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Fig. 9

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Output from the SL1M algorithm applied to the NGC 5921 dataset with different sized pixels. The first panel uses delta function pixels; the second panel uses Gaussian pixels 14 arcsec (2 pixels) across; the third panel, 26 arcsec; and the 4th panel, 56 arcsec. Note that these images have not been convolved with the Gaussians corresponding to the pixel size, or with the synthetic beam of the telescope.

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