Fig. 17

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Galaxy redshift distributions (N(z)) in the CLAUDS-HSC regions for three selections, as indicated in the top of each panel. The three panels in the top row show the results based on estimates with all the bands and are thus limited to E-COSMOS and XMM-LSS fields. The two panels in the bottom row show those computed with Ugrizy photometry for the four deep fields. For HPH, the N(z) is either based on the redshift point estimates (median of each PDZ; light red lines) or based on the stack of the individual PDZs (dark red line). For SLP, the N(z) is obtained with the redshift point estimate (blue lines). A comparison is made with COSMOS2020 Farmer/EAzY photo-zs (black lines) in the top panels. The COSMOS2020 curves are weighted to match the CLAUDS-HSC ones. The distributions are constructed in bins of δz = 0.05.
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