Fig. 7.
Confidence contours (68 and 95%) in (1 − b) vs. AT − M plane, for combination of CMB, SZ and X-ray cluster data in various cosmological models, with or without massive neutrinos, with or without free growth index γ, and free σ8. The black dashed line corresponds to the (1 − b)−AT − M relation leading to the same derived (SZ and X-ray) masses for a selected sample of clusters (see text for details).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.