Fig. 4.

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Top panel: Distribution of galaxies with KINEMETRY info on the stellar component in the SFR-M★ plane, color-coded by the average asymmetry parameter of the stellar kinematic map. As in Fig. 3, the lines indicate the boundaries separating star-forming, green valley, and quiescent galaxies as present in Behroozi et al. (2019). The upper curves indicate the PDF of galaxies classified as asymmetric according to different KINEMETRY thresholds in Iasym. Bottom panel: As in the upper panel, but for galaxies with KINEMETRY info on the gaseous component.
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