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Fig. 12


Distribution of the difference between photometric redshifts and VUDS spectroscopic redshifts for flags 3 and 4 (top panels) and flags 2 and 9 (bottom panels) for redshifts z < 1.5 (left panels) and redshifts z > 2 (right panels). The number of galaxies is indicated in each panel together with the σ of the distribution and the fraction of galaxies satisfying δz = (zspeczphot)/(1 + zspec) ≤ 0.1. The distribution peaked at 0 is for the main sample, while a secondary peak appearing beyond δz = 0.5 is produced by the degeneracy between the D4000 and the 1215 Å continuum breaks (see text).

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