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Fig. 5


Left: GSMFs of photometric early-type galaxies in D1 and D4 environments, renormalised to number density  = 1 for stellar masses  > ℳmin. Right: the same for photometrically late type galaxies. Dotted lines, circles and dark shaded regions represent the GSMFs in underdense regions, D1. Dashed lines, squares and light shaded regions illustrate D4 GSMFs.

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