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Fig. B.4.

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Comparison of power spectra demonstrating the impact of VT on extrapolation. In the left subplot we show a cross-section of the LIM cube at 3.42 < z < 3.87 for m1 when using VT to select galaxy location. In the right subplot we see the same, except for the random location selection case. In the lower subplot we compare the power spectra.

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