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Fig. 3


Illustration of the HNN deconvolution, using galaxies from the GREAT10 image processing challenge. The three rows show three different galaxies. In each row, are shown from left to right: the original GREAT10 postage stamp for each galaxy, the associated PSF, the HNN deconvolution, the residual image (difference between data and deconvolved images, reconvolved by the PSF), the ACF of the deconvolved galaxy, and the ACF clipped at the radius that encloses 90% of the total light.

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