Table C.2.
Details of the observations targeting the CO line emissions
| QSO | Obs freq | Beam cont | r.m.s. cont | line (spw:chans) | Beam line | r.m.s line | chan width | Project ID |
|---|---|---|---|---|---|---|---|---|
| (GHz) | [arcsec2] | [mJy/beam] | [arcsec2] | [mJy/beam] | [km s−1] | |||
| J0224-4711 | 95.33 | 3.95 × 2.32 | 0.016 | CO(7-6) (0/1:56-76)a | 3.53 × 2.07 | 0.14 | 43.7 | 2017.1.01472.S |
| [CI] (0/1:88-100)a | ||||||||
| J1319+0950 | 103.51 | 0.3 × 0.3 | 0.054 | CO(6-5) (0/1:100-141)a | 0.32 × 0.31 | 0.1 | 24 | 2018.1.01289.S |
| J2054-0005 | 92.26 | 0.42 × 0.32 | 0.006 | CO(6-5) (0/1:106-130)a | 0.39 × 0.30 | 0.1 | 24 | 2018.1.01289.S |
Notes. Columns: (1) Target QSO; (2) observed frequency of the observation; (3) clean beam of the continuum map; (4) r.m.s of the continuum map; (5) spw and channels of the detected emission lines; (6) clean beam of the continuum-subtracted cube; (7) r.m.s of the continuum-subtracted cube; (8) channel width of the continuum-subtracted cube; (9) project ID of the observation. a: spw 0 and spw 1 were combined since they covered almost the same spectral range and in order to maximize the S/N of the emission lines. (b): natural weighting. (c): Briggs weighting with robust = 0.5. (d): since the [CII] of J0110+2802 showed emission up to high-velocities (∼ 1000 km s−1), we combined the two spectral windows in the upper side band to ensure a reliable continuum subtraction.
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