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Fig. 4.


Marginal multi-probe constraints on the flat ΛCDM cosmological model, for the matter fluctuation amplitude parameter, σ8, the matter density parameter, Ωm, and the dimensionless Hubble parameter, h. The BOSS galaxy clustering constraints (blue), can be compared to the KiDS-1000 cosmic shear constraints (pink), the combined 3 × 2 pt analysis (red), and CMB constraints from Planck Collaboration VI (2020, grey).

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