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Fig. C.1.

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1.4 GHz radio luminosity function of SFGs (top row) and radio-excess AGNs (bottom row) in each field (green circles: GOODS-N; blue triangles: COSMOS/UltraVISTA). The black solid curves in the top row represent the best-fit model (PLE) for SFGs. The black solid curves in the bottom row represent the best-fit model (PDE) for radio-excess AGNs.

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