Fig. 6.
Redshift distributions of the lens (upper panel) and source (lower panel) galaxy samples. Lens galaxies are split at z = 0.5 into two redshift bins for both the BOSS and 2dFLenS surveys. Modelling is carried out with a weighted combination of their redshift distributions (in green). Lens distributions are constructed for galaxies in the KiDS overlap regions, respectively. Source galaxies are split into five tomographic bins based on their best photometric redshift estimates, as indicated by the shaded bands. The source redshift distributions are KiDS-1000-like and built from KV450 data.
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