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Proceedings Paper

Diffraction-limited imaging at IR wavelengths using aperture masks and fully filled apertures
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Paper Abstract

The performance of a phase recovery algorithm developed for speckle data collected using a pupil-plane mask has been investigated for use at near-infrared wavelengths. The method, based on the radio-astronomical self-calibration technique, has been tested alongside a state-of-the-art implementation of the Knox-Thompson scheme using both simulated and real specklegrams. Results indicate that the new procedure is as effective as the Knox-Thompson based image reconstruction scheme and is applicable to a wide range of astrophysically interesting sources.

Paper Details

Date Published: 1 August 1990
PDF: 13 pages
Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990); doi: 10.1117/12.19299
Show Author Affiliations
Christopher A. Haniff, California Institute of Technology (United Kingdom)
David F. Buscher, Mullard Radio Astronomy Observatory (United Kingdom)
Julian C. Christou, National Optical Astronomy Observatories (United States)
Stephen T. Ridgway, National Optical Astronomy Observatories (United States)


Published in SPIE Proceedings Vol. 1237:
Amplitude and Intensity Spatial Interferometry
James B. Breckinridge, Editor(s)

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