Fig. 5.

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SEDs of three CO emitters (filled magenta circles): 01a (top panel), 01b (middle panel), and 01c (bottom panel). Downward arrows represent 5σ upper limits. The CIGALE bestfit model is shown with a solid black line. Dotted lines show the stellar light (red for the older population and blue for the younger) before dust attenuation, and the solid red and blue lines show the attenuated stellar light. The orange line shows the dust component, and the green line shows the radio synchrotron emission.
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