Comparison of the updated lensfit measurements between KiDS (red) and SKiLLS (blue). All distributions are normalised with lensfit weights, except for the distribution of lensfit weight itself. The neighbour properties are based on the nearest neighbour found in the measured catalogue. The magnitude difference is defined as the neighbour magnitude minus the magnitude of the primary target. The lack of close pairs with distance below ∼1 arcsec is due to the conservative blending cut used by KiDS (see Appendix D). This cut helps to mitigate the worst of the blending bias.