High resolution imaging with reference to a widely separated star

Details High resolution imaging with reference to a widely separated star High resolution imaging with reference to a widely separated star

Jan 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996spie.2778.1004b&link_type=abstract

Conference Paper, SPIE Proceedings, Vol. 2778, p. 1004, 1005-.

Astronomy and Astrophysics

Astronomy

High Resolution, Imaging Techniques, Spatial Resolution, Binary Stars, Infrared Astronomy, Near Infrared Radiation

Scientific paper

It is shown that high resolution imaging is possible by use of a reference star that is separated wider than the isoplanatic angle from the object under observation. A shift-and-add operation to the reference star results in a high resolution image of the object, though not diffraction-limited. Observational results on a binary star with angular separation of 22 arcsec indicate that a simple adaptive optics system is feasible in the visible region.

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