Results of the axisymmetric modeling of NGC 1272 of the complete stellar kinematic dataset. As a function of the quality of the fits measured by the AIC_p we show: from left to right, and from top to bottom: the BH mass M_BH; the dynamical V-band mass-to-light ratio Υ_*, V; the DM density at 10 kpc ρ₁₀; and the inner slope of the DM density profile γ_DM. The gray points show the individual models, the red dots show the best-fitting model, and the black lines show the lower envelope of the distributions of gray points.