Fig. 7
Evolution of the rest-frame (NUV − r′) vs. (r′ − K) plane for VIPERS. A selection along the lines of of constant sSFRs (black ⟨sSFR⟩ arrow) and dust-extinction (grey SMC arrow) gives a clean separation for the majority of passive (red) and star-forming active (dusty red and blue) galaxies. The fraction of galaxies (in per cent) classified as passive and active is given in each panel.
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