Open Access
Table A.2.
Key properties of the sample used in this paper, as provided in Valentino et al. (2020).
| ID | Redshift | Log Stellar Mass [M⊙] | Infrared Luminosity [1012 L⊙] | Log SFR [M⊙ yr−1] | S/N CO(2–1) |
|---|---|---|---|---|---|
| 2299† | 1.3948 ± 0.00025 | 10.8221 | 4.911 ± 0.06045 | 2.864 | 15 |
| 2993 | 1.1917 ± 0.00031 | 10.9888 | 1.997 ± 0.1152 | 2.473 | 7 |
| 13205 | 1.2659 ± 0.00038 | 11.1442 | 1.619 ± 0.1395 | 2.382 | 5 |
| 13854 | 1.2695 ± 0.00024 | 11.0327 | 2.260 ± 0.1609 | 2.527 | 7 |
| 15069 | 1.2119 ± 0.00025 | 10.61 | 1.213 ± 0.09902 | 2.257 | 4 |
| 18911 | 1.1710 ± 0.00023 | 10.6379 | 0.801 ± 0.06477 | 2.077 | 3 |
| 19021 | 1.2581 ± 0.00024 | 10.2025 | 3.276 ± 0.09806 | 2.688 | 8 |
| 21060 | 1.2818 ± 0.00024 | 9.8400 | 1.834 ± 0.1005 | 2.436 | 4 |
| 21820† | 1.3790 ± 0.00032 | 10.9209 | 1.863 ± 0.06887 | 2.443 | 6 |
| 26925 | 1.1671 ± 0.00030 | 11.2428 | 0.842 ± 0.07139 | 2.098 | 7 |
| 27172 | 1.2348 ± 0.00032 | 10.757 | 1.002 ± 0.09275 | 2.174 | 4 |
| 30122 | 1.4626 ± 0.00031 | 11.08 | 2.086 ± 0.09912 | 2.492 | 9 |
| 30694 | 1.1611 ± 0.00021 | 10.7949 | 0.877 ± 0.09839 | 2.116 | 8 |
| 31880† | 1.3999 ± 0.00034 | 11.0176 | 1.888 ± 0.06537 | 2.449 | 7 |
| 34023†, ∧ | 1.3461 ± 0.00032 | 10.97 | 1.694 ± 0.09633 | 2.402 | 3 |
| 35349 | 1.2553 ± 0.00045 | 11.1876 | 1.221 ± 0.03919 | 2.259 | 8 |
| 37250 | 1.1525 ± 0.00034 | 10.95 | 1.831 ± 0.08732 | 2.436 | 14 |
| 38053 | 1.1550 ± 0.00036 | 10.7301 | 1.074 ± 0.1345 | 2.204 | 6 |
| 41210 | 1.3145 ± 0.00021 | 10.5562 | 2.580 ± 0.1015 | 2.585 | 12 |
| 41458 | 1.2949 ± 0.00022 | 10.8348 | 3.083 ± 0.1544 | 2.662 | 9 |
| 42925 | 1.6028 ± 0.00054 | 9.4012 | 4.900 ± 0.2856 | 2.863 | 6 |
| 44641 | 1.1509 ± 0.00024 | 11.55 | 1.054 ± 0.04951 | 2.196 | 5 |
| 44694 | 1.2056 ± 0.00036 | 10.7568 | 0.776 ± 0.1006 | 2.063 | 6 |
| 48881 | 1.1569 ± 0.00022 | 10.86 | 1.641 ± 0.1714 | 2.388 | 5 |
| 51330 | 1.6317 ± 0.00041 | 10.2205 | 4.675 ± 0.4038 | 2.843 | 6 |
| 51936† | 1.4030 ± 0.00029 | 10.243 | 2.034 ± 0.1167 | 2.481 | 9 |
Notes. † indicates the five galaxies where only one measurement set was kept to preserve beam consistency througout the sample. ∧Ultravista Ks band data is missing for this galaxy.
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