NGC 2369. Top and middle panels are SINFONI observed maps (not corrected from extinction) of the lines Brγ λ2.166 μm, and H₂ 1−0S(1)λ 2.122 μm. From left to right: flux, equivalent width, velocity dispersion and velocity. Lower panel shows, from left to right, the K band emission from our SINFONI data, HST/NICMOS F160W continuum image from the archive, HeIλ2.059 μm, and [FeII]λ1.644 μm emission maps. The brightest spaxel of the SINFONI K band is marked with a cross. The apertures used to extract the spectra at the bottom of the figure are drawn as white squares and labelled accordingly. At the bottom, the two rest-frame spectra extracted from apertures “A” and “B” are in black. The most relevant spectral features are labelled at the top and marked with a dotted line. The sky spectrum is overplotted as a dashed blue line, and the wavelength ranges of the water vapour atmospheric absorptions are marked in light grey.