Notes. The infrared ID refers to the Spitzer Space Telescope Source List (SSTSL2) for all the galaxies apart from PKS 1549–79 for which we report the 2MASS ID. The redshifts for the sources are based on emission-line measurements presented in Tadhunter et al. (1998), with the exception of PKS 1549–79 for which we used the redshift estimate for the low-ionisation lines from Tadhunter et al. (2001). The radio classifications of the sources (CC = Compact Core, CF = Compact Flat spectrum, CSS = Compact Steep Spectrum, GPS = Gigahertz-Peaked Spectrum) have been taken from literature (see Holt et al. 2008; Tzioumis et al. 2002). The radio luminosities have been taken from Holt et al. (2008) and Morganti et al. (1993), while the radio sources position angles remaining sources are from Tzioumis et al. (2002), with the exception of PKS 1549–79 and PKS 2314+03 whose radio position angles are from Holt et al. (2008). In most cases, the radio diameters represent the distances between the two brightest radio components – usually the two radio lobes the radio source – and are taken from Tzioumis et al. (2002). However, in the case of the flat-spectrum core source PKS 1549–79, which has a highly asymmetric core-jet radio structure (Holt et al. 2006; Oosterloo et al. 2019), the number given here is the full diameter of the source from Oosterloo et al. (2019). Moreover, in the case of PKS 2314+03 we give the diameter of the steep-spectrum compact core component from Thomasson et al. (2003), whereas the larger-scale FRII radio source associated with this object is much more extended (D_L ∼ 29 kpc).