Fig. 1.
Spherically averaged radial velocity profiles of two dark matter halos, one from TDSS (left panel) with M200 = 2.15 × 1015 M⊙, and one from TNG-300-3 (right panel) with M200 = 6.63 × 1014 M⊙. Error bars indicate the ⟨Vr⟩ uncertainty (standard error of the mean) in each shell. In both panels, the red vertical line indicates the turnaround radius.
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