Mass models of nine representative galaxies in our sample (similar plots for our full sample and the corresponding posterior distributions are available in this link). In each panel, the observed circular speed profiles are shown with dark red circular markers. The colour lines and bands represent the gravitational contribution from the stellar disc (orange), bulge (pink, if present), H I (blue), H₂ (green, if present) and dark matter (grey) to the total mass model (red) and their corresponding 1σ confidence bands.