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Fig. 3.


KiDS-1000 galaxy-galaxy lensing power spectra: tomographic band powers comparing the E-modes (left block) with the best-fit cosmological model from our combined multi-probe analysis. The tomographic bin combination of BOSS and 2dFLenS lenses (L) with KiDS-1000 sources (S), is indicated in the upper right corner of each sub-panel. Data within grey regions are not included in the cosmological analysis. The null-test B-modes (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).

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