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Fig. 7.
68% and 95% contours of the posterior distribution of {⟨byPe⟩, ⟨bg⟩, ⟨cgy⟩, ⟨cgκ⟩} in the third redshift bin with the halo model non-linear template in the third redshift bin. The contours and 1D posteriors have been smoothed for the purpose of presentation.
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