Fig. 2. The 11.2 µm data. Top left: the NGC 1068 raw image. Top right: the reference star used as PSF. Bottom left: the deconvolved image of NGC 1068. On all images, North is to the top, East to the left. The pixel scale is /pixel, and the total field spans . On the raw image and the PSF image, a series of 8 contours (step by factor 3 in intensity from one to the next) has been superimposed. On the deconvolved image, 10 contours (same step) have been superimposed. The bottom right panel features in its background the 20.5 µm deconvolved image on top of which the 11.2 µm contours have been superimposed, showing the correspondence of structures at 11.2 and 20.5 µm. Note that cloud (d) seen on the 20.5 µm image is not detected at 11.2 µm, probably because of temperature and opacity effects.