Table 5.
Molecular gas properties.
| Galaxy ID | zspec | J → J − 1 | νobs | SCO(J → J − 1)Δv | M(H2) | αCO | τdep |
 |
τdep, MS |
 |
|---|---|---|---|---|---|---|---|---|---|---|
| (GHz) | (Jy km s−1) | (1010 M⊙) |
 |
(109 yr) | (109 yr) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) |
| A963-1 | 0.211 | 1→0 | 95.163 |
 |
 |
3.24 |
 |
 |
 |
 |
| A963-2 | 0.208 | 1→0 | 95.415 |
 |
 |
3.94 |
 |
 |
 |
 |
| A2219-1 | 0.230 | 1→0 | 93.694 |
 |
 |
2.16 |
 |
 |
 |
 |
| A2219-2 | 0.233 | 1→0 | 93.504 |
 |
 |
4.36 |
 |
 |
 |
 |
| A1763-1 | 0.232 | 1→0 | 93.549 |
 |
 |
2.80 |
 |
 |
 |
 |
| A1763-2 | 0.226 | 1→0 | 94.015 |
 |
 |
4.36 |
 |
 |
 |
 |
| A697-1 | 0.274 | 1→0 | 90.466 |
 |
 |
4.21 |
 |
 |
 |
 |
| GAL1416+4446 | 0.396 | 1→0 | 82.549 | 1.0 ± 0.1 |
 |
4.22 |
 |
 |
 |
 |
| GAL0926+1242-A | 0.489 | 2→1 | 154.869 | 0.6 ± 0.1 |
 |
4.08 |
 |
 |
 |
 |
| GAL0926+1242-B | 0.489 | 2→1 | 154.869 | 0.5 ± 0.1 |
 |
2.67 |
 |
 |
 |
 |
| HLS071708+374557 | 0.542 | 2→1 | 149.467 |
 |
 |
2.82 |
 |
 |
 |
 |
| HLS071718+374124 | 0.576 | 2→1 | 146.28 |
 |
 |
4.18 |
 |
 |
 |
 |
| HLS071731+374250 | 0.537 | 2→1 | 149.953 |
 |
 |
3.66 |
 |
 |
 |
 |
| HLS071740+374755 | 0.563 | 2→1 | 147.497 |
 |
 |
4.16 |
 |
 |
 |
 |
| HLS071743+374040 | 0.544 | 2→1 | 149.312 |
 |
 |
3.26 |
 |
 |
 |
 |
| HLS071754+374303 | 0.544 | 2→1 | 149.312 |
 |
 |
3.58 |
 |
 |
 |
 |
| HLS071754+374639 | 0.545 | 2→1 | 149.216 |
 |
 |
4.32 |
 |
 |
 |
 |
| HLS071760+373709 | 0.553 | 2→1 | 148.447 | < 0.47 | < 0.90 | 4.01 | < 0.43 | < 0.19 |
 |
 |
| HLS071805+373805 | 0.555 | 2→1 | 148.256 | < 0.42 | < 0.87 | 4.36 | < 1.89 | < 0.24 |
 |
 |
| HLS071814+374117 | 0.542 | 2→1 | 149.525 |
 |
 |
3.90 |
 |
 |
 |
 |
Notes. (1) Galaxy name; (2) spectroscopic redshift of the galaxy; (3−4) CO(J → J − 1) transition and observer frame frequency; (5) CO(J → J − 1) velocity integrated flux; (6) molecular gas mass; (7) CO-to-H2 conversion factor; (8) depletion timescale τdep = M(H2)/SFR; (9) molecular gas to stellar mass ratio; (10 and 11) depletion timescale and molecular gas to stellar mass ratio for MS field galaxies (Tacconi et al. 2018). For HLS071760+373709 and HLS071805+373805, the quantities in Cols. (5,6,8,9) are 3σ upper limits.
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