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Fig. 10.

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Marginalised constraints for the joint distributions of Ωm, σ8, and S8 from KiDS-Legacy cosmic shear data (black), its combination with Pantheon+ SN Ia data and DESI Y1 BAO data (blue), and its combination with Pantheon+ SN Ia data and eBOSS DR16 BAO and RSD data (orange). These results can be compared to CMB constraints (green) inferred with the compressed Planck likelihood by Prince & Dunkley (2019). The inner and outer contours of the marginalised posteriors correspond to the 68% and 95% credible intervals, respectively.

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