![]() ![]() We discuss this in some detail, and we investigate the possible sources of systematics which can explain the tension. In the case of Abell S1063 a >2σ tension with the GR expectation arises. Range $0.13 < z_c < 0.45$ and caustic mass range $0.4-1.5$ $10^$ at 2σ, provides about a 2-fold improvement on previous constraints. ![]() Test by dynamically analyzing seven galaxy clusters, spanning the redshift Halo-to-main-cluster mass ratios to cluster-sized halo growth. We provide a new observational test for a key prediction of the \Lambda CDMĬosmological model: the contributions of mergers with different ![]()
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