Fig. 5.
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Two examples (SMILES IDs 1237 and 1479) of the best-fitting SEDs of the MIRI-selected SFGs candidates at z ∼ 1.5. The red and blue curves show the dust emission and the stellar emission, respectively. The purple circles show the observed photometric fluxes. The filled red circles are the model fluxes. The best model for 1479 requires an AGN component; in 1237 there is no AGN.
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