Radial profiles of the best fit found by ^3DBarolo for v_rot, v_rad, v_disp (σ_gas), PA (ϕ), and i. The position of the AGN (x_o and y_o in pixel units) and the systemic velocity (v_sys) are fixed to the values previously found by kinemetry. The size of the vertical bars in the radial profile of integrated intensities (Σ) reflect the deviations from axisymmetry in the gas distribution. The gray and red markers represent the output values of the fitted parameters obtained after the first (step-1) and second (step-2) runs, respectively.