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Table 1.
Log of the ALMA observations used in this work.
| ID | Date | texp | Noise RMS | Beam | Program | Band | Line |
|---|---|---|---|---|---|---|---|
| (min) | mJy/beam | (arcsec) | |||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) |
| J1448 | 02 Nov. 2024 | 9 | 0.082 | 1.03 × 0.91 | 2024.1.00061.S | 7 | CO(5–4) |
| 12 Mar. 2018 | 100 | 0.010 | 1.31 × 0.89 | 2017.1.01109.S | 4 | CO(2–1) | |
| 19 Mar. 2019 | 45 | 0.023 | 1.26 × 1.12 | 2018.1.01264.S | 7 | CO(4–3) | |
| 29 Mar. 2019 | 150 | 0.011 | 2.22 × 2.03 | 2018.1.01264.S | 4 | CO(2–1) | |
| J2258 | 06 Nov. 2024 | 8 | 0.083 | 1.17 × 0.86 | 2024.1.00061.S | 7 | CO(5–4) |
| 01 May 2018 | 100 | 0.009 | 2.34 × 1.99 | 2017.1.01109.S | 4 | CO(2–1) | |
| 18 May 2021 | 79 | 0.008 | 0.54 × 0.48 | 2019.1.00221.S | 4 | CO(2–1) | |
| ID83492 | 29 Oct. 2024 | 49 | 0.019 | 1.22 × 1.15 | 2024.1.00061.S | 6 | CO(5–4) |
| 09 Jan. 2020 | 34 | 0.011 | 1.90 × 1.30 | 2019.1.00900.S | 4 | CO(3–2) | |
| J1109 | 07 Dec. 2024 | 16 | 0.061 | 0.91 × 0.80 | 2024.1.00061.S | 7 | CO(5–4) |
| 10 Apr. 2018 | 99 | 0.012 | 1.85 × 1.57 | 2017.1.01109.S | 4 | CO(2–1) | |
| 19 Mar. 2020 | 49 | 0.010 | 0.96 × 0.70 | 2019.1.00221.S | 4 | CO(2–1) | |
| J1302 | 31 Oct. 2024 | 17 | 0.066 | 1.08 × 0.86 | 2024.1.00061.S | 7 | CO(5–4) |
| 21 Mar. 2018 | 100 | 0.013 | 1.07 × 0.98 | 2017.1.01109.S | 4 | CO(2–1) | |
| J0912 | 25 Oct. 2024 | 12 | 0.062 | 1.19 × 0.87 | 2024.1.00061.S | 7 | CO(5–4) |
| 08 Jan. 2017 | 98 | 0.013 | 2.39 × 1.91 | 2016.1.01126.S | 4 | CO(2–1) | |
| 24 Dec. 2018 | 50 | 0.013 | 0.91 × 0.72 | 2018.1.01240.S | 6 | CO(4–3) | |
| 23 Mar. 2021 | 147 | 0.012 | 0.78 × 0.71 | 2019.1.00221.S | 4 | CO(2–1) | |
| J2202 | 21 Oct. 2024 | 46 | 0.034 | 0.82 × 0.78 | 2024.1.00061.S | 7 | CO(5–4) |
| 07 Mar. 2017 | 95 | 0.015 | 3.06 × 2.16 | 2016.1.01126.S | 4 | CO(2–1) | |
| ID97148 | 19 Nov. 2024 | 110 | 0.026 | 1.39 × 1.09 | 2024.1.00061.S | 7 | CO(5–4) |
| 09 Jan. 2020 | 49 | 0.010 | 1.60 × 1.30 | 2019.1.00900.S | 4 | CO(3–2) |
Notes. Columns: (1) Galaxy ID; (2) Date of observations; (3) Integration time on source; (4) Continuum noise rms; (5) FWHM of the beam; (6) Program ID; (7) ALMA band used for the observations; (8) Targeted emission line.
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