Top: normalised redshift distributions n(z), measured from the EFS, for the 13 equi-populated bins that were used for the 3×2pt analysis for the SPV. Middle: resulting photometric magnification kernels for the 13 redshift bins shown above. Bottom: corresponding shear kernels before (dashed) and after (solid lines) BNT transformation. The latter case gives a better grasp of the tomographic information that can be inferred from WL observations.