Fig. 3
Distribution of the variable Δz for the 3813 galaxies in the ALHAMBRA area with i ≤ 22.5 and a measured spectroscopic redshift. The red line is the best least-squares fit of a Gaussian function to the data. The median, dispersion, and the factor C derived from the fit are labelled in the panel. A colour version of this plot is available in the electronic edition.
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