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Fig. 7.

image

True redshift distribution of the mock galaxies, separated into photometric redshift bins. The zB selection is shown in the legend. The cyan histogram shows the true redshift distribution of the galaxies in the parent noise-free sample. In order to determine the photometric redshifts we introduce flux errors that mimic a KiDS-like survey and depend on the relative ellipticity of the mock galaxy to the mock PSF.

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