Comparison between our results (x-axis) and the same parameter from the literature (y-axis): between the single Sérsic model and aperture flux from C18 (panel a), between the model flux in WISE W1 and the one from the S⁴G single Sérsic modelling (panel b), between the effective radius in WISE W1 and the one from the S⁴G single Sérsic modelling (panel c), between the Sérsic index in WISE W1 and the one from the S⁴G single Sérsic modelling (panel d), between the model flattening in WISE W1 and the one from the S⁴G single Sérsic fitting (panel e), between our estimate of the galaxy inclination and the one taken from HyperLeda (panel f). The clustering dots at 90° for both estimates are either galaxies for which an edge-on model in the S⁴G modelling pipeline was adopted, or for which the apparent flattening was less then the intrinsic one (see Appendix D). The black dotdash lines show the one-to-one relationship and the orange dashed lines refer to the regression lines.