Fig. 3.

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SFR–M★ plane of our galaxy sample, color-coded by the S/N of each individual object. The top panel shows our subsample with reliable stellar velocity maps (i.e., maps with ≥90% valid spaxels within 1Reff). The bottom panel shows galaxies with reliable gaseous velocity maps. The lines indicate the boundaries separating star-forming, green valley, and quiescent galaxies, as defined in Behroozi et al. (2019).
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