Comparison of the main parameters of the best-fit DC14 and coreNFW models: stellar mass (top left), halo mass (top right), halo concentration (bottom left), and log slope of the dark matter density at the innermost point of the rotation curve (bottom right). The inner log slopes in the latter plot were measured at the innermost point of each rotation curve and not in the actual centres of the galaxies. Therefore they are an upper limit to the real central slopes of the dark matter haloes. Colours and symbols are as in Figs. 5 and 8.