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Fig. 3


Probability distribution function of redshift errors at 0.5 <z < 0.7 and 0.7 <z < 1.2 in the VIPERS data. This is obtained from the redshift differences of reobserved galaxies, for which there are two independent redshift measurements. The dotted and dashed curves are best-fitting Gaussians for the redshift intervals 0.5 <z < 0.7 and 0.7 <z < 1.2 respectively.

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