The cosmological analysis of X-ray cluster surveys - V. The potential of cluster counts in the 1 < z < 2 range

Open Access

Fig. 12.

Impact of the z > 1 clusters in survey B on f_NL, Ω_m, and σ₈ for local primordial non-Gaussianities (cluster counts only). The outer and fainter ellipse corresponds to the analysis restricted to the 0.05 < z < 1 range, and the successive inner and darker ellipses extend the analysis out to z = 2.

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.