Fig. E.1.
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Comparison of the COSEBI data vector and the best fit model for spec-z fiducial and the reanalysis of Asgari et al. (2021) with corrected m-bias. The triangular arrangement of all 15 combinations of tomographic bins are labelled with their individual χ2-values. The COSEBIs modes are significantly correlated, therefore their goodness-of-fit cannot be estimated by eye.
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