Table 1.
Integrated line fluxes before magnification correction.
| Line | Telescope/ | Line width | Flux density |
|---|---|---|---|
| Instrument | km s−1 | Jy km s−1 | |
| 12CO(9-8)a | APEX/nFLASH | 550 | 2.1 ± 4.3 |
| 12CO(9-8)b | ALMA | 550 | 2.0 ± 1.5 |
| 12CO(6-5) | ALMA/ACA | 603 ± 60 | 6.6 ± 1.1 |
| 12CO(4-3) | ALMA/ACA | 543 ± 90 | 5.7 ± 1.0 |
| 12CO(4-3) | LMT/RSR | 580 ± 97 | 4.0 ± 0.5 |
| 12CO(4-3)c | NRO | 625 ± 120 | 6.5 ± 0.7 |
| 12CO(2-1)c | ATCA | 543 ± 106 | 3.0 ± 0.5 |
| [CI] | LMT/RSR | 362 ± 135 | 1.0 ± 0.3 |
| [CI] | ALMA/ACA | 340 ± 113 | 2.9 ± 1.0 |
| [CII]d | APEX/nFLASH | 598 ± 85 | 71.5 ± 15.4 |
| H2O+(202−111)(3/2−1/2) | ALMA/ACA | 230 ± 116 | 4.3 ± 1.0 |
| H2O+(211−202)(3/2−3/2) | ALMA/ACA | 548 ± 110 | 7.5 ± 1.6 |
| HCN(4-3) | LMT/RSR | 502 ± 126 | 1.0 ± 0.3 |
Notes. aValue obtained by forcing a measurement in the spectra, assuming a line velocity of 550 km s−1.
bFlux derived from ALMA spectra in which only half of the line is covered. A conservative 75% error is assigned to the value.
cMeasurements from Tamura et al. (2025).
dThe provided flux corresponds to the median spectrum; the measurements for the three independent spectra are consistent within the errors.
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