Fig. A.1.
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Top: Mean angular power spectra estimated from our mock catalogues (squares with RMS error bars) for the ℛ (red) and 𝒢 (blue) suites are compared to the corresponding output from the CAMB code (crosses). All spectra were binned using intervals Δℓ = 5. Bottom: Relative difference between the spectra (error bars here indicate the standard error of the mean).
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