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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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