Bottom panels: Distribution of haloes versus stellar mass for the galaxies in our sample, using a threshold of $\lambda /\sqrt{ϵ}\ge 0.31$ (left) and 0.71 (right). Blue stars and red dots represent disks and spheroids (CS), respectively. Upper panels: Histograms showing the log₁₀M₂₀₀ mass distribution for disks (starred blue bars) and spheroids (dashed red bars). Middle panels: Distribution of central disks (purple), satellite disks (blue), central spheroids (green), and satellite spheroids (red). We can see that disk galaxies do not have any particular distribution in M₂₀₀, showing even a slightly more extended distribution in halo mass than our CS and reaching up to the most massive clusters.