Fig. C.1.

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Comparison of the STFR, using only KROSS sample studied in GS23 datasets, with Tiley et al. (2019). The orange and green lines represent the best fit lines for our and Tiley et al. (2019)’s work, respectively. The blue and green data points represent- Upper Left Panel: Disk-like galaxies characterized by Vrot/σ > 3, Upper Right Panel: Rotation supported galaxies characterized by Vrot/σ > 1, and Lower Panel: KROSS and Tiley et al. (2019) matching sample for Vrot/σ > 1. We note that in this comparison, we used a rotation velocity with in Rout (i.e., Vrot), which is not corrected for pressure support; namely, Vrot is comparable to V2.2 of Tiley et al. (2019).
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