Same as Fig. A.1, but for the one-populations models with a varying three-parameter mass-to-light ratio (Sect. 4.2). From top to bottom and left to right, the panels show the inner anisotropy β₀, outer anisotropy β_∞, the anisotropy transition radius log(R_β), inner rotation parameter κ₀, outer rotation parameter κ_∞, the rotation transition radius log(R_κ), the inner mass-to-light ratio 𝚼₀, outer mass-to-light ratio 𝚼_∞, mass-to-light ratio transition radius log(R_𝚼), and the fraction of background stars ϵ in percent. The black hole mass is fixed to 4.3 × 10⁶ M_⊙, dark matter is not considered in the gravitational potential.