Relations between the azimuthal AM of the dynamical disk components and the AM modulus of the DM halo for the galaxy sample in Paper II. Top panels: y-axis gives the total DM AM within the virial radius J_h, while the bottom ones show the AM within 15% of the virial radius J_h(< 0.15 r₂₀₀). From left to right, the panels show the relations for (single large scale) disks, thin and thick, respectively. In each panel, the black line is the linear fit through the data points, while the gray lines show 100 realization of the relation drawn from the covariance matrix of the fit. The Pearson correlation coefficient r_P and the root-mean-square deviation rms are given in the bottom right corner of each panel. In the top and central panels, the highlighted cyan points correspond to the best MW analog in the NIHAO sample, g8.26e11 (Obreja et al. 2018; Buck et al. 2020).