(General comments about the panels as in Fig. A.1.) IRAS F07160-6215 (NGC 2369): this is an edge-on dusty galaxy, whose structure could strongly affect the pattern of its velocity field and velocity dispersion map. Indeed, the velocity field has a clear rotation component with some irregularities, and the velocity dispersion map shows distorted inner (~1 kpc) regions, with values ranging between 120 and 200 km s^-1, where a broad component has been considered to properly fit the spectra. The scale is 0.221 kpc/′′.