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Fig. 9.


Comparison of lensfit-weighted normalised distributions of galaxy properties between KV-450 data (black), KiDS observations of COSMOS (blue), COllege simulations (green) and COllege simulations after re-weighting (orange) the simulated galaxies to match the joint distribution of signal-to-noise ratio and size in the KV-450 data sets (cf. Sect. 6). No redshift cuts are applied here, but similar level of agreement can be seen for each tomographic bin individually.

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