Table D.1.
Calculated molecular line ratios used as input for radiative transfer modelling of LARS 3 and 8.
| ID | Line | Imb | CAP | θ | Line/CO(1–0) |
|---|---|---|---|---|---|
| [K km s−1] | [arcsec] | ||||
| 3 | CO(1–0) | 7.13 | 1.94 | 22.1 | 1.00 |
| 3 | CO(2–1) | 15.93 | 3.58 | 11.0 | 1.02 |
| 3 | HCN(1–0) | 1.06 | 1.00 | 28.7 | 0.13 |
| 3 | HCO+(1–0) | 1.08 | 1.00 | 28.6 | 0.13 |
| 8 | CO(1–0) | 6.85 | 1.36 | 22.2 | 1.00 |
| 8 | CO(2–1) | 11.70 | 1.10 | 11.1 | 0.35 |
| 8 | CO(3–2) | 6.50 | 1.00 | 18.5 | 0.48 |
| 8 | HCN(1–0) | 0.29 | 1.00 | 28.9 | 0.05 |
| 8 | HCO+(1–0) | 0.19 | 1.00 | 28.7 | 0.03 |
Notes. The galaxy id is given in Col. 1, followed by the observed integrated main beam brightness temperature in Col. 2 and the aperture correction factor as well as the beam size in Cols. 3 and 4. Normalized line ratios (Col. 5) are then calculated as: 
. The squared beam size needs to be taken into account, as explained in Solomon & Vanden Bout (2005).
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