(General comments about the panels as in Fig. A.1.) IRAS F06076-2139: this system consists of two galaxies in interaction with a rather complex morphology. The Hα image shows a rather different structure than that shown by the VIMOS continuum and the HST-ACS image. The southern galaxy is characterized by a ring and a tidal tail-like structures extending towards the west and northwest part from the nucleus. The faint broad component found in a small region of the ring in the southern object is likely due to the superposition of the emission of the two galaxies along the line-of-sight. This system was already studied in Arribas et al. (2008). The scale is 0.743 kpc/′′.