Table 3.
ALMA and NOEMA CO(2–1) observations.
| Galaxy | Beam | PAbeam | Pixel | Instrument & Prog ID | PI | Ref | CO(2–1) |
|---|---|---|---|---|---|---|---|
| (″ × ″) | (deg) | (″) | Ring/Mini-spiral? | ||||
| IC 4518W | 0.23 × 0.20 | −86 | 0.025 | ALMA#2017.1.00255.S | Pereira-Santaella | This work | Perturbed |
| Mrk 1066 | 0.44 × 0.40 | 40 | 0.075 | NOEMA W14CB | Alonso-Herrero | 1 | Yes |
| NGC 1365 | 0.25 × 0.22 | 71 | 0.05 | ALMA#2013.1.01161.S | Sakamoto | This work | Yes |
| NGC 1386 | 0.62 × 0.45 | 85 | 0.1 | ALMA#2012.1.00474.S | Nagar | 2 | Yes? |
| NGC 1808 | 1.14 × 0.84 | 87 | 0.15 | ALMA#2017.1.00984.S | Salak | This work | Yes |
| NGC 2273 | 0.72 × 0.58 | 32 | 0.13 | NOEMA W14CB | Alonso-Herrero | 1 | Yes |
| NGC 3081 | 0.57 × 0.49 | 83 | 0.1 | ALMA#2015.1.00086.S | Nagar | 2 | Yes |
| NGC 3227 | 0.21 × 0.16 | 42 | 0.025 | ALMA#2016.1.00254.S | Alonso-Herrero | 3 | Yes |
| NGC 4253 | 0.55 × 0.30 | 22 | 0.071 | NOEMA WP16BP | Alonso-Herrero | 1 | Yes |
| NGC 4388 | 0.84 × 0.36 | 21 | 0.071 | NOEMA W14CB | Alonso-Herrero | 1 | ? |
| NGC 5135 | 0.31 × 0.22 | 63 | 0.05 | ALMA#2013.1.00243.S | Colina | 4 | Yes |
| NGC 5643 | 0.26 × 0.16 | −70 | 0.04 | ALMA#2016.1.00254.S | Alonso-Herrero | 5 | Yes |
| NGC 7130 | 0.30 × 0.25 | 62 | 0.025 | ALMA#2017.1.00255.S | Pereira-Santaella | This work | Yes |
| NGC 7172 | 0.56 × 0.44 | 76 | 0.1 | ALMA#2015.1.00116.S | Kohno | This work | ? |
| NGC 7213 | 0.61 × 0.58 | 79 | 0.12 | ALMA#2012.1.00474.S | Nagar | 2 | Yes |
| NGC 7465 | 0.59 × 0.30 | 23 | 0.071 | NOEMA WP16BP | Alonso-Herrero | 1 | No |
| NGC 7469 | 0.23 × 0.18 | −39 | 0.04 | ALMA#2017.1.00395.S | Díaz-Santos | This work | Yes |
| NGC 7582 | 0.17 × 0.16 | −16 | 0.04 | ALMA#2016.1.00254.S | Alonso-Herrero | This work | Yes |
Notes. Beam and PAbeam are the synthesized beam sizes and position angles of the CO(2–1) observations, respectively. “Pixel” refers to the pixel size of the CO(2–1) flux images. The “Ref.” column lists references of previously published works using the same dataset. The last column indicates whether a ring or a mini-spiral is detected in CO(2–1) in the central ∼4″ × 4″.
References. 1. Domínguez-Fernández et al. (2020), 2. Ramakrishnan et al. (2019), 3. Alonso-Herrero et al. (2019), 4. Sabatini et al. (2018), 5. Alonso-Herrero et al. (2018).
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