2016
DOI: 10.1117/1.jrs.10.035019
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Star smear removal for full-frame charge-coupled device images based on Gaussian fitting

Abstract: .Image smear, produced by the shutter-less operation of full-frame charge-coupled device (CCD) sensors, greatly affects the performance of target detection, the centering accuracy, and visual magnitude estimation. We study the operation principle of full-frame CCDs, analyze the cause and properties of smear effect, and propose a smear removal algorithm for star images of full-frame CCDs. The proposed method locates the smears and extracts the rough profiles of the smeared stars by finding the conditional extre… Show more

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Cited by 4 publications
(1 citation statement)
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“…The fitting methods estimate the star centroid by fitting the intensity of a star spot to the Gaussian function. As the star spot conforms to a 2-dimensional Gaussian function, the Gaussian fitting algorithm (GF) can in theory achieve the highest star centroiding accuracy [ 11 , 12 , 13 ]. However, since solving the Gaussian parameters is a nonlinear optimization problem, which is inevitably a multiple-step iteration process, the algorithm is quite sensitive to the initial parameters and is time consuming in practice.…”
Section: Introductionmentioning
confidence: 99%
“…The fitting methods estimate the star centroid by fitting the intensity of a star spot to the Gaussian function. As the star spot conforms to a 2-dimensional Gaussian function, the Gaussian fitting algorithm (GF) can in theory achieve the highest star centroiding accuracy [ 11 , 12 , 13 ]. However, since solving the Gaussian parameters is a nonlinear optimization problem, which is inevitably a multiple-step iteration process, the algorithm is quite sensitive to the initial parameters and is time consuming in practice.…”
Section: Introductionmentioning
confidence: 99%