Fig. 4.
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Cooling time for relativistic electrons underoging synchrotron and inverse compton losses (as in Eq. (2)), as function of their Lorentz factor and cosmic redshift, for two B = 0.1 μG and B = 10 μG. The solid black lines mark the region corresponding to our choice of the timescale τ for the age determination of CRe injected at run-time.
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