1 August 1990 Infrared speckle imaging at Palomar
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Diffraction-limited infrared images of three binary stars reconstructed using speckle imaging techniques are presented. Three methods of recovering the objects' Fourier amplitudes are compared, Fourier deconvolution, projection onto convex sets, and CLEAN. The objects' Fourier phases are retrieved via bispectral analysis. It is shown that the quality of the final reconstructed images is a function of the percentage of the total bispectral volume utilized in the reconstruction procedure.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrea M. Ghez, Andrea M. Ghez, Peter W. Gorham, Peter W. Gorham, Christopher A. Haniff, Christopher A. Haniff, Shrinivas R. Kulkarni, Shrinivas R. Kulkarni, Keith Matthews, Keith Matthews, Gerry X. Neugebauer, Gerry X. Neugebauer, W. Nicholas Weir, W. Nicholas Weir, } "Infrared speckle imaging at Palomar", Proc. SPIE 1237, Amplitude and Intensity Spatial Interferometry, (1 August 1990); doi: 10.1117/12.19298; https://doi.org/10.1117/12.19298


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