Fig. 6

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Results of the SED fitting procedure, before optimizing it into our redshift range. The figure shows the photometric redshift as a function of spectroscopic redshift. The internal red dotted lines indicate the limit for which |∆z| = |(zphot − zspec)/(1 + zspec)| > 0.15, which defines the outliers. Red continuos lines indicate the limit for catastrophic outliers |zphot − zspec| > 1. The outlier fraction is 6.06% and the σnmad is 0.0418.
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