Notes. The format of the columns is as follows: (1) source name, the asterisk stands for the radio parameters (T_B, peak, and total α and β_c) are collected from Baan & Klöckner (2006). (2) optical redshift. (3) the optical spectroscopic classification in the literature: ⁽¹⁾Darling & Giovanelli (2006), ⁽²⁾Yuan et al. (2010), ⁽³⁾Baan et al. (1998). Symbols: H, H II region (starburst); L, LINER; S2, Seyfert type 2; S1, Seyfert type 1. cp = starburst–AGN composite galaxies. (4) and (5) are the IRAS 60 and 100 μm flux densities in Jy. (6) luminosity of the OH 1667 MHz line from Zhang et al. (2014). (7) brightness temperature from Table A.1 with lower uncertainties. (8) and (9) are the spectral indexes derived from the integrated and peak flux densities of Table A.1. (10) and (11), the FIR-radio luminosity ratio derived from equation (Baan & Klöckner 2006) (q = log(3.36×10²*(2.58 f_{60 μm} + f_{100 μm})/F_radio)) using radio flux density at 1.4 GHz and 4.8 GHz, respectively. Most radio flux densities are from Table A.1. For sources that do not have a 1.4 GHz flux density, we used the flux densities from the NVSS survey. For sources without 4.8 GHz, we derived the flux density from fitting the multiband radio flux densities from Table A.1. (12) The nuclear activity factor (Baan & Klöckner 2006) was derived from equation: β_c = 0.308[q-0.75×T_b+3×α_peak-1]. Positive values indicate a starburst signature for the dominant nuclear power source, and negative values indicate an AGN signature. (13) The relative positions between OH line and continuum peak positions from Table A.1. The error on relative positions was estimated using equation from Tarchi et al. (2011): , where θ denotes the beam FWHM of the map, S/N stands for signal-to-noise ratio, line and cont refer to line and continuum emission.