Table 4.
Integrated CO line fluxes and derived CO luminosities for each galaxy.
| Arc | CO | μΔνSν | μL′CO |
|---|---|---|---|
| Transition | [Jy ⋅ Km s−1] | [1010 K km s−1 pc2] | |
| J0033 | (4–3) | 2.0±0.1 | 3.4±0.2 |
| J0108 | (4–3) | 1.3±0.4 | 1.4±0.4 |
| J0900A | (4–3) | < 0.5 | < 0.6 |
| J0900B | (4–3) | < 0.5 | < 0.6 |
| J1050 | (4–3) | < 0.3 | < 1.2 |
| J1050A | (3–2) | 0.4±0.1 | 1.2±0.3 |
| J1226A | (5–4) | < 0.4 | < 0.7 |
| J1226B | (5–4) | < 0.2 | < 0.4 |
| J1429 | (3–2) | < 0.4 | < 1.7 |
| J1527 | (3–2) | < 0.4 | < 1.6 |
| J2111 | (3–2) | < 0.2 | < 0.9 |
| Sunburst | (4–3) | < 0.4 | < 0.6 |
Notes. Listed are the galaxy names, CO transition line, unmagnified integrated flux (Jy kms−1), and unmagnified calculated CO luminosities (μL′CO in units of 1010 K km s−1pc2). Statistical uncertainties on the measured values are included, with upper limits being considered at the 3σ significance level.
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