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Table 3
Summary of CO lines detections and setups.
| Line | Freq | Array | Beam size | Beam PA | CO integrated intensity | Noise level |
|---|---|---|---|---|---|---|
| (GHz) | (″) | (°) | (Jy km s−1) | (mJy beam−1 km s−1) | ||
| 13CO J = 1 → 0 | 110.201 | ALMA | 0.70 × 0.51 | 58 | 0.16 ± 0.03 | 6.8 |
| C18O J = 1 → 0 | 109.782 | ALMA | 0.70 × 0.51 | 58 | <0.05 | |
| 12CO J = 1 → 0 | 115.271 | CARMA (b) | 4.8 × 4.1 | 29 | 1.6 ± 0.2 (b) | |
| 13CO J = 2 → 1 | 220.399 | NOEMA | 2.30 × 1.20 | −172 | 1.2 ± 0.2 | 23 |
| C18O J = 2 → 1 | 219.560 | NOEMA | 2.30 × 1.20 | −172 | < 0.10 | |
| 12CO J = 2 → 1 | 230.538 | NOEMA | 2.40 × 1.20 | 11 | 10 ± 1 | 31 |
| 12CO J = 3 → 2 | 345.796 | ALMA (a) | 0.43 × 0.33 | −58 | 18.4 ± 0.3 (a) | 40 |
Notes. (a) Archival data from project ALMA.1.00698.S. For non detections, we provide 3σ upper limits.
References. (b)From Flaherty et al. (2016).
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