Fig. 7.
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Distributions of the three distinguishing features used to develop our diagnostic tool. From top to bottom: log10(PAH1/Cont215), log10(PAH2/Cont215), and log10(PAH3/Cont215), measured from both the S5 sample (green) of star-forming galaxies and our simulated sample of galaxies (purple). We find very good agreement between the two samples for all the features.
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