Notes. Columns: (1) and (2): object designation in the Infrared Astronomical Satellite (IRAS) Faint Source Catalog (FSC) and other identification; (3) and (4): right ascension (hours, minutes and seconds) and declination (degrees, arcminutes and arcseconds) from the IRAS FSC; (5): redshift derived from the CO(2–1) emission line; (6): luminosity distance assuming a ΛDCM cosmology with H₀ = 67.8 km s⁻¹ Mpc⁻¹, Ω_M = 0.308, Ω_Λ = 0.692, using the E. L. Wright Cosmology calculator, which is based on the prescription given by Wright (2006); (7): scale; (8): logarithmic infrared luminosity, L_IR, as derived in Díaz-Santos et al. (2017) assuming for the sample the luminosity distances, D_L, from Armus et al. (2009). We then scaled the L_IR according to the D_L used in this work. For individual galaxies in multiple systems, these are estimated dividing the total luminosity according to the relative fluxes in the MIPS images at 24 μm; (9): SFR derived following the Kennicutt & Evans (2012) relation with a Kroupa (Kroupa 2001) IMF (as in Murphy et al. 2011; 10): ‘Composite’ classification based on IRAC and HST morphological classifications complemented by the kinematic classification based on the ionized and molecular gas tracers (i.e., Hα and CO). For further details see Sect. 2 and Appendix A. 0 (R), 0 (P), 1 and 2 stand for isolated rotating disk, isolated perturbed disk, interacting and merger systems, respectively; (11): (y) indicates that the object shows evidence of an AGN.

References. This information is taken from the references listed according to the following code: (a) Arribas et al. (2014), (b) Yuan et al. (2010), (c) Pereira-Santaella et al. (2011), (d) Jiménez-Bailón et al. (2007), (e) Alonso-Herrero et al. (2009).