Comparison of the integrated velocity dispersion profiles as a function of the spherical radius r of the AGAMA-04 galaxy spheroid with those identified by the six different dynamical decomposition methods. Top panel: Comparison of the radial integrated velocity dispersion profiles σ_r(< r). Middle panel: Comparison of the azimuthal integrated velocity dispersion profiles σ_ϕ(< r). Bottom panel: Comparison of the polar integrated velocity dispersion profiles σ_θ(< r). In all cases, the profiles corresponding to the original spheroid are shown with a black solid line.