Table A.1.
Observational properties of the CO sample.
| Name |
 |
 |
D(b) | log |
λEdd (d) | Hubble & AGN type(e) | Hubble stage T(e) | PA(f) | i(f) |
|---|---|---|---|---|---|---|---|---|---|
| —- | hms | ° ′ ″ | Mpc | erg s−1 | —- | —- | —- | o | o |
| AGN sample: CO(3-2) | |||||||||
| NGC1566 | 04:20:00.395 | -54:56:16.60 | 7.2 | 40.50 | -2.89 | (R’1)SAB(rs)bc; Sy1.5 | 4.0 | 44 | 49 |
| NGC1808 | 05:07:42.329 | -37:30:45.85 | 9.3 | 39.80 | -4.51 | (R’1)SAB(s:)b; Sy2 | 1.2 | 146 | 83 |
| NGC1672 | 04:45:42.496 | -59:14:49.92 | 11.4 | 39.10 | -6.41 | (R’1)SB(r)bc; Sy2 | 3.3 | 155 | 29 |
| NGC1068 | 02:42:40.709 | -00:00:47.94 | 14.0 | 42.82 | -0.70 | (R)SA(rs)b; Sy2 | 3.0 | 289 | 41 |
| NGC6300 | 17:16:59.543. | -62:49:14.04 | 14.0 | 41.73 | -1.72 | SB(rs)b Sy2 | 3.1 | 95 | 57 |
| NGC1326 | 03:23:56.416 | -36:27:52.68 | 14.9 | 39.90 | -4.02 | (R1)SB(rl)0/a; LINER | -0.7 | 71 | 53 |
| NGC5643 | 14:32:40.699 | -44:10:27.93 | 16.9 | 42.41 | -1.23 | SAB(rs)c; Sy2 | 5.0 | 301 | 30 |
| NGC613 | 01:34:18.189 | -29:25:06.59 | 17.2 | 41.20 | -3.48 | SB(rs)bc; HII Sy | 4.0 | 122 | 36 |
| NGC7314 | 22:35:46.201 | -26:03:01.58 | 17.4 | 42.18 | -2.07 | SAB(rs)bc; Sy1.9 | 4.0 | 191 | 55 |
| NGC4388 | 12:25:46.781 | +12:39:43.75 | 18.1 | 42.45 | -1.07 | SA(s)b: sp; Sy2 Sy1.9 | 2.8 | 82 | 79 |
| NGC1365 | 03:33:36.369 | -36:08:25.50 | 18.3 | 42.09 | -2.15 | (R’)SBb(s)b; HII Sy1.8 | 3.2 | 40 | 41 |
| NGC4941 | 13:04:13.103 | -05:33:05.73 | 20.5 | 41.40 | -2.10 | (R)SAB(r)ab:; Sy2 | 2.1 | 212 | 41 |
| NGC7213 | 22:09:16.209 | -47:10:00.12 | 22.0 | 41.85 | -3.01 | SA(s)a:; LINER Sy1.5 | 0.9 | 133 | 35 |
| NGC7582 | 23:18:23.643 | -42:22:13.54 | 22.5 | 43.49 | -1.70 | (R’1)SB(s)ab; Sy2 | 2.1 | 344 | 59 |
| NGC6814 | 19:42:40.587 | -10:19:25.10 | 22.8 | 42.24 | -1.62 | SAB(rs)bc; HII Sy1.5 | 4.0 | 84 | 57 |
| NGC3227 | 10:23:30.577 | +19:51:54.28 | 23.0 | 42.37 | -1.20 | SAB(s) pec; Sy1.5 | 1.5 | 152 | 52 |
| NGC5506 | 14:13:14.878 | -03:12:27.66 | 26.4 | 42.98 | -1.22 | Sa pec sp ; Sy1.9 | 1.2 | 275 | 80 |
| NGC7465 | 23:02:00.961 | +15:57:53.21 | 27.2 | 41.93 | -2.10 | (R’)SB(s)0; Sy2 | -1.8 | 66 | 54.5 |
| NGC7172 | 22:02:01.891 | -31:52:10.48 | 37.0 | 42.84 | -1.60 | Sa pec sp; Sy2 HII | 0.6 | 92 | 85 |
| NGC5728 | 14:42:23.872 | -17:15:11.01 | 44.5 | 43.19 | -1.72 | (R1)SAB(r)a; HII Sy2 | 1.2 | 15 | 59 |
| AGN sample: CO(2-1) | |||||||||
| NGC4826 | 12:56:43.643 | +21:40:59.30 | 4.4 | 37.78 | -6.66 | (R)SA(rs)ab; HII Sy2 | 2.2 | 112 | 60 |
| NGC5236 | 13:37:00.94 | -29:51:56.16 | 4.9 | 38.70 | —- | SAB(s)c; HII Sbrst | 5.0 | 225 | 24 |
| NGC2903 | 09:32:10.10 | +21:30:02.88 | 10.0 | 38.00 | -6.62 | SAB(rs)bc; HII | 4.0 | 204 | 67 |
| NGC3351 | 10:43:57.731 | +11:42:13.35 | 10.0 | 38.03 | -6.75 | SB(r)b; HII Sbrst | 3.1 | 193 | 45 |
| NGC1637 | 04:41:28.10 | -02:51:28.80 | 11.7 | 38.04 | —- | SAB(rs)c; AGN | 5.0 | 21 | 31 |
| NGC4501 | 12:31:59.220 | 14:25:12.69 | 14.0 | 39.68 | -5.78 | SAb -SA(rs)b; HII Sy2 | 3.3 | 135 | 59 |
| NGC4438 | 12:27:45.675 | 13:00:31.18 | 16.5 | 38.72 | -6.35 | SA(s)0/a pec:; LINER | 2.8 | 30 | 60 |
| NGC4569 | 12:36:49.80 | +13:09:46.30 | 16.8 | 39.60 | -5.50 | SAB(rs)ab; LINER Sy | 2.4 | 23 | 70 |
| NGC4579 | 12:37:43.58 | +11:49:02.49 | 16.8 | 41.42 | -3.82 | SAB(rs)b; LINER Sy1.9 | 2.8 | 95 | 36 |
| NGC3718 | 11:32:34.880 | +53:04:04.32 | 17.0 | 40.64 | -4.64 | SB(s)a pec; Sy1 LINER | 1.1 | . 120 | 60 |
| NGC3368 | 10: 46:45.50 | 11:49:12.00 | 18.0 | 39.30 | -5.53 | SABab SAB(rs)ab;Sy LINER | 2.1 | 165 | 60 |
| NGC2110 | 05:52:11.377 | -07:27:22.48 | 34.8 | 42.67 | -1.87 | SAB0-; Sy2 | -3.0 | 175 | 46 |
| NGC2782 | 09:14:05.111 | 40:06:49.24. | 35.0 | 39.50 | -6.10 | SAB(rs)a; Sy1 Sbrst | 1.1 | 75 | 20 |
| NGC7172 | 22:02:01.891 | -31:52:10.48 | 37.0 | 42.84 | -1.60 | Sa pec sp; Sy2 HII | 0.6 | 92 | 85 |
| MCG-06-30-15 | 13:35:53.770 | -34:17:44.16 | 38.3 | 42.86 | -1.28 | S?; Sy1.2 | 2.0 | 116 | 59 |
| NGC2992 | 09:45:41.943 | -14:19:34.57 | 39.2 | 42.20 | -2.29 | Sa pec; Sy1.9 | 0.9 | 29 | 80 |
| NGC3081 | 09:59:29.546 | -22:49:34.78 | 40.3 | 43.10 | -1.47 | ( R1)SAB(r)0/a; Sy2 | 0.0 | 71 | 60 |
| ESO137-34 | 16:35:13.996 | -58:04:47.77 | 41.5 | 42.80 | -1.99 | SAB(s)0/a? Sy2 | 0.6 | 18 | 41 |
| NGC5728 | 14:42:23.872 | -17:15:11.01 | 44.5 | 43.19 | -1.72 | (R1)SAB(r)a; HII Sy2 | 1.2 | 15 | 59 |
| ESO21-g004 | 13:32:40.621 | -77:50:40.40 | 45.1 | 42.32 | —- | SA(s)0/a: | 0.20 | 100 | 65 |
| AGN sample: CO(1-0) | |||||||||
| M51 | 13:29:52.68 | +47:11:42.72 | 8.6 | 39.00 | -5.25 | SA(s)bc pec; HII Sy2.5 | 4.0 | 173 | 21 |
| NGC6300 | 17:16:59.543. | -62:49:14.04 | 14.0 | 41.73 | -1.72 | SB(rs)b Sy2 | 3.1 | 95 | 57 |
| NGC4321 | 12:22:54.954 | +15:49:20.49 | 16.8 | 40.40 | -3.80 | SAB(s)bc; LINER HII | 4.0 | 153 | 32 |
| NGC5643 | 14:32:40.699 | -44:10:27.93 | 16.9 | 42.41 | -1.23 | SAB(rs)c; Sy2 | 5.0 | 301 | 30 |
| NGC7314 | 22:35:46.201 | -26:03:01.58 | 17.4 | 42.18 | -2.07 | SAB(rs)bc; Sy1.9 | 4.0 | 191 | 55 |
| NGC4388 | 12:25:46.781 | +12:39:43.75 | 18.1 | 42.45 | -1.07 | SA(s)b: sp; Sy2 Sy1.9 | 2.8 | 82 | 79 |
| NGC6221 | 16:52:46.346 | -59:13:01.08 | 22.9 | 41.26 | -2.90 | Sb: pec ; HII LIRG | 3.1 | 1 | 51 |
| NGC3227 | 10:23:30.577 | +19:51:54.28 | 23.0 | 42.37 | -1.20 | SAB(s) pec; Sy1.5 | 1.5 | 152 | 52 |
| NGC4180 | 12:13:03.072 | +07:02:19.95 | 36.0 | 42.08 | —- | Sab:; Sy LINER | 2.0 | 21 | 80 |
| NGC7172 | 22:02:01.891 | -31:52:10.48 | 37.0 | 42.84 | -1.60 | Sa pec sp; Sy2 HII | 0.6 | 92 | 85 |
| NGC4593 | 12:39:39.444 | -05:20:39.03 | 41.8 | 43.02 | -0.98 | (R)SB(rs)b Sy1 | 3.0 | 38 | 33 |
| NGC1125 | 02:51:40.459 | -16:39:02.34 | 42.6 | 42.65 | -2.15 | (R’)SAB(rl:)0+; Sy2 | 0.0 | 54 | 75 |
| NGC5728 | 14:42:23.872 | -17:15:11.01 | 44.5 | 43.19 | -1.72 | (R1)SAB(r)a; HII Sy2 | 1.2 | 15 | 59 |
| NGC3281 | 10:31:52.082 | -34:51:13.38 | 52.0 | 43.22 | -2.06 | SAB(rs+)a; Sy2 | 2.4 | 140 | 60 |
| nonAGN sample: CO(2-1) | |||||||||
| NGC5068 | 13:18:54.700 | -21:02:19.32 | 5.2 | —- | —- | SB(s)d | 6.0 | 342 | 36 |
| NGC3621 | 11:18:16.296 | - 32:48:45.36 | 7.1 | —- | —- | SA(s)d; HII | 6.9 | 344 | 66 |
| IC5332 | 23:34:27.480 | -36:06:03.9 | 9.0 | —- | —- | SA(s)d | 6.8 | 74 | 27 |
| NGC3596 | 11:15:06.100 | +14:47:13.56 | 11.3 | —- | —- | SAB(rs)c; HII | 5.2 | 169 | 15 |
| NGC4781 | 12:54:23.800 | -10:32:13.56 | 11.3 | —- | —- | SB(rs)d; HII | 7.0 | 290 | 59 |
| NGC2835 | 09:17:52.800 | -22:21:16.92 | 12.2 | —- | —- | SAB(rs)c; HII | 5.0 | 1 | 41 |
| NGC5530 | 14:18:27.300 | -43:23:17.88 | 12.3 | —- | —- | SA(rs)bc | 4.2 | 305 | 62 |
| NGC1947 | 05:26:47.545 | -63:45:35.82 | 17.2 | —- | —- | S0- pec; LINER | -2.8 | 119 | 29 |
| NGC1079 | 02:43:44.337 | -29:00:11.75 | 18.9 | —- | —- | (R)SAB(rs)0/a pec | 0.6 | 90 | 56 |
| NGC3717 | 11:31:31.878 | -30:18:27.78 | 19.1 | —- | —- | SAb: sp; HII | 3.1 | 32 | 79 |
| NGC7727 | 23:39:53.804 | -12:17:34.18 | 21.0 | —- | —- | SAB(s)a pec | 1.1 | 0 | 26 |
| NGC5921 | 15:21:56.487 | +05:04:14.27 | 21 | —- | —- | SB(r)bc; LINER | 4.0 | 140 | 50 |
| NGC3175 | 10:14:42.111 | -28:52:19.42 | 21.0 | —- | —- | SAB(s)b; HII | 2.0 | 55 | 76 |
| NGC718 | 01:53:13.282 | +04:11:44.93 | 21.4 | —- | —- | SAB(s)a | 1.0 | 150 | 50 |
| NGC5845 | 15:06:00.787 | +01:38:01.77 | 27.0 | —- | —- | E | -4.9 | 153 | 50 |
| ESO-093-g003 | 10:59:26.062 | -66:19:58.31 | 29.8 | —- | —- | SAB(r)0/a? | 0.3 | 145 | 66 |
| NGC5037 | 13:14:59.357 | -16:35:24.99 | 35.0 | —- | —- | SA(s)a | 1.2 | 44 | 74 |
| NGC3749 | 11:35:53.192 | -37:59:50.90 | 41.0 | —- | —- | SA(s)a pec sp; HII | 1.1 | 109 | 65 |
| NGC4224 | 12:16:33.782 | +07:27:43.54 | 41.0 | —- | —- | SA(s)cd: sp; HII | 6.0 | 56 | 59 |
Notes. (a) Positions of the AGN continuum sources derived from the ALMA and PdBI CO mages taken from the references listed in Sect. 3. (b) Median value of redshift-independent distances taken from the Nasa Extragalactic Database (NED). (c) Luminosities of hard X-rays in the 2-10 keV range are taken from Ricci et al. (2017b), Combes et al. (2019), García-Burillo et al. (2021) or redetermined in this work (see Appendix B); luminosities are intrinsic (corrected for absorption) and rescaled to the adopted distances. (d) Eddington ratios adopted from García-Burillo et al. (2021) and references therein, except for NGC 1068 where we used the most recent determination of the BH mass published by Gallimore & Impellizzeri (2023) and the bolometric AGN luminosity derived by the torus model of García-Burillo et al. (2014). (e) Hubble classification, stage type T-parameter, and AGN classification (when available) are taken from NED. (f) Position and inclination angles used in the deprojection of the images are taken from HyperLEDA or redetermined in this work using the software package kinemetry (Krajnović et al. 2006) for the galaxies published by García-Burillo et al. (2021).
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