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Table 3.
Best-fit values for the ensemble VERTICO samples.
| Sample | Index (N) | log10 A | σ |
|---|---|---|---|
| (log10 M⊙ yr−1 pc2) | (dex) | ||
| Galaxies: 720 pc | 0.97 ± 0.07 | −3.20 ± 0.08 | 0.42 |
| Galaxies: 1.2 kpc | 0.91 ± 0.08 | −3.15 ± 0.11 | 0.35 |
| HI-deficient | 0.93 ± 0.04 | −2.98 ± 0.09 | 0.30 |
| HI-normal | 0.84 ± 0.04 | −3.26 ± 0.10 | 0.41 |
Notes. Best-fit slope (N), intercept (referenced to Σmol units of 1 M⊙ pc−2), and scatter (σ) results for the resolved KS relation in the VERTICO sample, comparing the ensembles at 720 pc and 1.2 kpc resolution, as well as the HI-normal and HI-deficient samples of galaxies.
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