Table 1.
VERTICO subsample of low-inclination (i ≤ 80°) galaxies.
| Galaxy | RA | Dec | i | PA | log10 SFR | log10 M* | defHI M* |
|---|---|---|---|---|---|---|---|
| (hh:mm:ss) | (dd:mm:ss) | (°) | (°) | (M⊙ yr−1) | (M⊙) | (dex) | |
| IC3392 | 12:28:43 | +14:59:57 | 68 | 219 | −1.30 | 9.51 | 1.50 |
| NGC4064 | 12:04:11 | +18:26:39 | 70 | 150 | −1.07 | 9.47 | 1.50  |
| NGC4189 | 12:13:47 | +13:25:35 | 42 | 70 | −0.33 | 9.75 | 0.63  |
| NGC4254 | 12:18:50 | +14:25:06 | 39 | 243 | 0.70 | 10.52 | −0.03  |
| NGC4293 | 12:21:13 | +18:23:03 | 67 | 239 | −0.27 | 10.50 | 2.16  |
| NGC4294 | 12:21:18 | +11:30:39 | 74 | 151 | −0.39 | 9.38 | 0.18  |
| NGC4298 | 12:21:33 | +14:36:20 | 52 | 132 | −0.26 | 10.11 | 0.68  |
| NGC4299 | 12:21:41 | +11:30:06 | 14 | 128 | −0.34 | 9.06 | −0.72  |
| NGC4321 | 12:22:55 | +15:49:33 | 32 | 280 | 0.54 | 10.71 | 0.36  |
| NGC4351 | 12:24:01 | +12:12:15 | 48 | 251 | −0.91 | 9.37 | 0.55  |
| NGC4380 | 12:25:22 | +10:01:00 | 61 | 158 | −0.77 | 10.11 | 1.27  |
| NGC4383 | 12:25:25 | +16:28:12 | 56 | 17 | 0.01 | 9.44 | −0.39  |
| NGC4394 | 12:25:56 | +18:12:52 | 32 | 312 | −0.79 | 10.34 | 0.90  |
| NGC4405 | 12:26:07 | +16:10:52 | 46 | 18 | −0.88 | 9.75 | 1.73  |
| NGC4419 | 12:26:56 | +15:02:51 | 74 | 131 | −0.12 | 10.06 | 1.65  |
| NGC4424 | 12:27:12 | +09:25:14 | 61 | 274 | −0.52 | 9.89 | 1.14  |
| NGC4450 | 12:28:29 | +17:05:05 | 51 | 170 | −0.55 | 10.70 | 1.35  |
| NGC4457 | 12:28:59 | +03:34:14 | 37 | 256 | −0.49 | 10.42 | 1.29  |
| NGC4501 | 12:31:59 | +14:25:11 | 65 | 320 | 0.43 | 11.00 | 0.80  |
| NGC4532 | 12:34:19 | +06:28:06 | 64 | 159 | −0.16 | 9.25 | −0.25  |
| NGC4535 | 12:34:20 | +08:11:54 | 48 | 12 | 0.31 | 10.49 | 0.07  |
| NGC4536 | 12:34:27 | +02:11:16 | 74 | 118 | 0.47 | 10.19 | −0.26  |
| NGC4548 | 12:35:27 | +14:29:44 | 37 | 318 | −0.28 | 10.65 | 0.96  |
| NGC4561 | 12:36:08 | +19:19:22 | 28 | 60 | −0.64 | 9.09 | −0.64  |
| NGC4567 | 12:36:33 | +11:15:29 | 49 | 251 | 0.03 | 10.25 | −0.27  |
| NGC4568 | 12:36:34 | +11:14:22 | 70 | 211 | 0.29 | 10.47 | 0.40  |
| NGC4569 | 12:36:50 | +13:09:55 | 69 | 203 | 0.16 | 10.86 | 1.12  |
| NGC4579 | 12:37:43 | +11:49:06 | 40 | 273 | 0.08 | 10.92 | 1.20  |
| NGC4580 | 12:37:48 | +05:22:06 | 46 | 337 | −0.90 | 9.94 | 1.99  |
| NGC4606 | 12:40:58 | +11:54:44 | 69 | 38 | −1.33 | 9.61 | 1.86  |
| NGC4651 | 12:43:43 | +16:23:38 | 53 | 75 | −0.10 | 10.31 | 0.09  |
| NGC4654 | 12:43:57 | +13:07:33 | 61 | 300 | 0.31 | 10.26 | −0.01  |
| NGC4694 | 12:48:15 | +10:59:01 | 62 | 323 | −0.85 | 9.94 | 1.03  |
| NGC4698 | 12:48:23 | +08:29:15 | 66 | 347 | −0.83 | 10.49 | 0.37  |
| NGC4713 | 12:49:58 | +05:18:40 | 45 | 89 | −0.20 | 9.31 | −0.42  |
| NGC4772 | 12:53:29 | +02:10:06 | 60 | 325 | −1.08 | 10.18 | 0.48  |
| NGC4808 | 12:55:49 | +04:18:15 | 72 | 127 | −0.19 | 9.63 | −0.27  |
Notes. The right ascension and declination of the galaxies optical centers are taken from the NASA/IPAC Extragalactic Database (https://ned.ipac.caltech.edu/). The orientation parameters (optical inclinations and position angles) are drawn from Brown et al. (2021), and are calculated using fits to SDSS photometry. The average star formation rates and integrated stellar mass are adopted from Leroy et al. (2019). HI deficiencies are adopted from Zabel et al. (2022), and are calculated using the predicted HI mass from field galaxies at fixed stellar mass.
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