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Fig. 11
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Same as Fig. 10 but for all the HSC-CLAUDS fields combined and split by i-band magnitudes. The comparison is extended to faint magnitude bins, as indicated in each panel, with faint spectroscopic sources coming from the DEEP-23 (mi ≤ 24), XMM-LSS, and E-COSMOS (mi ≤ 26) fields.
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