UV to millimeter SEDs for 27 OFGs. The symbol convention and lines are the same as those in Figs. 7. The data from the UV to MIR (16 μm) bands are fitted with the FAST++ code (see §4.1). From 24 μm up to millimeter wavelengths, we fitted galaxies with a Herschel counterpart using the CIGALE code (orange solid line) and galaxies without a Herschel counterpart but with the ALMA 1.13 mm detection using the dust template libraries (green line; Schreiber et al. 2018c, see §4.2).