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Deconvolution algorithms have been used successfully foroptimization/restoration/deblurring of astronomical images in a variety ofwavelengths, especially in the optical band (e.g., for HST). We present here aniterative Richardson-Lucy type method designed for treatment of images obtainedwith the H.E.S.S. array of ground-based gamma-ray telescopes. Its applicationto shell-type supernova remnant images yields refined details relevant for thestudy of correlations with other wavelengths, and hence for interpretation interms either of hadronic or leptonic origin of the observed VHE gamma-rayemission.

A Deconvolution technique for VHE Gamma-ray Astronomy, and its application to the morphological study of shell-type supernova remnants