. Sampling techniques are used to explore the Bayesian posterior density in imaging problems. Besides the familiar MAP estimators, such techniques can easily provide more detailed information on the posterior, such as moments and marginal densities. From these, error bars and confidence levels can be assessed, and hypothesis testing performed. The algorithms are implemented in IRAF, and are being tested on both simulated and actual ROSAT images. 1. Introduction The image formation process introduces uncertainties in pixel values, due to both deterministic (Point Response Function, PRF) and random (noise) effects. The traditional approach to this problem involves some sort of inversion technique, and these are usually unable to use optimall...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
We present a new, fully generative model for constructing astronomical catalogs from optical telesco...
The pervasive presence of noise corrupts the data and their interpretation implies a solution of an ...
In this paper, a performance study of a methodology for reconstruction of high-resolution remote sen...
This thesis is concerned with methods for Bayesian inference and their applications in astrophysics....
Two important issues, computation and model evaluation, in general nonlinear image restoration are a...
Bayesian methods are being increasingly employed in many different areas of research in the physical...
When preparing an article on image restoration in astronomy, it is obvious that some topics have to ...
Radio astronomy image formation can be treated as a linear inverse problem. However, due to physical...
When preparing an article on image restoration in astronomy, it is obvious that some topics have to ...
Bayesian probability theory is employed to provide a stable and unique solution to the ill-posed inv...
This chapter considers the use of statistical modelling approaches and stochastic estimation algorit...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
We present a new, fully generative model for constructing astronomical catalogs from optical telesco...
The pervasive presence of noise corrupts the data and their interpretation implies a solution of an ...
In this paper, a performance study of a methodology for reconstruction of high-resolution remote sen...
This thesis is concerned with methods for Bayesian inference and their applications in astrophysics....
Two important issues, computation and model evaluation, in general nonlinear image restoration are a...
Bayesian methods are being increasingly employed in many different areas of research in the physical...
When preparing an article on image restoration in astronomy, it is obvious that some topics have to ...
Radio astronomy image formation can be treated as a linear inverse problem. However, due to physical...
When preparing an article on image restoration in astronomy, it is obvious that some topics have to ...
Bayesian probability theory is employed to provide a stable and unique solution to the ill-posed inv...
This chapter considers the use of statistical modelling approaches and stochastic estimation algorit...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
The inverse temperature parameter of the Potts model governs the strength of spatial cohesion and th...
We present a new, fully generative model for constructing astronomical catalogs from optical telesco...