High resolution imaging with reference to a widely separated star

Naoshi Baba

doi:10.1117/12.2316176

1 September 1996 High resolution imaging with reference to a widely separated star

Naoshi Baba

Author Affiliations +

Proceedings Volume 2778, 17th Congress of the International Commission for Optics: Optics for Science and New Technology; 2778DJ (1996) https://doi.org/10.1117/12.2316176
Event: 17th Congress of the International Commission for Optics: Optics for Science and New Technology, 1996, Taejon, Korea, Republic of

Abstract

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

Citation Download Citation

Naoshi Baba "High resolution imaging with reference to a widely separated star", Proc. SPIE 2778, 17th Congress of the International Commission for Optics: Optics for Science and New Technology, 2778DJ (1 September 1996); https://doi.org/10.1117/12.2316176

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