Fig. 2.
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Evolution of the average misalignment angles θa (upper panels) and θc (lower panels) of the stellar and dark matter major and minor axes respectively, as a function of total mass. Left panels show the evolution of the alignments of BGGs that are classified as red at z = 0, i.e (g − r)z = 0 > 0.6, while the right panels show the evolution of blue BGGs i.e (g − r)z = 0 < 0.6.
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