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Fig. E.1.


Marginalised posterior distributions for the extended set of cosmological parameters shown in Fig. 6, comparing the fiducial 3 × 2 pt analysis (red) to a selection of our sensitivity test analyses where we ignore the impact of baryon feedback (the ‘No baryon’ case, sea-green), limit the analysis to a linear galaxy bias model (the ‘No higher order GC’ case, lime-green), and remove individual tomographic bins from our weak lensing observables (orange, purple and pink).

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