Table 5.
Star formation, BH, and dynamical properties.
| Galaxy | SFR | M⋆ | M• | Mdyn |
|---|---|---|---|---|
| [M⊙ yr−1] | [1011 M⊙] | [109 M⊙] | [1010 M⊙] | |
| (1) | (2) | (3) | (4) | (5) |
| W0116–0505 | 202 |
4.83 |
≤3.2 | … |
| W0134–2922 | 431 |
2.00 |
… | … |
| W0220+0137 | 803 |
1.21 |
≤40 | 2.8 |
| W0236+0528 | 493 |
0.84 |
… | … |
| W0410–0913 | 3314 |
1.61 |
≤316 | … |
| W0831+0140 | 2863 |
1.52 |
≤5.0 | … |
| W2246–0526 | 688 |
3.04 |
4.0 |
5.5 |
Notes. (1) Galaxy name; (2) Star formation rate of the galaxy host, derived from far-IR scaling relations (Sect. 6 for details); (3) Stellar mass of the galaxy host, derived from rest-UV through near-IR photometry (see text and Appendix B for details); (4) BH mass, derived from rest-UV and optical spectroscopy (Finnerty et al. 2020; except W2246–0526, Tsai et al. 2018); (5) Dynamical mass, derived from kinematic modeling of the [C II] line (this work; see Appendix A). The errors quoted in the SFR and M⋆ are not standard deviations, but refer to the entire range of values spanned by the individual estimates used to calculate the averages.
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