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Fig. 14


Evolution of the number density of the blue and red galaxy populations in VIPERS (filled circles and diamonds, respectively) with different stellar masses. Upward arrows represent lower limits when ρN is estimated in a bin of mass affected by incompleteness, while a downward arrow represents the upper limit in case of zero detection (rightmost panel). The error corridors reflect the overall uncertainties, which include both Poisson noise and cosmic variance added in quadrature.

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