Table 1.

Free parameters of the framework.

αInterpolates AM proxy between Mvir (α = 0) and vmax (α = 1)
AM scatterUniversal Gaussian scatter in stellar mass at fixed proxy
νControls degree of halo expansion (−) or contraction (+)
Selection factorGoverns impact of selection effects on theoretical FJR and FP
|$\mathcal {N}(f(M_{\ast }), \sigma _\beta )$|Distribution from which galaxy anisotropy β is drawn
αInterpolates AM proxy between Mvir (α = 0) and vmax (α = 1)
AM scatterUniversal Gaussian scatter in stellar mass at fixed proxy
νControls degree of halo expansion (−) or contraction (+)
Selection factorGoverns impact of selection effects on theoretical FJR and FP
|$\mathcal {N}(f(M_{\ast }), \sigma _\beta )$|Distribution from which galaxy anisotropy β is drawn
Table 1.

Free parameters of the framework.

αInterpolates AM proxy between Mvir (α = 0) and vmax (α = 1)
AM scatterUniversal Gaussian scatter in stellar mass at fixed proxy
νControls degree of halo expansion (−) or contraction (+)
Selection factorGoverns impact of selection effects on theoretical FJR and FP
|$\mathcal {N}(f(M_{\ast }), \sigma _\beta )$|Distribution from which galaxy anisotropy β is drawn
αInterpolates AM proxy between Mvir (α = 0) and vmax (α = 1)
AM scatterUniversal Gaussian scatter in stellar mass at fixed proxy
νControls degree of halo expansion (−) or contraction (+)
Selection factorGoverns impact of selection effects on theoretical FJR and FP
|$\mathcal {N}(f(M_{\ast }), \sigma _\beta )$|Distribution from which galaxy anisotropy β is drawn
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