Table 3.
Limits of the uniform pyGravSphere-emcee priors on the dark-matter parameters.
| Prior | Minimum | Maximum |
|---|---|---|
| log10(ρ0/M⊙ kpc−3) | 3 | 15 |
| log10(rs/kpc) | −2.5 | 2.5 |
| α(a) | 0.5 | 3 |
| β(a) | 3 | 9 |
| γ(a) | 0 | 1.5 |
| γi(b) | 0 | 9 |
 |
−1 | 1 |
 |
−1 | 1 |
| log10(r0/kpc) | log10(0.5R1/2/kpc) | log10(2R1/2/kpc) |
| η | 1 | 3 |
Notes. Listed are the characteristic density (ρ0), the NFW scale radius (rs) (Eq. (1)), the Hernquist–Zhao α, β, and γ parameters (Eq. (20)), the broken power-law slopes (γi) (Eq. (19)), the symmetrized inner and outer velocity anisotropies (
and 
) (Eqs. (16) and (17)), the anisotropy transition radius (r0), and the sharpness of the anisotropy transition (η) (Eq. (13)).
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