Fig. 1.

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Examples of Subaru riz-composite images of the optically selected clusters with overlaid the eROSITA X-ray intensity maps, HSC J084528+032739 (left) and HSC J092557+004122 (right). The red contours are linearly spaced by half of the average height of galaxy density maps over all CAMIRA clusters at the same redshift. The white contours for X-ray emission are ten levels logarithmically spaced from [10 − 1000] cts s−1 deg−2. In each panel, the X-ray centroid and the initial CAMIRA coordinates are marked by the yellow and pink cross, respectively. The green circle denotes the position of the confirmed BCG. The magenta circle indicates R500.
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