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Fig. 1.
Redshift distribution p(z) of galaxies with mr < 20.25 in the 64 MS light cones, compared to the estimated redshift distribution of KiDS galaxies with mr < 20.30 (Bilicki et al. 2018, in the plot B18). Shown in green is the weighted source redshift PDF of the highest three tomographic bins; from Hildebrandt et al. (2020).
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