Toward high-resolution imaging with a simple adaptive-optics system

Details Toward high-resolution imaging with a simple adaptive-optics system Toward high-resolution imaging with a simple adaptive-optics system

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996optl...21..626b&link_type=abstract

Optics Letters, Volume 21, Issue 9, May 1, 1996, pp.626-628

Physics

Optics

3

Adaptive Optics, Astronomical Optics, Atmospheric And Ocean Optics, Image Analysis, Image Processing, Imaging Systems, Speckle Imaging

Scientific paper

High-resolution imaging with reference to a widely separated star is examined. Peak tracking of the specklegram in the reference channel results in a high-resolution image in the observational channel. A binary star with angular separation of 30.5 arcsec is examined in white light, and the resultant image of the primary star obtained with reference to the secondary star is shown to have better resolution than the centroid tracking image by a factor of 3.

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