Fig. 9.

Constraints of ⟨bg⟩ and ⟨byPe⟩ for different non-linear matter power spectrum models with different scale cuts kcut. We also plot the fitting of ⟨bg⟩ and ⟨byPe⟩ with a pure linear model in purple (i.e. ⟨cgκ⟩ and ⟨cgy⟩ are both fixed to be zero). We note that for low redshifts and low kcut, we do not have enough degrees-of-freedom so ⟨bg⟩ and ⟨byPe⟩ are not presented. In addition, for high redshift bins, large-scale cuts are beyond the high limit of ℓ, so with these kcut values, the constraints do not change.
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