Notes. Column (1): object designation in the Infrared Astronomical Satellite (IRAS) Point Source Catalogue (PSC) and in the IRAS Faint Source Catalogue (FSC; with prefix “F”). Column (2): other name. Column (3): redshift from the NASA Extragalactic Database (NED). Column (4): infrared luminosity (L_IR = L_{(8−1000 μm)}) in units of solar bolometric luminosity calculated with the flux in the four IRAS bands as given in Sanders et al. (2003) when available. Otherwise, the standard prescription in Sanders & Mirabel (1996) with the values in the IRAS-FSC and IRAS-PSC catalogues was used. For some targets (22%, i.e.,11/51), new updated L_IR values can be found in the Surace et al. (2004). However, for sake of homogeneity, preferred to use the values described above for the whole sample. For those systems for which it was possible to measure the L_IR of the individual galaxies, that of the system is indicated in parenthesis. Column (5): morphology class defined as follows: 0 identifies isolated rotating disks, 1 interacting systems, and 2 mergers. We refer to Rodríguez-Zaurín et al. (2011) and Bellocchi et al. (2013) for further details about this classification. Column (6): S.C. stands for (nuclear) spectroscopic classification of the ionization type. H defines HII galaxy, L, LINER, and Sy stands for Seyfert (see Rodríguez-Zaurín et al. 2011). Column (7): AGN and SB indicate, respectively, evidence of an AGN (from the infrared, optical, and X-ray observations) and starburst galaxies. When possible we also give an estimate of the AGN contribution to the 24 μm and bolometric luminosity (round and square parenthesis, respectively). Columns (8) and (9): our classification scheme, according to the integrated spectra (i.e., 1D, Col. (8)) and the maps (i.e., 2D, Col. (9)). If multiple classifications are quoted for the same object, each classification refers to different kinematic components. The letter S refers to a systemic component, while R and B indicate, respectively, the presence of redshifted (i.e., V> 60 km s^-1) and blueshifted (i.e., V< −60 km s^-1) components (with respect to the stars). GW stands for galaxy in which footprint of a galactic winds was found via NaD (see Sect. 4.3) and RD indicates the presence of a disk of neutral gas (see Sect. 4.8).

Reference.