Fig. 13.

image

Robust scatter (σNMAD; upper panels) and outlier fraction (OLF; lower panels) for the consensus photo-z estimate (z1, median) as a function of spectroscopic redshift and apparent iPS1 magnitude. For the AGN subset (left panels) each cell corresponds to a minimum of 30 sources with the colour of the cell representing the scatter of that subset. For the galaxy plots (right panels) each cell corresponds to a minimum of 100 sources. The top and side bar of each panel shows the trends in σNMAD or OLF averaged over all magnitudes and redshifts respectively. For reference, we also plot the distribution of the spectroscopic training sample within this parameter space as grey contours – plotted contours are linearly spaced in source density.

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