SED models obtained with the GalaPy software for the studied galaxies, as explained in Appendix E, with available enough photometric observations in the literature. In the main panels, the abscissas and ordinates correspond to the observed wavelength in Ångströms and the flux density in mJy. Points correspond to the photometric measurements obtained from the WISE archive and Meerkat continuum levels (this work), while solid lines correspond to the unattenuated stellar emission (green), molecular cloud component (MC, purple), stellar emission considering extinction (extinct, red), and diffuse dust (DD, yellow). The bottom sub-panels highlight the residuals with 1 and 2σ shaded areas, which are also labelled in the main panels.