Fig. 12.

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Probability distributions of bootstrapped realistions of the rms of the projected misalignment angle between the BCG orientation angle and the dark matter halo at various projected apertures for the m9 fiducial run. Only haloes with at least 1000 stellar particles within 30 kpc are considered. The distributions calculated for both VR and HBT-HERONS are shown, with negligible differences. The apertures for which these values are calculated are 30, 50, and 100 kpc, as well as for the total halo.
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