Fig. 8.
Left: Y-band magnitude vs the Kullback–Leibler divergence, DKL. The PDF of brighter sources carries more information content, i.e. narrower PDF, compared to faint sources. Right: Δz = zphot − zspec as a function of information content split per galaxy class. QSO PDFs have the distinctly lower information content compare to normal galaxies and AGN.
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