Fig. H.1.
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1D marginalised posteriors and 2D confidence contours for cosmological parameters and for baryonic feedback parameters, obtained by fitting photometric observables (WL+GCph+XCph) to the w0waCDM+∑mν model, with and without varying baryonic feedback parameters (red-filled and green-empty contours, respectively). The contours for baryonic feedback parameters are also shown when they are varied.
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