Paper
23 August 1995 Speckle deconvolution imaging using an iterative algorithm
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Abstract
We present an application of an iterative deconvolution algorithm to speckle interferometric data. This blind deconvolution algorithm permits the recovery of the target distribution when the point spread function is either unknown or poorly known. The algorithm is applied to specklegrams of the multiple star systems, and the results for (zetz) UMa are compared to shift-and-add results for the same data. The linearity of the algorithm is demonstrated and the signal-to-noise ratio of the reconstruction is shown to grow as the square root of the number of specklegrams used. This algorithm does not require the use of an unresolved target for point spread function calibration.
© (1995) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Julian C. Christou, E. Keith Hege, and Stuart M. Jefferies "Speckle deconvolution imaging using an iterative algorithm", Proc. SPIE 2566, Advanced Imaging Technologies and Commercial Applications, (23 August 1995); https://doi.org/10.1117/12.217368
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Cited by 5 scholarly publications.
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KEYWORDS
Point spread functions

Speckle

Detection and tracking algorithms

Deconvolution

Reconstruction algorithms

Signal to noise ratio

Speckle imaging

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