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Fig. 3.

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Top:zmean photometric redshift distributions obtained with DNF for the six photometric samples up to mVIS = 25. The zmean photo-z estimate returned by DNF is the value resulting from the mean of the nearest neighbors redshifts. Lower: photometric redshift distributions obtained with DNF for the zmc statistic, which for each galaxy is a one-point sampling of the redshift probability distribution estimated from the nearest neighbor (see text for details). All samples have the same number density of 41.5 galaxies per arcmin2.

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