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Fig. 7.

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(S/N)WL of the clusters and groups detected by AMICO in the XXL-North field of HSC-SSP. Top: (S/N)WL as a function of redshift and richness. The (S/N)WL is computed as the median value for the candidate groups in the bin, and (S/N)WL is colour-coded as shown in the right bar. The number of candidates is superimposed in each bin. Bottom: Same as in the top panel for (S/N)WL as a function of redshift and (S/N)det. In other words, this panel shows the S/N of the optical detection of the algorithm.

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