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Fig. A.1.

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Distributions of L1.4 (top), LIR (middle), and galaxy ℳ* (bottom) of our sample, as a function of redshift. Grey empty circles are VLA sources with an optical-NIR counterpart (Laigle et al. 2016) within the UltraVISTA 1.5 deg2 area, while red crosses mark the subset classified as ‘star-forming’ based on NUVrJ criteria. Dotted lines in the bottom panel enclose the ℳ*z space of the final sample (5,658 sources).

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