(General comments about the panels as in Fig. A.1.) IRAS F06206-6315: this system has a double nuclei separated by ~4 kpc, as clearly seen in the the Near Infrared Camera and Multi-Object Spectrometer (NICMOS/HST) image. There is a tidal tail starting in the north and bending towards the southeast, which contains a local peak of Hα emission (i.e., a possible tidal dwarf galaxy candidate). The brightest nucleus seems to be in positional agreement with the kinematic center. The velocity field is regular, and most of the spectra are well fitted using one component. The scale is of 1.72 kpc/′′.