Rotation and dispersion profiles for NGC 2808 and each of its populations. The rotation profiles for each population are shown on the left and the dispersion profiles on the right. The angle of rotation is shown in the center. The continuous profiles (solid lines) and binned profiles (symbols) shown here are each determined by fitting the respective model to line-of-sight velocities of single stars. The shaded area represents the 1σ uncertainty of each continuous profile and rotation angle. The dotted vertical line in each radial profile illustrates the half-light radius of NGC 2808.