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Fig. B.1.

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SEDs computed from scenario 0, for typical cases of low ( = 0.1 M/yr, left) and high ( = 10 M/yr, right) SFRs. The coloured lines (solid for the primary CRs and dashed for the secondary CRs) are the individual contributions of different non-thermal radiative mechanisms (the colour-coding is the same as in Fig. 2). The dashed brown line is the thermal free-free emission; the grey shaded region represents the Fermi-LAT energy range; and the vertical dotted black lines show the studied radio frequencies (150 MHz and 1.4 GHz).

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