Paper
1 August 1990 Diffraction-limited imaging at IR wavelengths using aperture masks and fully filled apertures
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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.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christopher A. Haniff, David F. Buscher, Julian C. Christou, and Stephen T. Ridgway "Diffraction-limited imaging at IR wavelengths using aperture masks and fully filled apertures", Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990); https://doi.org/10.1117/12.19299
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Cited by 4 scholarly publications.
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KEYWORDS
Calibration

Image restoration

Speckle

Ultraviolet radiation

Astronomy

Signal to noise ratio

Interferometry

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