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Fig. 3.

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Left: spectral energy distribution of the emission produced by electrons injected in the ISM (in red) and JET regions (in blue). A magnetic field BISM = 5 μG is assumed for the ISM, whereas a range in the value of BJET = 5, 10, 15, 20 and 30 μG is probed for the JET region. Particle injection is considered up to tinj = 103 yr for the JET region and from tinj = 103 yr until tinj = 20 kyr for the ISM region (red-dotted lines). Particles are assumed to follow a power-law distribution with a low and a high energy cutoff and , respectively. Green and orange vertical bands denote Chandra and MeerKAT frequency coverage. Right: same as in the left panel but for a particle spectrum with a low-energy cutoff .

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