I. Introduction
Many image restoration tasks can be posted as the following inverse problem: Given an observed image corrupted according to some forward model and noise, find the underlying image which “best explains” the observation. In estimation, we often formulate this problem as a maximum-a-posteriori (MAP) estimation [1], where the goal is to maximize the posterior probability: \begin{align} \boldsymbol{\widehat{x}}&= \mathop {\underset{\mathbf{x}}{\text{argmax}}} p(\mathbf{x}| \mathbf{y}) \nonumber \\ &= \mathop {\underset{\mathbf{x}}{\text{argmin}}} -\log p(\mathbf{y}| \mathbf{x}) - \log p(\mathbf{x}), \end{align}
for some conditional probability defining the forward imaging model, and a prior
distribution defining the
probability distribution of the latent image. Because of the explicit use of the forward and the prior models, MAP
estimation is also a model-based image reconstruction (MBIR) method [2] which
has many important applications in deblurring [3]–
[5], interpolation [6]–
[8], super-resolution [9]
–[12] and computed tomography [13]
, to name a few.