Signal-to-noise ratio for astronomical imaging by deconvolution from wave-front sensing

Details Signal-to-noise ratio for astronomical imaging by deconvolution from wave-front sensing Signal-to-noise ratio for astronomical imaging by deconvolution from wave-front sensing

Aug 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994apopt..33.5400r&link_type=ejournal

Applied Optics, Volume 33, Issue 23, August 10, 1994, pp.5400-5414

Astronomy and Astrophysics

Astronomy

9

Image Processing, Wavefront Sensing, Signal-To-Noise Ratio, Imaging, Image Reconstruction, Convolution, Astronomy

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