@miki

An optically-selected cluster catalog at redshift 0.1<z<1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data

, , , , , , , , , , , , , , , , , , , , , , , , and . (2017)cite arxiv:1701.00818Comment: 16 pages, 15 figures, cluster catalogs will be made available after the paper is accepted.

Abstract

We present an optically-selected cluster catalog from the Hyper Suprime-Cam (HSC) Subaru Strategic Program. The HSC images are sufficiently deep to detect cluster member galaxies down to $M_*10^10.2M_ødot$ even at $z1$, allowing a reliable cluster detection at such high redshifts. We apply the CAMIRA algorithm to the HSC Wide S16A dataset covering $232$ deg$^2$ to construct a catalog of 1921 clusters at redshift $0.1<z<1.1$ and richness $N_mem>15$ that roughly corresponds to $M_200m\gtrsim 10^14h^-1M_ødot$. We confirm good cluster photometric redshift performance, with the bias and scatter in $\Delta z/(1+z)$ being better than 0.005 and 0.01 over most of the redshift range, respectively. We compare our cluster catalog with large X-ray cluster catalogs from XXL and XMM-LSS surveys and find good correlation between richness and X-ray properties. We also study the miscentering effect from the distribution of offsets between optical and X-ray cluster centers. We confirm the high ($>0.9$) completeness and purity for high mass clusters by analyzing mock galaxy catalogs.

Description

[1701.00818] An optically-selected cluster catalog at redshift 0.1&lt;z&lt;1.1 from the Hyper Suprime-Cam Subaru Strategic Program S16A data

Links and resources

Tags