KiDS-1000 cosmic shear power spectra: tomographic band powers comparing the E-modes (upper left block) with the best-fit cosmological model from our combined multi-probe analysis. The tomographic bin combination is indicated in the upper right corner of each sub-panel. The null-test B-modes (lower right block – note the reduced ordinate scale), are consistent with zero for both the full data vector and each bin combination individually. The errors are estimated analytically (Joachimi et al. 2021). See Sect. 3 for a discussion on the goodness-of-fit.