Our new KV450 redshift distribution estimates, for the gold sample; a reduced photometric sample of galaxies with 100% representation in the spectroscopic sample, and which satisfies the quality cuts QC1. The figure shows the reconstructed redshift distributions (green) alongside the purely tomographically binned spectroscopic data (purple). The figure is annotated with the mean redshift estimates for the purely tomographically binned sample (⟨z⟩_raw) and the weighted gold sample (⟨z⟩_w, g), the difference that our reweighting has had on the spectroscopic means (Δ⟨z⟩), and the fractional number of galaxies in the gold sample compared to the original KV450 cosmic shear sample .