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2005 (v1)PublicationUploaded on: April 14, 2023
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2003 (v1)Publication
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2000 (v1)Publication
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2000 (v1)Publication
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1998 (v1)Publication
The book provides an introduction to the theory of inverse problems and their application to imaging
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2003 (v1)Publication
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1997 (v1)Publication
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2000 (v1)Publication
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2009 (v1)Publication
This paper describes VisualPedia, an extension of Media-Wiki, which has been developed to promote collaboration among school teachers while producing class material. The user profile of MediaWiki is expanded to allow a personalized content delivery that is tailored to different users, including users with disabilities.
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2002 (v1)Publication
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2009 (v1)Publication
Image deblurring is an important topic in imaging science. In this review, we consider together fluorescence microscopy and optical/infrared astronomy because of two common features: in both cases the imaging system can be described, with a sufficiently good approximation, by a convolution operator, whose kernel is the so-called point-spread...
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2006 (v1)Publication
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2009 (v1)Publication
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1999 (v1)Publication
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1999 (v1)Publication
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2002 (v1)Publication
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2010 (v1)Publication
In applications of imaging science, such as emission tomography, fluorescence microscopy and optical/infrared astronomy, image intensity is measured via the counting of incident particles (photons, gamma-rays, etc). Fluctuations in the emission-counting process can be described by modeling the data as realizations of Poisson random variables...
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2004 (v1)Publication
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2005 (v1)Publication
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2007 (v1)Publication
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2003 (v1)Publication
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2016 (v1)Publication
The Software Package AIRY (acronym of Astronomical Image Restoration in interferometrY) is a complete tool for the simulation and the deconvolution of astronomical images. The data can be a post-Adaptive-optics image of a single dish telescope or a set of multiple images of a Fizeau interferometer. Written in IDL and freely downloadable, AIRY...
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2011 (v1)Publication
LINC-NIRVANA (LN) is the Fizeau interferometer of the Large Binocular Telescope which consists of two 8.4 m mirrors with a center-to-center distance of 14.4 m, hence providing a maximum path of 22.8 m in the direction of the baseline joining the two centers. LN is a true imager since interference occurs in the focal plane and not in the...
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