Table 1
Properties of the simulations performed in this work.
| Run | Time |  |
Radiative tran.(a) | Lines v (b) | Post-processing type |
|---|---|---|---|---|---|
| 1 | 50 kyr | 2.5 × 10−17 s−1 | LTE | 215–230 GHz | Single-dish |
| 2(*) | 100 kyr | 2.5 × 10−17 s−1 | LTE | 215–230 GHz | Single-dish |
| 3 | 100 kyr | 2.5 × 10−18 s−1 | LTE | 215–230 GHz | Single-dish |
| 4 | 100 kyr | 2.5 × 10−17 s−1 | LTE | 215–230 GHz | ALMA-like |
| 5 | 100 kyr | 2.5 × 10−17 s−1 | LVG | 215–230 GHz | Single-dish |
| 6 | 100 kyr | 2.5 × 10−17 s−1 | LVG | 72–110 GHz | Single-dish |
| 7 | 50 kyr | variable | LTE | 215–230 GHz | Single-dish |
| 8 | 100 kyr | variable | LTE | 215–230 GHz | Single-dish |
Notes. Run 2, highlighted with the asterisk symbol, is the reference one.(a) Type of radiative transfer used to produce the synthetic observations.(b) Frequency coverage of the simulated molecular lines. 215-230 GHz indicates we use the DCO+ and H13CO+ (3–2) and the C18O (2–1) lines, whilst 72–110 GHz refers to the run using the lowest-J transitions.
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