(General comments about the panels as in Fig. A.1.) IRAS 12116-5615: this is one of the few objects for which the morphological classification is uncertain (class 2 or 0). It shows a very compact Hα emission. The Hα velocity field has a typical rotation pattern, but the velocity dispersion map is not centrally peaked. The latter shows higher values in the outer parts, which also have high excitation and low-Hα surface brightness (see Monreal-Ibero et al. 2010). The scale is of 0.545 kpc/′′.