Results for NGC 1566 (first row), NGC 3351 (second row), and NGC 3953 (third row). For each galaxy, from left to right, we show: (i) how the galaxy cells populate the log Σ_⋆ – log Σ_SFR plane with the corresponding best-fit MS (black line), as well as the MS found by Enia et al. (2020) for unbarred galaxies (grey line), where each point is colour coded according to the d_norm values and the ones sampling the bar-hosting region (d_norm ≤ R_bar, norm) are circled in red; (ii) the spatially resolved distribution of the stellar mass surface density; (iii) the spatially resolved distribution of the SFR surface density; and (iv) the map representing the distance of each cell from the best-fit MS. In the last three columns, we display the 25th level isophote of semi-major axis equal to R₂₅ with a solid black line and the rescaled ellipse enclosing the bar with a dashed black line.