Figure 3. [C II] FWHM vs. line luminosity for the AS2UDS [C II] emitters. We compare our sample to star-forming galaxies and AGNs from the literature. The dashed line shows the 1σ limit for false positives in the AS2UDS sample (i.e., 84% of false positives lie to the left of this line). The solid line shows a LFWHM C 0.5
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