The universal distribution of halo interlopers in projected phase space - Bias in galaxy cluster concentration and velocity anisotropy?

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Table 3:

Statistics of interloper surface densities $\Sigma _{\rm i}$ (in N_v r_v^-2).
Velocity cut	No	Yes
Arithmetic mean	0.116	0.098
Geometric mean	0.102	0.085
Standard deviation of $\log\hat\Sigma_{\rm i}$	0.216	0.229
Spearman rank correlation	0.025	-0.008
Probability	0.34	0.44

Notes. Spearman rank correlation is between mean surface density of interlopers and halo mass. Probability is of having a stronger correlation by chance.

Source LaTeX | All tables | In the text

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