(General comments about the panels as in Fig. A.1.) IRAS F01341-3735 (ESO 297-G011/G012): this system is composed of two galaxies (i.e., northern, southern) separated by ~25 kpc, implying the need of two VIMOS pointings. The present maps correspond to the northern galaxy, which shows a regular velocity field. The velocity dispersion map has two symmetric local maxima of ~70 km s^-1 around the nucleus, which are well fitted using one Gaussian model. These regions have low Hα surface brightness and are associated with high excitation and high σ, as reported by Monreal-Ibero et al. (2010). In the innermost regions (i.e., ~1.5 kpc²), the Hα-[NII] emission lines need a secondary broad component. The spatial scale is of 0.352 kpc/′′.