Dark Energy Survey Deep Field photometric redshift performance and training incompleteness assessment

Open Access

Fig. 5.

Precision of the photo-z defined by MAD(Δz) (upper panel) and the $σ_{68}^{Norm}$ $\sigma_{68}^{\mathrm{Norm}}$ (bottom panel) as a function of the mag(i) for the complete training sample (blue lines) and incomplete training sample (magenta lines). The solid lines display the metrics calculated with z_spec and the dashed lines were calculated by replacing z_spec with DNF_ZN.

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