Free Access

Fig. 1


Assumed redshift distribution of galaxies and redshift binning for the fiducial lensing survey. Shadowed areas highlight the sample selections in the distribution of redshift estimates, and the black lines show the true redshift distribution within the samples after including the effect of a redshift uncertainty of σz = 0.05(1 + z). As additional survey parameters, we have (sources) and (lenses), an effective survey area of 200   deg2, and a shape noise variance σϵ = 0.3. All galaxies are unbiased with respect to the dark matter density field.

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.