Table 3.
L′CO10, obs luminosity, αco, molecular gas mass, and aperture correction factor for the CO-VG sample.
| CAVITY | L′CO10, obs | αco | log MH2 | fap |
|---|---|---|---|---|
| ID | [108 K km s−1 pc 2] | [M⊙ (K km s−1 pc2)−1] | [M⊙] | |
| (1) | (2) | (3) | (4) | (5) |
| 3427 | 8.18 ± 1.04 | 3.1 | 9.43 ± 0.05 | 1.05 |
| 3670 | 2.60 ± 0.58 | 3.5 | 8.98 ± 0.10 | 1.05 |
| 7926 | 15.58 ± 1.11 | 4.1 | 9.84 ± 0.03 | 1.09 |
| 7948 | 3.52 ± 0.63 | 2.8 | 9.07 ± 0.08 | 1.18 |
| 8556 | < 1.12 | 3.1 | < 8.57 | 1.06 |
| 8595 | < 1.30 | 3.8 | < 8.72 | 1.05 |
| 8645 | 14.36 ± 1.36 | 3.5 | 9.71 ± 0.04 | 1.03 |
| 8646 | 6.28 ± 0.50 | 3.1 | 9.31 ± 0.03 | 1.06 |
| 8728 | 3.20 ± 0.49 | 3.3 | 9.09 ± 0.07 | 1.17 |
| 8996 | < 1.35 | 3.0 | < 8.65 | 1.08 |
| ... | ... | ... | ... | ... |
Notes. (1) Catalogue ID in the CAVITY sample. (2) Beam-integrated CO (1–0) line luminosity. (3) CO-to-H2 conversion factor, calculated using the Accurso et al. (2017, Eq. 25) prescription. (4) Molecular gas mass and total error. (5) Aperture correction factor. The molecular gas mass has been derived from the CO(1–0) line emission, except for those galaxies marked with an asterisk, where the CO(1–0) was not detected and the molecular gas mass was derived from the CO(2–1) line emission. The full table is available online at the CDS.
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