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Fig. 1

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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.

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