CO(2-1) spectra from the two nuclear regions of Mrk 1066 integrated over an area equal to the beam. The Gaussians we fit to identify the different kinematic components are the color dash-dotted lines and their sum the black line. The horizontal orange dashed line is the 5σ level, where σ is the standard deviation in the channels outside of the spectral window (vertical gray dashed lines). We also show the modeled velocity (vertical red dashed line) for the rotating disk obtained with ^3DBAROLO for the central pixel of the area (purple stars in Fig. 2, panel e). Relative coordinates in pc from the AGN for the central pixel of the apertures are given in the top left boxes.