Fig. 3.
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Average scatter of the photometric redshifts in bins of photometric redshift, derived from the comparison to spectroscopic redshifts (dashed lines) or from the mean width of 15th-to-85th percentiles around the median of the individual PDZ (solid lines) for the same subset of galaxies. The lines stop when fewer than 200 galaxies are available in the considered redshift bin.
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