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Fig. 7.

image

Photometric redshift results as a function of the r magnitude and the i − z colour. These results were obtained with a 100-fold cross-validation strategy on the galaxy set with the five magnitudes available (𝒯5). Left panel: average standard deviation of the redshifts of the nearest neighbours σ(zNN), middle panel: rms of the actual error zphot − zspec, and right panel: average estimated errors δzphot. The colour scale and the black contours are set as in Fig. 6.

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