Figure 5
The KS-probability that the cumulative -distribution (solid lines) and -distribution (dashed lines) obtained from the SDSS groups is consistent with that obtained from our mocks, as a function of bvel. Results are shown for four log halo mass intervals, indicated in square brackets in each panel. The horizontal dotted line in each panel indicates PKS = 0.01: based on estimates of the scatter due to cosmic variance, we consider two distributions to be statistically equivalent when PKS > 0.01.

The KS-probability that the cumulative formula-distribution (solid lines) and formula-distribution (dashed lines) obtained from the SDSS groups is consistent with that obtained from our mocks, as a function of bvel. Results are shown for four log halo mass intervals, indicated in square brackets in each panel. The horizontal dotted line in each panel indicates PKS = 0.01: based on estimates of the scatter due to cosmic variance, we consider two distributions to be statistically equivalent when PKS > 0.01.

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