Kinematic maps of NGC 1277. From left to right, V, σ, and V_rms maps of NGC 1277. The dashed line in the left panel indicates the kinematic major axis determined with kinemetry. The top row shows an interpolated version of the maps, whereas the lower one shows the individual fibre values. The grey contours denote isophotes separated by 0.5 mag arcsec⁻² intervals obtained from an HST F625W image (top row) and from the integral field data integrated between 6150 Å and 6650 Å (lower row). The axes are in units of arcseconds.