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Proceedings Paper

Phase diversity in an exo-planet imager
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Paper Abstract

A possible system for imaging an exo-planet uses a telescope, coronagraphic mask, and Lyot stop. However, the optics must be nearly flawless for a planet to be imaged, since imperfections cause the image to have speckles which mask the planet. The speckle pattern can be suppressed by removing its phase with an adaptive optic and by reimaging it through a lens with a small, central obscuration. We show how phase diversity can be used to determine the phase.

Paper Details

Date Published: 14 September 2005
PDF: 8 pages
Proc. SPIE 5905, Techniques and Instrumentation for Detection of Exoplanets II, 590510 (14 September 2005); doi: 10.1117/12.628734
Show Author Affiliations
Robert A. Gonsalves, Tufts Univ. (United States)
Volker Tolls, Harvard-Smithsonian Ctr. for Astrophysics (United States)


Published in SPIE Proceedings Vol. 5905:
Techniques and Instrumentation for Detection of Exoplanets II
Daniel R. Coulter, Editor(s)

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