IRAS 06206-6315. Top panels show the A_V map derived from the Paα at 1.876μm and Brγ at 2.166μm line ratio, the observed maps of the Paα emission, together with the star formation rate surface density (Σ_SFR) map, corrected from extinction. Units are [mag], log[erg s^-1 cm^-2], and [M_⊙ yr^-1 kpc^-2], respectively. The nucleus and Paα peak are marked with a plus sign (+) and a diamond (◇), respectively. The main nucleus is defined as the brightest spaxel of the SINFONI K-band image (Paper I), and the Brγ (Paα) peak corresponds to the brightest spaxel of the corresponding emission map. Bottom left panel shows the observed (blue histogram) and the corrected-from-extinction (yellow histogram) Σ_SFR spaxel-by-spaxel distributions. The relationship between the corrected Σ_SFR values and the A_V is shown in the bottom right panel only for those points with a spaxel-by-spaxel correction of the extinction. The blue histograms show the projected distribution onto each axis and are arbitrarily normalised, whereas the blue lines are the median of each distribution.