Fig. 9.
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Measurements of the re-normalised bias function, F, for haloes of three different mass selections. A reliable scale-independent reconstruction seems generally possible from damping scales up to kd ≲ 0.2 h Mpc−1. The function looks generally better approximated by a Gaussian than a quadratic bias model, especially in regions where the function gets close to zero F ≲ 0.5.
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