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Fig. B.1.

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Comparison of the power spectra of Si15 with samples using randomised redshifts. Reasonable variation fits randomise the sample galaxies’ redshifts within one standard deviation, with maximum variation fits including as many or as few galaxies as is plausible. In most cases, the reasonable variation power spectra are nearly indistinguishable from the default power spectra. We do not include other [CII] models for clarity.

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