Free Access

Fig. 1.


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.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.