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Fig. 3.

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Photometric redshift errors in the KiDS-Bright sample as a function of photo-z (left) and of the KiDS r-band AUTO magnitude (right), calibrated on overlapping GAMA data. Each dot is a galaxy, with contours overplotted in the highest number density areas. The thick red line is the running median and the thin red lines illustrate the scatter (SMAD) around the median. The stripes in the left panel originate from the large-scale structures present in the GAMA fields.

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