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: http://www.stsci.edu/stsci/meetings/irw/proceedings/bundschuhb.dir/section3_6.html
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Fig. 6 shows an image of Saturn which was recorded with the Wide Field / Planetary Camera. It is stored in the file SATURN.FITS. The measured point spread function from the data file SATURN_PSF.FITS is also displayed.
Fig. 7 shows the result of restoration. The restored image appears much clearer, with higher contrast than the measured data. The edges, which are considerably blurred in the measured data, can now be located exactly. Therefore the improvement provided by the restoration is obvious.
