Dark Matter Halos: The Dynamical Basis of Effective Empirical Models

Table 2

Parameters of empirical models in the anisotropic case.

𝛼	1.25	1.27	1.29
Einasto model (1)
𝜂	0.259	0.226	0.194
SE model (1)
𝜏	0.630	0.642	0.654
𝜂	0.368	0.326	0.285
gNFW model (2)
𝜏	0.630	0.642	0.654
𝜂	0.808	0.688	0.578
𝜉	3.396	4.018	4.812