Fig. 13


Angular two-point correlation function of the bright XXL cluster sample. The different levels of correlation come from different estimators. The scatter between these estimators is well within the Poisson uncertainties, shown by the vertical error bars. The dashed line shows the expected correlation in the WMAP9 cosmology with the set of scaling relations obtained in Paper III and Paper IV.

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.