DocumentCode :
1359643
Title :
Imaging with LINC-NIRVANA
Author :
Bertero, M. ; Boccacci, P. ; Desidera, G. ; La Camera, A. ; Carbillet, M. ; Lanteri, Henri
Author_Institution :
Univ. of Genova, Genoa, Italy
Volume :
27
Issue :
1
fYear :
2010
Firstpage :
110
Lastpage :
115
Abstract :
The basic problem of LINC-NIRVANA (LN) imaging is to combine the different images for getting a single image, possibly with a resolution close to that of a 22.8 m mirror in all directions. This result can be hardly reached in practice because it depends on the level and uniformity of the adaptive optics (AO) correction and on the declination of the scientific target, controlling the orientations of the baseline that can be used during its observation. In this article, we give a brief introduction to this problem. It can be solved by iterative methods related to the well-known Richardson-Lucy (RL) algorithm. Since RL is a particular case of the maximum likelihood method introduced by Shepp and Vardi in emission tomography and denoted expectation maximization (EM), improvements of EM, proposed in the field of medical imaging can be applied to LN.
Keywords :
adaptive optics; astronomical image processing; astronomical techniques; astronomical telescopes; deconvolution; expectation-maximisation algorithm; interferometers; interferometry; Fizeau interferometer; LINC-NIRVANA; Large Binocular Telescope; Richardson-Lucy algorithm; adaptive optics correction; anisotropic resolution; expectation maximization; image deconvolution methods; image fusion; iterative methods; maximum likelihood method; target declination; Anisotropic magnetoresistance; Cameras; Deconvolution; Image resolution; Instruments; Interference; Mirrors; Optical imaging; Optical interferometry; Telescopes;
fLanguage :
English
Journal_Title :
Signal Processing Magazine, IEEE
Publisher :
ieee
ISSN :
1053-5888
Type :
jour
DOI :
10.1109/MSP.2009.934714
Filename :
5355501
Link To Document :
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