Fig. 2
Effect of the regularization scheme on the deconvolution results. Left: a VLT/FORS2 optical image of a spiral galaxy is shown in the top panel, along with the HST/ACS observation of the same galaxy in the bottom panel. Middle: deconvolution with the new regularization scheme along with the residual image in the bottom panel. Right: same as in the middle panel, but with the regularization term used in the original MCS algorithm. The PSNR is given for each deconvolution, and the mean square errors (MSE) are given with the residual images.
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