(General comments about the panels as in Fig. A.1.) IRAS 08424-3130 (ESO 432-IG006): the Digital Sky Survey (DSS) image shows a pair of spiral galaxies (nuclear separation of ~9 kpc) in interaction. Only part of the nuclear region of both galaxies is covered by our VIMOS FoV. The area covered by the Hα emission line for the northern galaxy is very small, so that its kinematical classification was not possible. The southern object reveals a relatively regular velocity field with an amplitude of 133 km s^-1 and an almost centrally peaked velocity dispersion map. The spatial scale is 0.329 kpc/′′.