Fig. 1.
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Footprint of the HSC-Y3 weak lensing dataset (grey dots) and the sky distributions of the eRASS1 clusters together with those categorized based on the availability of weak-lensing shear profile g+ and/or the BCG stellar mass estimate M⋆, BCG. The eRASS1 clusters with available g+ are marked as blue circles (23 clusters), those with M⋆, BCG as green diamonds (28 clusters), and those with both measurements as red squares (73 clusters). The other eRASS1 clusters with neither g+ nor M⋆, BCG are shown as grey crosses, and are excluded from this study.
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