Cumulative mass (left panel), mass-to-light ratio (middle panel), and rotation curve (right panel) of the LMC according to best-fit NFW only (black) and mixed (magenta) gravitational potentials of the axisymmetric Jeans model. The vertical dashed lines denote the extent of the kinematic tracers and the viral radius (R₂₀₀) and the horizontal lines denote the enclosed mass and mass-to-light ratio within these radii. In the rotation curve plot, we overlay the total mean velocity of each Voronoi bin defined in Fig. 6 as orange dots, as well as the total velocity of all LMC member stars as a transparent blue cloud.