Table 4
Galaxy mass estimated using OIII images. Derived quantity yields and metallicities.
| Name | log Mgas(ΣSFR) M⊙ | Gas fraction | 12 + log(O/H) | log Yields |
|
|
||||
| CDFaC9 | 9.51 ± 0.29 | 0.27 ± 0.17 | 8.07  |
–2.61 ± 0.54 |
| CDFS4414 | 10.11 ± 0.30 | 0.37 ± 0.20 | 8.47  |
–2.09 ± 0.50 |
| CDFS4417 | 10.47 ± 0.30 | 0.72 ± 0.18 | 8.48  |
–1.60 ± 0.62 |
| CDFS6664 | 9.61 ± 0.30 | 0.69 ± 0.17 | 7.88  |
–2.25 ± 0.72 |
| CDFS16767 | 9.49 ± 0.30 | 0.32 ± 0.16 | 8.28  |
–2.34 ± 0.69 |
| CDFS11991 | 9.47 ± 0.30 | 0.50 ± 0.19 | 7.87  |
–2.53 ± 0.68 |
| CDFS2528 | 9.97 ± 0.30 | 0.73 ± 0.14 | 8.22  |
–1.84 ± 0.87 |
| CDFS16272 | 9.30 ± 0.30 | 0.68 ± 0.16 | 7.92  |
–2.22 ± 0.77 |
| CDFS9313 | 9.87 ± 0.30 | 0.79 ± 0.16 | 7.95  |
–1.97 ± 0.83 |
| CDFS9340 | 9.89 ± 0.30 | 0.91 ± 0.08 | 8.28  |
–1.23 ± 1.18 |
| CDFS12631 | 10.31 ± 0.30 | 0.69 ± 0.20 | 7.89  |
–2.25 ± 0.69 |
| CDFS14411 | 9.72 ± 0.30 | 0.73 ± 0.14 | 8.16  |
–1.89 ± 0.74 |
| CDFS5161 | 9.87 ± 0.30 | 0.62 ± 0.27 | 7.69  |
–2.54 ± 0.93 |
| LnA1689-2 | 10.09 ± 0.31 | 0.62 ± 0.23 | 7.92  |
–2.32 ± 1.42 |
| LnA1689-4 | 9.17 ± 0.29 | 0.84 ± 0.14 | 7.92  |
–1.89 ± 0.66 |
| LnA1689-1 | 9.58 ± 0.30 | 0.32 ± 0.16 | 8.35  |
–2.27 ± 0.66 |
| Q1422D88 | 9.63 ± 0.30 | 0.10 ± 0.07 | 7.94  |
–2.99 ± 0.71 |
| 3C324C3 | 9.80 ± 0.30 | 0.57 ± 0.23 | 7.79  |
–2.51 ± 0.91 |
| Cosmic Eye | 9.63 ± 0.29 | 0.55 ± 0.32 | 7.97  |
–2.37 ± 0.81 |
| SSA22aM38 | 10.14 ± 0.30 | 0.19 ± 0.15 | 8.14  |
–2.64 ± 0.45 |
| SSA22aD17 | 9.40 ± 0.30 | 0.22 ± 0.25 | 8.24  |
–2.50 ± 0.54 |
| SSA22aaug96M16 | 9.33 ± 0.30 | 0.16 ± 0.11 | 8.21  |
–2.62 ± 0.95 |
| SSA22aC16 | 10.81 ± 0.29 | 0.61 ± 0.24 | 8.35  |
–1.90 ± 0.62 |
| SSA22aC36 | 10.01 ± 0.30 | 0.45 ± 0.22 | 8.44 |
–2.02 ± 0.57 |
| DSF2237bC21 | 10.08 ± 0.30 | 0.16 ± 0.11 | 8.79  |
–2.04 ± 0.36 |
| DSF2237bD29 | 9.85 ± 0.30 | 0.12 ± 0.09 | 8.34  |
–2.55 ± 0.52 |
Notes. Column 1, object name; Col. 2, mass of gas in [M⊙] obtained by inverting the Schmidt-Kennicutt law and adding the surface star formation rate at every galaxy pixel throughout the galaxy extention; Col. 3, gas fraction; Col. 4, metallicity at 0.375 arcsec using the Maiolino et al. (2008) metallicity calibration; Col. 5, effective yields.
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