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Fig. 3

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Histograms for sources detected in g, but not detected in Ks for template sample with models. (a) Histogram showing the dN/d log SX distribution of the template sample of X-ray sources that are detected in HSC g-band, but not in CFHT Ks (depth matched with AKARI NEP Deep Field; See text), constructed from the COSMOS Legacy survey. The curve shows the best-fit model. (b, c) Histograms of log SX + 0.4 g distribution of the template sample and the best-fit model.

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