Position-velocity (P-V, top) and position-dispersion (P-σ, bottom) curves of the stellar (black) and gas component of NGC 1052 from the MUSE data. Specifically, the gas component is probed via the [O III] (magenta), [O I] (blue), and H α (green) emission lines. Similarly to Fig. 11 the curves were obtained considering a pseudo-slit 1″ in width aligned according to the major (left) and minor (centre) axis of the rotation, as well as the axis of the radio jet (right). The position angles are listed in Tables 1 and 4. Velocities are centred to the kinematic centre, and the radius is calculated as the distance from the photometric centre. The grey dashed lines show zero points for position and velocity, as reference.