Table 2.
Description of the ALMA observations and datasets of the ALPAKA sample.
| ID | Project ID | Line | Frequency Range | Beam | Channel Width | RMS | Integration time |
|---|---|---|---|---|---|---|---|
| (GHz) | (“×”) | (km s−1) | (mJy beam−1) | (h) | |||
| 1 | 2017.1.01659.S | CO(2-1) | 146.72–148.59 | 0.49 × 0.39 | 39 | 0.056 | 10.48 |
| 2 | 2016.1.00624.S | CO(3-2) | 212.07–231.00 | 0.20 × 0.16 | 32 | 0.23 | 0.72 |
| 3 | 2016.1.01426.S | CO(5-4) | 217.00–236.54 | 0.14 × 0.10 | 30 | 0.12 | 1.5 |
| 4 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.50 × 0.34 | 25 | 0.096 | 12.8 |
| 5 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.50 × 0.34 | 25 | 0.094 | 12.8 |
| 6 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.50 × 0.34 | 25 | 0.1 | 12.8 |
| 7 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.50 × 0.35 | 25 | 0.1 | 12.8 |
| 8 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.50 × 0.34 | 25 | 0.1 | 12.8 |
| 9 | 2017.1.00471.S | CO(2-1) | 92.06–93.93 | 0.51 × 0.35 | 25 | 0.1 | 12.8 |
| 10 | 2017.1.01674.S | CO(2-1) | 91.42–106.72 | 0.30 × 0.28 | 25 | 0.069 | 3.65 |
| 2015.1.00862.S | CO(2-1) | 91.77–107.49 | comb. | comb. | comb. | 2.49 | |
| 11 | 2017.1.01228.S | CO(2-1) | 85.90–101.81 | 0.53 × 0.42 | 26 | 0.1 | 2.69 |
| 12 | 2018.1.00974.S | CO(2-1) | 86.72–102.53 | 0.39 × 0.30 | 39 | 0.1 | 2.91 |
| 13 | 2017.1.00413.S | [CI](3P2 − 3P1) | 243.03–261.99 | 0.19 × 0.16 | 18 | 0.15 | 1.09 |
| 14 | 2019.1.01362.S | CO(4-3) | 140.58–156.27 | 0.18 × 0.17 | 16 | 0.043 | 13.82 |
| 2017.1.01045.S | CO(4-3) | 140.80–156.38 | comb. | comb. | comb. | 3.89 | |
| 2013.1.00059.S | CO(4-3) | 140.48–156.10 | comb. | comb. | comb. | 1.56 | |
| 15 | 2018.1.00543.S | CO(3-2) | 92.34–108.18 | 0.28 × 0.23 | 32 | 0.058 | 5.95 |
| 16 | 2015.1.00723.S | CO(7-6) | 226.21–245.50 | 0.22 × 0.20 | 19 | 0.11 | 2.55 |
| 17 | 2015.1.00723.S | CO(7-6) | 226.21–245.50 | 0.22 × 0.20 | 19 | 0.11 | 2.55 |
| 18 | 2018.1.01146.S | [CI](3P1 − 3P0) | 86.51–102.39 | 0.25 × 0.19 | 32 | 0.082 | 1.33 |
| 19 | 2016.1.01155.S | CO(3-2) | 85.75–100.61 | 0.35 × 0.29 | 35 | 0.12 | 3.32 |
| 20 | 2016.1.01155.S | CO(3-2) | 85.75–100.61 | 0.35 × 0.29 | 35 | 0.12 | 3.32 |
| 21 | 2016.1.01155.S | CO(3-2) | 85.75–100.61 | 0.36 × 0.30 | 35 | 0.13 | 3.32 |
| 22 | 2017.1.01677.S | CO(5-4) | 133.53–149.39 | 0.19 × 0.16 | 32 | 0.13 | 2.31 |
| 23 | 2018.1.01306.S | CO(3-2) | 84.09–99.78 | 0.24 × 0.20 | 28 | 0.069 | 5.71 |
| 24 | 2018.1.01306.S | CO(3-2) | 84.09–99.78 | 0.24 × 0.20 | 28 | 0.075 | 5.71 |
| 25 | 2018.1.01306.S | CO(3-2) | 84.09–99.78 | 0.24 × 0.20 | 28 | 0.074 | 5.71 |
| 26 | 2017.1.01677.S | CO(5-4) | 129.50–144.99 | 0.28 × 0.21 | 35 | 0.11 | 3.40 |
| 27 | 2017.1.01677.S | CO(5-4) | 129.50–144.99 | 0.29 × 0.21 | 36 | 0.12 | 3.40 |
| 28 | 2017.1.00908.S | CO(6-5) | 135.76–151.74 | 0.18 × 0.15 | 31 | 0.06 | 3.61 |
Notes. For targets ID4 – 9, the observation consists of three mosaic pointings; the corresponding on-source integration time refers to the total value summed over all pointings. For targets with multiple observations (i.e., ID10 and 14), we image the CO after combining the corresponding measurement sets and we list the resulting properties of the cubes (beam, channel width, RMS).
Here, we provide the list of principal investigators (PIs) for the ALMA projects employed in this work: 2017.1.01659.S, Chemin, L.; 2016.1.00624.S, Freundlich, J.; 2017.1.00471.S, Hayashi, M.; 2017.1.01674.S, Molina, J.; 2015.1.00862.S, Ibar, E.; 2017.1.01228.S, Noble, A.; 2018.1.00974.S, Noble, A.; 2017.1.00413.S, Barro, G.; 2019.1.01362.S, Herrera-Camus, R.; 2017.1.01045.S, Brisbin, D.; 2013.1.00059.S, Aravena, M.; 2018.1.00543.S, Herrera-Camus, R.; 2015.1.00723.S, Oteo, I.; 2018.1.01146.S, Nagar, N.; 2016.1.01155.S, Wang, T.; 2017.1.01677.S, Cassata, P.; 2018.1.01306.S, Umehata, H.; 2017.1.00908.S, Assef, R.
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