  This paper presents unique adaptive optics images at 3.5 and 4.8 microns of
the central arcsec in the AGN of NGC1068. They enlight the presence of hot to
warm dust close to the central engine of the AGN. At a radius around 40 pc, the
dust is clearly contained within a disc-like structure perpendicular to the
ionizing cone axis. These observations support AGN dusty/molecular torus
modeling.
