Table 2.
Molecular and atomic gas properties of CHILES z = 0.12 galaxies.
| COSMOS | RA Dec | zHI⊙a | DL | SCOδvb | log(MH2) | SHIδv | log(MHI) | log(M*) c | S1.4 GHz | SFR1.4 GHz | SFR |
|---|---|---|---|---|---|---|---|---|---|---|---|
| ID | J2000 | Mpc | Jy km s−1 | M⊙ | Jy Hz | M⊙ | M⊙ | μJy | M⊙ yr−1 | M⊙ yr−1 | |
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) | (11) | (12) |
| 0969208 | 10h01m16.7s2d17m11.9s | 0.12163 | 569 | 1.648 | 9.71 | 14028.9 | 10.42 | 10.50 | 470.3 ± 21.4 | 13.05 | 5.87 |
| 1189669 | 10h02m09.4s2d20m52.1s | 0.12688 | 595 | 2.226 | 9.88 | 5138.1 | 10.02 | 10.20 | 338.7 ± 17.2 | 10.27 | 6.14 |
| 1197519 | 10h01m20.5s2d18m17.8s | 0.123 | 576 | 1.973 | 9.80 | 4583.6 | 9.94 | 10.30 | 562.7 ± 9.8 | 16.04 | 7.20 |
| 1204323 | 10h01m23.2s2d24m15.0s | 0.12745 | 596 | 1.552 | 9.72 | 1997.0 | 9.61 | 10.10 | 122.0 ± 6.5 | 3.71 | 3.89 |
| 1411106 | 10h01m36.9s2d30m32.1s | 0.12353 | 579 | 2.320 | 9.88 | 4367.7 | 9.92 | 10.50 | 209.0 ± 10.9 | 6.01 | 5.87 |
| 1008875 | 10h00m51.1s2d11m37.7s | 0.12289 | 575 | < 0.107 | < 8.53 | 2204.8 | 9.62 | 9.60 | 62.7 ± 8.5 | 1.25† | 0.33 |
| 1009969 | 10h00m53.1s2d10m57.7s | 0.12389 | 580 | < 0.107 | < 8.55 | 1764.8 | 9.53 | 9.56 | – | – | 0.62 |
| 1197786 | 10h01m31.5s2d25m57.7s | 0.12337 | 578 | < 0.107 | < 8.53 | 4087.5 | 9.39 | 9.45 | 49.1 ± 3.1 | 1.41 | 0.57 |
| 1200839 | 10h01m20.3s2d27m14.9s | 0.12133 | 567 | < 0.150 | < 8.66 | 1272.9 | 9.88 | 9.35 | 21.6 ± 2.5 | 0.60 | 1.28 |
| 1399657 | 10h01m57.4s2d35m08.8s | 0.11358 | 528 | < 0.085 | < 8.35 | 1196.7 | 9.28 | 9.54 | 32.9 ± 10.7 | 0.79 | 0.32 |
| 1429536 | 10h01m33.8s2d33m03.0s | 0.11269 | 524 | < 0.146 | < 8.59 | 1597.5 | 9.40 | 9.39 | – | – | 0.56 |
| 1430950 | 10h01m11.6s2d32m27.1s | 0.11159 | 518 | < 0.107 | < 8.44 | 2263.2 | 9.54 | 8.92 | – | – | 0.51 |
| 1440643 | 10h01m26.9s2d28m02.9s | 0.12197 | 571 | < 0.107 | < 8.52 | 2295.6 | 9.63 | 8.48 | 36.6 ± 2.8 | 1.02 | 0.59 |
| 1440745 | 10h01m19.8s2d27m56.5s | 0.12309 | 576 | < 0.085 | < 8.43 | 725.9 | 9.14 | 8.79 | 22.8 ± 2.7 | 0.65 | 0.24 |
Notes. The table is sorted first by CO detections (top) vs. non-detections (bottom), and then by COSMOS ID number. aUncertainty on the H I redshift is ∼0.00008. bThe CO flux is calculated from CASA. The limiting CO luminosity is calculated from 3σ in the 5″ smoothed data, over 50 km s−1. cWe reproduce the stellar mass and SFR from (Hess et al. 2019); the uncertainties were reported of order 25% and 35%, respectively. †Star formation for 1008875 is calculated from 70% of the total S1.4 GHz flux, where the other 30% is due to AGN activity. See text for details.
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