Maps of the stellar LOS velocity subtracted of systemic velocity (top panels) and velocity dispersion corrected for σ_inst (bottom panels) of NGC 4277 derived from the S/N = 40 Voronoi-binned MUSE data (left panels) and from the asymmetric-drift-corrected dynamical model (right panels). The FOV is 13 × 13 and is oriented with north being up and east to the left. The solid and dashed white lines mark the region adopted for modelling between the inner edge of the inner disc and location of the disc break radius, respectively.