Point-spread function reconstruction in ground-based astronomy by l(1)-l(p) model.


In ground-based astronomy, images of objects in outer space are acquired via ground-based telescopes. However, the imaging system is generally interfered by atmospheric turbulence, and hence images so acquired are blurred with unknown point-spread function (PSF). To restore the observed images, the wavefront of light at the telescope's aperture is utilized… (More)
DOI: 10.1364/JOSAA.29.002263

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