Notes. Column (1): object designation in the Infrared Astronomical Satellite (IRAS) Faint Source Catalog (FSC). Column (2): other identification. Column (3): redshift from the NASA Extragalactic Database (NED). Column (4): luminosity distance assuming a ΛDCM cosmology with H₀ = 70 km s^-1 Mpc^-1, Ω_M = 0.3, and Ω_Λ = 0.7, using the E. L. Wright Cosmology calculator, which is based on the prescription given by Wright (2006). Column (5): scale. Column (6): infrared luminosity (L_IR = L(8–1000) μm) in units of solar bolometric luminosity, calculated using the fluxes in the four IRAS bands as given in Sanders et al. (2003) when available. Otherwise, the standard prescription given in Sanders & Mirabel (1996) with the values in the IRAS Point and Faint Source catalogs was used. Column (7): morphological class defined as follows: 0 identifies isolated objects, 1 pre-coalescence systems, and 2 stands for merger objects. For those objects for which the morphological classification is uncertain, the various possible classes are shown in the table with the preferred morphological classification indicated in the first place and alternative classification within brackets (see text for further details). Column (8): notes with the following code: (a) system composed of two galaxies. (b) system composed of three galaxies. (c) there are two VIMOS pointings for the northern source. (d) interacting system (i.e., see notes a and b) for which the total infrared luminosity L_IR could be approximately assigned among the members of the system according to the Spitzer/MIPS photometry. For further details, see B13.