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Fig. C.1.

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Marginalised one-dimensional posterior distributions of the cosmological parameters h (first column), Ωm (second column) and σ8 (third column) for different combinations of data sets (rows). The first row shows the constraints from the WL data set only, while the following rows show the constraints obtained when subsequently adding the Clustering, Ly-α, and Recomb data sets. In each panel we show a superposition of the constraints from our split analysis of growth and geometry theory regimes (green and grey contours respectively), a traditional analysis with one single set of cosmological parameters (red), and the Planck 2018 (Planck Collaboration VI 2020) constraints for reference (blue).

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