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An Iterative Method for Edge-Preserving MAP Estimation When Data-Noise Is Poisson
2010
SIAM Journal on Scientific Computing
In numerous applications of image processing, e.g. astronomical and medical imaging, data-noise is well-modeled by a Poisson distribution. This motivates the use of the negative-log Poisson likelihood function for data fitting. (The fact that application scientists in both astronomical and medical imaging regularly choose this function for data fitting provides further motivation.) However difficulties arise when the negative-log Poisson likelihood is used. Chief among them are the facts that
doi:10.1137/080726884
fatcat:eli4fhaudvc33dau7etuqommjm