LMC axisymmetry tests. Left panels: Residual variance of the mean V_LOS versus the mean V_Y correlation for different line of nodes orientations, colour-coded by the inclination angle for all stars (top), old stars (middle), and young stars (bottom) rows, respectively. Middle panels: Line of nodes orientation versus inclination angle, colour-coded by the residual variance for the old stars and separated into old and young populations. The shaded regions in these panels correspond to the best fit values from the 3D Jeans model and their uncertainties. Right panels: Mean V_LOS versus mean V_Ytan(θ) for the LMC orientation with minimum residual variance for each respective population. These plots are colour-coded by distance from the centre of each Voronoi bin, and the dashed lines indicate a perfect anti-correlation.