Fig. 10.
Photometric redshift distributions of PAUS W3 galaxies, split into (LEPHARE) red/blue samples (shaded histograms), along with the n(z) for red/blue clones in the windowed randoms (solid lines) and the unwindowed randoms (dashed lines). Randoms shown here are the ‘zph-randoms’ described in Sect. 3.3. Each histogram/curve is individually normalised to unit area.
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