Fig. A.1
We report, as an example, the spectrum of 3C 171, 3C 305, 3C 433 and 3C 445 in the extended regions fitted with three different models: powerlaw, Mekal, and Xstar, absorbed by a Galactic column density value. We add to the model an intrinsically absorbed powerlaw, to reproduce the emission seen at higher energies (due to the leaking of the nuclear emission).
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