Notes. Columns (2)–(4): right ascension, declination, and redshift from the NASA Extragalactic Database (NED). Columns (5) and (6): luminosity distance and angular scale from Ned Wright’s Cosmology Calculator (Wright 2006) assuming H₀ = 70 km s⁻¹ Mpc⁻¹, Ω_M = 0.3 and Ω_Λ = 0.7. Column (7): infrared luminosities, where L_IR(8–1000 μm) was calculated from the IRAS flux densities f₁₂, f₂₅, f₆₀ and f₁₀₀ presented in Sanders et al. (2003). Column (8): spectroscopic classification as in Table 1 from Piqueras López et al. (2012). Galaxies classified as composite present IR emission that can be explained by a combination of AGN activity and star formation. Column (9): gravitational interaction stage classification as follows: (a) isolated, (b) interacting pair, (c) ongoing merger, and (d) post-coalescence merger. This classification is a simplified version based on the morphology classes presented in Yuan et al. (2010), when possible, and Arribas et al. (2008).