Notes. ^( * )Not included in the sample of Paper I. (1) Identification number used in this paper. (2) Galaxy name. (3) Redshift. (4) Luminosity distance calculated from redshift following the same procedure as Sanders et al. (2003). (5) Infrared luminosity based on IRAS fluxes taken from Sanders et al. (2003) and calculated with the same methods used by Sanders & Mirabel (1996). Only for UGC 11763 are fluxes taken from Sanders et al. (1989). (6) Bolometric AGN fraction (α_AGN = L_AGN/L_bol) calculated from mid-infrared diagnostics by Díaz-Santos et al. (2017). See Sect. 2 for detail. (7) Merger stage visually determined by Stierwalt et al. (2013). N = nonmerger, a = pre-merger, b = early-stage merger, c = mid-stage merger, and d = late-stage merger. (8) Presence of CON found by HCN-vib observations. Details are presented in Paper I. (9) Presence of molecular outflow found by CO and/or OH observations.

References. (i) García-Burillo et al. (2015); (ii) Fluetsch et al. (2019); (iii) Lutz et al. (2020); (iv) Cicone et al. (2014); (v) Pereira-Santaella et al. (2016) for CO observations and (vi) Veilleux et al. (2013) and (vii) González-Alfonso et al. (2017) for OH observations. (10) Presence of molecular inflow found by CO and/or OH observations. References are (α) Veilleux et al. (2013) and (β) Falstad et al. (2021) for OH observations and (γ) González-Alfonso et al. (2021) for CO and OH observations.