2015
DOI: 10.1080/17415977.2015.1046859
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A stochastic approach to quantifying the blur with uncertainty estimation for high-energy X-ray imaging systems

Abstract: One of the primary causes of blur in a high-energy X-ray imaging system is the shape and extent of the radiation source, or 'spot'. It is important to be able to quantify the size of the spot as it provides a lower bound on the recoverable resolution for a radiograph, and penumbral imaging methods -which involve the analysis of blur caused by a structured aperture -can be used to obtain the spot's spatial profile. We present a Bayesian approach for estimating the spot shape that, unlike variational methods, is… Show more

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Cited by 12 publications
(11 citation statements)
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“…We use this example to illustrate that IACT of the Gibbs sampler can remain constant as the dimension of x and the number of observations increase with image size. Many practical difficulties, e.g., estimation of noise and regularization parameters (see, e.g., [3,19,42]), are neglected in this example.…”
Section: Example 4: Image Deblurringmentioning
confidence: 99%
See 1 more Smart Citation
“…We use this example to illustrate that IACT of the Gibbs sampler can remain constant as the dimension of x and the number of observations increase with image size. Many practical difficulties, e.g., estimation of noise and regularization parameters (see, e.g., [3,19,42]), are neglected in this example.…”
Section: Example 4: Image Deblurringmentioning
confidence: 99%
“…As in the above examples, this effective dimension increases with dimension. We use MALA, pCN and l-MwG to draw samples from the posterior distribution (19), which is not Gaussian because the L96 model is nonlinear, i.e., M 0→T (x 0 ) is not a linear function of x 0 . The MALA proposal we use is…”
Section: Example 5: a Nonlinear Inverse Problemmentioning
confidence: 99%
“…In the probabilistic framework, the solution to (7) is equivalent to a maximum a posteriori (MAP) estimate when the PSF is assumed to be a Gaussian, and taking n = 2 guarantees that the corresponding prior covariance operator is trace class [27]. Since data and estimates are inherently discrete quantities, we proceed by discretizing (5) and (10).…”
Section: Figmentioning
confidence: 99%
“…To quantitatively analyze the images captured in this way, it is important to understand how each of these components degrades the signal and introduces blurring artifacts. The size and spatial profile of the radiation source, or "spot" produces a so-called source blur [5,9]. Blur is also caused by X-ray scatter in the scene, through the conversion and scattering of light in the scintillating crystal, optical lensing, and the response of the CCD array recording the visible light [9,19,18].…”
Section: Introductionmentioning
confidence: 99%