NGC 2369. Top panels show the SINFONI K band continuum emission, the observed maps (not corrected from extinction) of the lines Brγ at 2.166 μm and Brδ at 1.945 μm, together with the A_V map. The white contour englobes those spaxels above S/N = 4 considered to build the A_V map and distribution. The brightest spaxel of the K band continuum is marked with a plus symbol (+), and has been used as reference to obtain the radial profile in the bottom right panel. The secondary nucleus, if present, is marked with a cross (×). Bottom left panel shows the A_V distribution of all valid spaxels (blue histogram) and the distributions of the those spaxels above (red) and below (yellow) the median value of the Brδ S/N distribution. The relationship between the surface brightness of the lines and the A_V is shown in the central panel, where the points with A_V < 0 are outlined with a black contour. Finally, the radial distribution of the extinction is shown in the bottom right panel, where the blue line represents the mean value of A_V for different radial bins and its error. The bins are obtained as the 1/30 of the total radial coverage of the map.