Table 1.
General information about the sample.
| # | Name | RA, Dec | z | DL | Scale | Type | log(M*) | log(MBH) | log(LAGN) |
|---|---|---|---|---|---|---|---|---|---|
| hh:mm:ss.ss dd:mm:ss.ss | Mpc | pc/″ | M⊙ | M⊙ | erg s−1 | ||||
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
| 1 | NGC 6860 | 20:08:46.89 −61:05:59.77 | 0.01477 | 64.0 | 301 | 1.5 | 10.3 | 7.3–8.3 | 43.6–43.8 |
| 2 | Mrk 915 | 22:36:46.50 −12:32:42.80 | 0.02415 | 105 | 487 | 1.5/1.9 | 10.0 | 7.3–8.4 | 44.1–44.3 |
| 3 | MCG -01-24-012 | 09:20:46.26 −08:03:21.97 | 0.01972 | 85.7 | 400 | 1.9/2 | 9.64 | 7.2 ± 0.3 | 44.3–44.8 |
Notes. This is a reproduction of Table 1 from Paper I, where the literature references for the last four columns are listed. (1) Source ID (for reference); (2) Galaxy name; (3) RA and DEC coordinates of the ALMA millimeter continuum peak (in the ICRS frame); (4) Redshift, corresponding to the systemic velocity (in the LSRK frame) of the disk model fit to the data (see Sect. D); (5) Luminosity distance; (6) Angular scale; (7) Seyfert type; (8) AGN total luminosity; (9) Stellar mass; (10) Black Hole mass; The range of values in MBH and LAGN arises from the different measurements that we collected from the literature, with the exceptions calculated by us described below in the notes. In particular for LAGN, the ranges are partly due to an observed intrinsic X-Ray variability.
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