Table 4.
Properties for the CO-VG sample.
| CAVITY ID | log M⋆ | log SFR | 12 + log O/H |
|---|---|---|---|
| [M⊙] | [M⊙ yr−1] | ||
| (1) | (2) | (3) | (4) |
| 3427 | 10.52 ± 0.10 | 0.59 ± 0.01 | 8.80 |
| 3670 | 10.27 ± 0.09 | −0.32 ± 0.01 | 8.74 |
| 7926 | 10.72 ± 0.10 | 0.54 ± 0.01 | 8.72 |
| 7948 | 10.59 ± 0.09 | −0.08 ± 0.01 | 8.81 |
| 8556 | 10.34 ± 0.09 | −0.80 ± 0.16 | 8.76 |
| 8595 | 10.12 ± 0.08 | −0.05 ± 0.01 | 8.73 |
| 8645 | 10.45 ± 0.11 | 1.31 ± 0.01 | 8.84 |
| 8646 | 10.32 ± 0.09 | 0.34 ± 0.01 | 8.82 |
| 8728 | 9.96 ± 0.08 | 0.02 ± 0.01 | 8.78 |
| 8996 | 9.96 ± 0.09 | −0.48 ± 0.14 | 8.78 |
| ... | ... | ... | ... |
Notes. (1) Catalogue ID in the CAVITY sample. (2) Stellar mass from the MPA-JHU catalogue (Kauffmann et al. 2003b; Brinchmann et al. 2004; Tremonti et al. 2004; Salim et al. 2007). (3) Hα based SFR calculated following the method presented in Duarte Puertas et al. (2017). (4) Gas-phase metallicity 12 + log O/H using both the [N II]/Hα and [O III]/Hβ line ratios and the calibration of Pettini & Pagel (2004). The full table is available online at the CDS.
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