Notes. (1) Galaxy name; (2) RA and Dec coordinates of the ALMA millimeter continuum peak (in the ICRS frame); (3) Redshift, corresponding to the systemic velocity (in the LSRK frame); (4) Luminosity distance; (5) Angular scale; (6) Seyfert type; (7) AGN total luminosity; (8) Stellar mass; (9) Black hole mass; The range of values in M_BH and L_AGN 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 L_AGN, the ranges are partially due to an observed intrinsic X-Ray variability. ^a: Lipari et al. (1993), with detected variability on the Hα BRL shape and UV continuum between 1989 and 1991. ^b: Goodrich (1995), Bennert et al. (2006), Trippe et al. (2010). ^c: Véron-Cetty & Véron (2006), Onori et al. (2017), La Franca et al. (2015). ^d: Hernández-Yévenes et al. (2024), from Wide-field Infrared Survey Explorer (WISE) photometry, using W1 and the W1 − W2 color for M/L corrections. ^e: Bennert et al. (2006), range from different methods, including the M_BH − σ_* relation and from L_5100 Å. ^f: La Franca et al. (2015), from Paβ BRL line. ^g: Bennert et al. (2006), from L_5100 Å. ^h: Obtained by us using the Duras et al. (2020, 0.37 dex) correction with L_{2 − 10 KeV} values from Ballo et al. (2017, Mrk 915) and Winter et al. (2009, NGC 6860). ⁱ: Middei et al. (2021), from L_{2 − 10 KeV}. ^j: La Franca et al. (2015), from L_{14 − 195 KeV}.