HSC Wide S16A cluster catalog

The HSC images are sufficiently deep to detect cluster member galaxies down to M*~10^10.2^M_{sun}_ even at z~1, allowing a reliable cluster detection at such high redshifts. We apply the CAMIRA algorithm to the HSC Wide S16A dataset covering ~232deg^2^ to construct a catalog of 1921 clusters at redshift 0.1<z<1.1 and richness N_mem_>15 that roughly corresponds to M_200m_>~10^14^h^-1^M_{sun}_.

We confirm good cluster photometric redshift performance, with the bias and the scatter in {DELTA}z/(1+z) being better than 0.005 and 0.01, respectively, over most of the redshift range. We compare our cluster catalog with large X-ray cluster catalogs from the XXL and XMM-LSS (the XMM Large Scale Structure) surveys and find good correlation between richness and X-ray properties.We also study the mis-centering effect from the distribution of offsets between optical and X-ray cluster centers.