Spectral energy distribution (SED) of two of our galaxies (upper panel: ID 12091; lower panel: ID 19062) as fit using CIGALE. Observed flux densities are shown by opened blue circles, while observed upper limits are shown by downward blue triangles. Black, red, orange, blue, and green lines correspond to the total, dust, AGN, stellar unattenuated and stellar attenuated emission, respectively. For the galaxy ID 12091, the AGN contribution (i.e., L_AGN/(L_AGN + L_dust) is of 0% and the sharpest MIRI band (shortest wavelength) dominated by dust emission (i.e., ) is the 10 μm band. For the galaxy ID 19062, the AGN contribution is of 30% and none of the MIRI bands is dominated by dust emission.