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Fig. 4

image

Spectral energy distribution of PKS 1510089 constructed from the MAGIC data gathered on MJD 57 160 and 57 161 (Period A). The observed spectrum is shown by red empty squares with inclined hashing, and the EBL-deabsorbed spectrum according to the Domínguez et al. (2011) model by magenta filled circles with vertical hashing. The hashing shows the uncertainty of the forward folding with a power law. The SED constructed from the data taken on MJD between 57 164 and 57 166 (Period B) is shown as empty (observed) and filled (EBL-deabsorbed) blue circles. For comparison, MAGIC measurements performed in Feb.Mar. 2012 and H.E.S.S. measurements from Mar. 2009 (Abramowski et al. 2013) are shown as gray diamonds and stars, respectively.

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