A method for space-variant deblurring with application to adaptive optics imaging in astronomy

Journal
Date Issued
2015
Author(s)
La Camera, A.
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Boccacci, P.
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Bertero, M.
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DOI
Description
This work has been partially supported by INAF (National Institute for Astrophysics) under the project TECNO-INAF 2010 “Exploiting the adaptive power: a dedicated free software to optimize and maximize the scientific output of images from present and future adaptive optics facilities”. L.S. acknowledges Carmelo Arcidiacono and Antonio Sollima for the useful discussions.
Abstract
Context. Images from adaptive optics systems are generally affected by significant distortions of the point spread function (PSF) across the field of view, depending on the position of natural and artificial guide stars. Image reduction techniques circumventing or mitigating these effects are important tools to take full advantage of the scientific information encoded in adaptive optics images. Aims: The aim of this paper is to propose a method for the deblurring of the astronomical image, given a set of samples of the space-variant PSF. Methods: The method is based on a partitioning of the image domain into regions of isoplanatism and on applying suitable deconvolution methods with boundary effects correction to each region. Results: The effectiveness of the boundary effects correction is proved. Moreover, the criterion for extending the disjoint sections to partially overlapping sections is validated. The method is applied to simulated images of a stellar system characterized by a spatially variable PSF. We obtain good photometric quality, and therefore good science quality, by performing aperture photometry on the deblurred images. The proposed method is implemented in IDL in the Software Package "Patch", which is available on "http://www.airyproject.eu"
Volume
579
Start page
A1
Uri
Url
Issn Identifier
0004-6361
Ads BibCode
2015A&A...579A...1L
Rights
open.access
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