NIR-through-millimetre SEDs (CFHT/WIRCam, Spitzer/IRAC, Herschel/SPIRE, SCUBA-2, and ALMA at 1.3 and 2.2 mm) of the sources with line detections (full red circles). Downward arrows are 5σ upper limits. The CIGALE best-fit model is shown with a solid black line. The dotted blue line shows the stellar light before dust attenuation, and the solid blue line shows the attenuated stellar light. The green line shows the dust component. The best-fit modified blackbody model to the submm/millimetre data is shown with a dashed magenta line. The source identifier is annotated and listed in Table 3.