Free Access

Fig. 6


Baryonic acoustic oscillations in the power spectrum for the extragalactic sky in the redshift range 0.0 < z < 3.0. At wavenumbers above the vertical dashed line (corresponding to 0.2 h Mpc-1) our assumption of a linear clustering starts to break down. The red curve shows the original input model for the BAOs.

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.