Fig. 12

Satellite fraction of colour selected blue and red galaxies in VIEPRS-like mocks. The halo occupation distribution (HOD) model used to build the mock catalogues identifies galaxies as either satellite or central. Plotted are the fraction of satellite galaxies fsat in the flux- (empty markers) and volume-limited (filled markers) VIPERS-like mock samples for red (top panel) and blue (bottom panel) galaxies. In both panels fsat is measured in redshift bins of width Δz = 0.1 between 0.6 ≤ z ≤ 1.0.
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