Fig. 15.

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Left: spectrum (folded with the instrument spectral response) of the emission in the west jet region (including the AGN contamination and the residual thermal emission from the ICM) fitted with a power law. Right: unfolded spectrum with the three components in the model shown with dotted lines. The lowest dotted line corresponds to the thermal emission from the overlapping ICM, while the line in the middle accounts for the AGN wings contamination. The IC from the relativistic population in the west jet is shown by the unabsorbed power law that is dominating at any energy.
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