Table 2.
Parameters of ALMA observations and adopted kinematics for analyses.
| ALMA observations |
Adopted kinematics |
||||||||
|---|---|---|---|---|---|---|---|---|---|
| ID | Galaxy | Beam (PA) | Resolution | Sensitivity |
 |
 |
PA | vsys | |
| (″ × ″ (°)) | (pc × pc) | (mJy beam−1) | (h:m:s) | (°:′:″) | (°) | (km s−1) | |||
| 1 | IRAS 17208−0014 | 0.35 × 0.32 (74) | 298 × 272 | 0.680 | 17:23:21.96 | −00:17:00.9 | 105 | 12 321 | |
| 2 | IRAS 09022−3615 | 0.33 × 0.28 (64) | 382 × 324 | 0.145 | 09:04:12.71 | −36:27:01.9 | 10 | 16 847 | |
| 3 | IRAS 13120−5453 | 0.36 × 0.32 (18) | 225 × 200 | 0.730 | 13:15:06.32 | −55:09:22.8 | 95 | 9037 | |
| 4 | IRAS F14378−3651 | 0.29 × 0.26 (66) | 388 × 347 | 0.194 | 14:40:59.01 | −37:04:31.9 | 30 | 19 143 | |
| 5 | IRAS F05189−2524 | 0.42 × 0.27 (81) | 343 × 220 | 0.244 | 05:21:01.40 | −25:21:45.3 | 90 | 12 257 | |
| 6 | IRAS F10565+2448 | 0.33 × 0.22 (−1) | 281 × 187 | 0.227 | 10:59:18.13 | +24:32:34.5 | 90 | 12 387 | |
| 7 | IRAS 19542+1110 | 0.34 × 0.29 (−53) | 423 × 360 | 0.175 | 19:56:35.78 | +11:19:05.0 | 45 | 17 678 | |
| 8 | ESO 148−IG002 | 0.40 × 0.31 (31) | 344 × 267 | 0.236 | 23:15:46.75 | −59:03:15.5 | 0 | 12 793 | |
| 9 | NGC 6240 | 0.32 × 0.26 (58) | 161 × 130 | 0.281 | 16:52:58.89 | +02:24:03.4 | 40 | 7129 | |
| 10 | IRAS F17138-1017 | 0.38 × 0.29 (−76) | 139 × 106 | 0.576 | 17:16:35.81 | −10:20:39.0 | 5 | 5113 | |
| 11 | IRAS 17578−0400 | 0.36 × 0.29 (−65) | 102 × 82 | 0.512 | 18:00:31.84 | −04:00:53.5 | 110 | 3981 | |
| 12 | ESO 173−G015 | 0.33 × 0.30 (−7) | 51 × 47 | 0.434 | 13:27:23.77 | −57:29:22.0 | 165 | 2963 | |
| 13 | UGC 11763 | 0.35 × 0.31 (51) | 397 × 351 | 0.206 | 21:32:27.82 | +10:08:19.2 | ⋯ | 17 859 | |
| 14 | NGC 3110 | 0.40 × 0.27 (56) | 142 × 96 | 0.384 | 10:04:02.09 | −06:28:29.5 | 170 | 4973 | |
| 15 | IC 4734 | 0.38 × 0.29 (28) | 126 × 96 | 0.525 | 18:38:25.70 | −57:29:25.2 | 105 | 4606 | |
| 16 | NGC 5135 | 0.33 × 0.27 (85) | 83 × 68 | 0.630 | 13:25:43.99 | −29:49:60.0 | 15 | 4052 | |
| 17 | ESO 221−IG10 | 0.34 × 0.31 (−57) | 95 × 87 | 0.582 | 13:50:56.94 | −49:03:19.2 | 40 | 3113 | |
| 18 | IC 5179 | 0.28 × 0.23 (68) | 63 × 52 | 0.391 | 22:16:09.13 | −36:50:37.0 | 50 | 3350 | |
| 19 | UGC 2982 | 0.36 × 0.30 (126) | 117 × 98 | 0.359 | 04:12:22.67 | +05:32:49.1 | ⋯ | 5200 | |
| 20 | NGC 2369 | 0.28 × 0.25 (7) | 59 × 53 | 0.511 | 07:16:37.68 | −62:20:36.6 | 50 | 3187 | |
| 21 | ESO 286−G035 | 0.29 × 0.26 (52) | 101 × 90 | 0.409 | 21:04:11.12 | −43:35:35.8 | 20 | 5129 | |
| 22 | ESO 320−G030 | 0.34 × 0.29 (69) | 62 × 53 | 0.453 | 11:53:11.72 | −39:07:49.1 | 130 | 3049 | |
| 23 | NGC 5734 | 0.31 × 0.30 (35) | 89 × 86 | 0.417 | 14:45:09.04 | −20:52:13.5 | 40 | 4029 | |
Notes. “Beam” refers to the synthesized beam obtained after cleaning with natural weighting. “Resolution” is the projected physical size corresponding to the synthesized beam at the distance of the galaxy. “Sensitivity” is 1σ rms per beam in 20 km s−1 velocity channels calculated from flux-free parts. The adopted galaxy kinematics were roughly estimated from the velocity field seen outside the most nuclear region. The systemic velocity vsys is given in radio convention with respect to the LSRK.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.