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Fig. 5.

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Rest-frame spectral luminosities at different redshifts for galaxies that are observed face-on. Different colors indicate results from models with different stellar masses: M = 109M (blue), M = 1010M (green), and M = 1011M (red). Different linestyles refer to different emission types: the total radio emission Lν (solid lines) depends on the free-free luminosity (dotted lines) and the unabsorbed synchrotron emission (dashed lines). The grey vertical line represents νobs = 1.4 GHz and the grey region indicates the range for redshifting between z = 0 − 4 (i.e., from left to right).

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