Table 4.
Molecular gas properties.
| Galaxy ID | zspec | CO(J → J–1) | νobs | SCO(J → J − 1) | M(H2) | τdep | 
|
τdep, MS | 
|
|---|---|---|---|---|---|---|---|---|---|
| (GHz) | (Jy km s−1) | (1010 M⊙) | (109 yr) | (109 yr) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| DES-RG 399 | 0.388439 | 3→2 | 249.054 | <1.5 | <1.0 | <0.48 | <0.11 |  |
0.12 ± 0.11 |
| DES-RG 708 | 0.60573 | 3→2 | 215.351 | <1.5 | <2.6 | <0.23 | <0.09 |  |
0.13 ± 0.11 |
| COSMOS-FRI 16 | 0.9687 | 4→3 | 234.185 | <5.5 | <18.8 | <7.2 | <1.5 |  |
0.32 ± 0.22 |
| COSMOS-FRI 31 | 0.9123 | 4→3 | 241.036 | <5.2 | <15.8 | — | <1.8 |  |
0.33 ± 0.24 |
| COSMOS-FRI 70 | 2.625 | 7→6 | 222.525 | 0.69 ± 0.31 | <6.6 | <0.27 | <0.29 |  |
0.71 ± 0.28 |
Notes. (1) Galaxy name; (2) spectroscopic redshift as in Table 3; (3)–(4) CO(J → J–1) transition and observer frame frequency; (5) CO(J → J–1) velocity integrated flux; (6) molecular gas mass; (7) depletion time scale τdep = M(H2)/SFR24 μm; (8) molecular gas to stellar mass ratio; (9)–(10) depletion time scale and molecular gas to stellar mass ratio for main sequence field galaxies (Tacconi et al. 2018). Upper limits are reported at 3σ.
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