Fig. 8.
Constraints of ⟨bg⟩ and ⟨byPe⟩ in each tomographic bin. The best-fitting parameter values and errors are calculated as the modes and standard deviations of the Gaussian KDE fittings of marginalised posterior distributions. Dots with different colours are correspond to the different non-linear power spectrum models. The grey line shows the best-fit model from Chiang et al. (2020).
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