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