Fig. 6.
Frequency distribution of |cos θ|, where θ is the angle between the spin vector and the major (red), intermediate (green), minor (blue) axis of the DM halos, for two distinct halo environments: Upper panel: halos in dense environment (1 < Risol/rvir < 4). Lower panel: extremely isolated halos (30 < Risol/rvir < 70). The shaded splines denote the Poisson uncertainties.
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