In this paper we propose a solution to the problem of reducing the boundary effects (ripples) in the deconvolution of astronomical images. The approach applies to the Richardson-Lucy method (RLM), namely the most frequently used deconvolution method in Astronomy, and is based on the idea of using RLM for attempting a reconstruction of the astronomical target in a domain broader than that of the detected image. Even if, in general, the reconstruction outside the image domain is not reliable, this approach, in a sense, is letting RLM to choose the appropriate boundary conditions and, as a consequence, the reconstruction inside the domain is considerably improved. We propose a simple implementation of this approach, allowing a reductio...
We address the problem of deconvolution of astronomical images that could be obtained with future la...
We develop a self-consistent automatic procedure to restore information from astronomical observati...
This article reviews different deconvolution methods. The all-pervasive presence of noise is what ma...
The deconvolution of astronomical images by the Richardson-Lucy method (RLM) is extended here to the...
Received —; accepted —. Our approach proposed in a previous paper for the reduction of boundary effe...
Our approach proposed in a previous paper for the reduction of boundary effects in the deconvolutio...
Context. The Richardson-Lucy method is the most popular deconvolution method in astronomy because it...
It is well-known that when an astronomical image is collected by a telescope, the measured intensiti...
Context.The standard Richardson-Lucy method (RLM) does not work well in the deconvolution of astron...
It is well-known that when an astronomical image is collected by a telescope, the measured intensiti...
Richardson-Lucy (RL) deconvolution is one of the classical methods widely used in X-ray astronomy an...
In previous papers we proposed methods and software for the restoration of images provided by Fizeau...
Context. Images from adaptive optics systems are generally affected by significant distortions of th...
A new method for improving the resolution of astronomical images is presented. It is based on the pr...
Astronomy and Astrophysics, 430, pp. 731-738 (2005)International audienceIn previous papers we propo...
We address the problem of deconvolution of astronomical images that could be obtained with future la...
We develop a self-consistent automatic procedure to restore information from astronomical observati...
This article reviews different deconvolution methods. The all-pervasive presence of noise is what ma...
The deconvolution of astronomical images by the Richardson-Lucy method (RLM) is extended here to the...
Received —; accepted —. Our approach proposed in a previous paper for the reduction of boundary effe...
Our approach proposed in a previous paper for the reduction of boundary effects in the deconvolutio...
Context. The Richardson-Lucy method is the most popular deconvolution method in astronomy because it...
It is well-known that when an astronomical image is collected by a telescope, the measured intensiti...
Context.The standard Richardson-Lucy method (RLM) does not work well in the deconvolution of astron...
It is well-known that when an astronomical image is collected by a telescope, the measured intensiti...
Richardson-Lucy (RL) deconvolution is one of the classical methods widely used in X-ray astronomy an...
In previous papers we proposed methods and software for the restoration of images provided by Fizeau...
Context. Images from adaptive optics systems are generally affected by significant distortions of th...
A new method for improving the resolution of astronomical images is presented. It is based on the pr...
Astronomy and Astrophysics, 430, pp. 731-738 (2005)International audienceIn previous papers we propo...
We address the problem of deconvolution of astronomical images that could be obtained with future la...
We develop a self-consistent automatic procedure to restore information from astronomical observati...
This article reviews different deconvolution methods. The all-pervasive presence of noise is what ma...