Fig. 6
Spectral energy distribution of HESS J1943+213 in γ-rays. The Fermi-LAT error contour (red) has been extrapolated toward the H.E.S.S. energy range (blue points) and corrected for EBL absorption using the model of Franceschini et al. (2008) assuming different values for z from z = 0.01 (green line) to z = 0.7 (red line). The inset gives the corresponding χ2 as a function of the redshift z.
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