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Table B.1.
Physical properties of GAMA 526784 and its star clusters.
| Source | CO(1-0)5σ (μJy) | SFR (10−5 M⊙ yr−1) | 12 + log([O/H]) | log(M⋆/M⊙) | log(MH2/M⊙)αCO, met | log(MHI/M⊙) |
|---|---|---|---|---|---|---|
| GAMA 526784 | ≤5.80 | 100 | 8.30 |
 |
≤7.60 | 8.70 ± 0.90 |
| Globular Cluster 1 | ≤1.88 | – | – | 5.64 | – | – |
| Star Cluster 2 | ≤0.87 | 7.49 | 8.09 | 5.19 | ≤7.09 | – |
| Globular Cluster 3 | ≤0.61 | – | – | 5.90 | – | – |
| Globular Cluster 4 | ≤0.82 | – | – | 5.93 | – | – |
| Globular Cluster 5 | ≤1.14 | – | – | 5.89 | – | – |
| Star Cluster 6 | ≤0.57 | 0.73 | 8.24 | 5.75 | ≤6.59 | – |
| Star Cluster 7 | ≤1.03 | 1.48 | 8.39 | 4.88 | ≤6.64 | – |
| Star Cluster 8 | ≤0.85 | 34.00 | 8.20 | 5.33 | ≤6.93 | – |
| Star Cluster 9 | ≤0.90 | 8.55 | 8.34 | 5.06 | ≤6.71 | – |
| Globular Cluster 10 | ≤0.57 | – | – | 5.77 | – | – |
| Star Cluster 11 | ≤1.03 | 1.45 | 8.39 | 4.50 | ≤6.66 | – |
| Star Cluster 12 | ≤0.84 | 33.00 | 8.23 | 5.50 | ≤6.88 | – |
| Star Cluster 13 | ≤0.59 | 0.86 | 8.36 | 5.49 | ≤6.41 | – |
| Star Cluster 14 | ≤0.66 | 3.08 | 8.32 | 4.60 | ≤6.61 | – |
| Star Cluster 15 | ≤0.71 | 4.27 | 8.30 | 4.93 | ≤6.66 | – |
| Star Cluster 16 | ≤0.60 | 0.98 | 8.40 | 5.73 | ≤6.34 | – |
| Star Cluster 17 | ≤0.60 | 0.71 | 8.30 | 4.17 | ≤6.56 | – |
| Star Cluster 18 | ≤0.58 | 2.13 | 8.39 | 5.69 | ≤6.37 | – |
| Star Cluster 19 | ≤0.61 | 19.00 | 8.24 | 5.52 | ≤6.70 | – |
| Star Cluster 20 | ≤0.62 | 18.00 | 8.27 | 5.47 | ≤6.66 | – |
| Globular Cluster 21 | ≤0.62 | – | – | 5.69 | – | – |
| Star Cluster 22 | ≤0.64 | 1.43 | 8.41 | 4.27 | ≤6.43 | – |
| Star Cluster 23 | ≤0.60 | 17.00 | 8.17 | 5.05 | ≤6.83 | – |
| Star Cluster 24 | ≤0.58 | 7.74 | 8.32 | 4.55 | ≤6.57 | – |
| Star Cluster 25 | ≤0.58 | 5.71 | 8.37 | 4.58 | ≤6.48 | – |
| Star Cluster 26 | ≤0.61 | 2.62 | 8.25 | 4.91 | ≤6.66 | – |
| Star Cluster 27 | ≤0.92 | 9.37 | 8.17 | 4.65 | ≤7.01 | – |
| Globular Cluster 28 | ≤1.01 | – | – | 5.50 | – | – |
| Globular Cluster 29 | ≤0.71 | – | – | 5.83 | – | – |
Notes. Columns show: (1) Source ID from Paper I; (2) 5σ CO(1-0) flux upper limits; (3) SFRs from Hα measurements; (4) Gas-phase metallicities; (5) Stellar masses; (6) Molecular gas mass upper limits; (7) Neutral gas mass (for the main galaxy only).
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