Comparisons between all models considered for the HS6 fiducial cosmology for angular power spectra of WL (top left), galaxy clustering (top right) and their cross-correlation (bottom right) as well as for the matter power spectrum (bottom left). We show these for the WL redshift bin 6 and galaxy clustering bin 2, with the matter power spectrum plotted at z = 0.5, the redshift at which the kernels of both observables peak for the chosen bins. For all angular spectra, the error bands taken from the diagonal of the covariance are also shown.