. (2008). The BAT energy flux relates to a one-day average, while the Fermi-LAT energy flux relates to three-day average centered at the VHE observation. Filled markers are those fit by the theoretical model, while open markers are not. The black line represents the best fit with a one–zone SSC model, with the results of the fit reported in Table 2.
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