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Table D.1.
Summary of the model parameters sampled in the hierarchical inference on TDLMC Rung3 with the anisotropy model of Eq. (D.1).
| Name | Prior | Description |
|---|---|---|
| Cosmology | ||
| H0 [km s−1 Mpc−1] | 𝒰([0, 150]) | Hubble constant |
| Ωm | =0.27 | Current normalized matter density |
| Mass profile | ||
| λint | 𝒰([0.8, 1.2]) | Internal MST population mean |
| σ(λint) | 𝒰([0, 0.2]) | 1-σ Gaussian scatter in the internal MST |
| Stellar kinematics | ||
| ⟨aani⟩ | 𝒰([0.1, 5]) or 𝒰(log([0.1, 5])) | Scaled anisotropy radius (Eqs. (51) and (52)) |
| σ(aani) | 𝒰([0, 1]) | σ(aani)⟨aani⟩ is the 1-σ Gaussian scatter in aani |
| β∞ | 𝒰([0, 1]) | Anisotropy at infinity (Eq. (D.1)) |
| σ(β∞) | 𝒰([0, 1]) | 1-σ Gaussian scatter in β∞ distribution |
| Line of sight | ||
| ⟨κext⟩ | =0 | Population mean in external convergence of lenses |
| σ(κext) | =0.025 | 1-σ Gaussian scatter in κext |
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