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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3837
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dc.contributor.authorShevgaonkar, R. K-
dc.date.accessioned2008-09-23T14:25:12Z-
dc.date.available2008-09-23T14:25:12Z-
dc.date.issued1987-04-
dc.identifier.citationAstronomy And Astrophysics, Vol. 176, No. 1, No. 159 -170en
dc.identifier.issn0004-6361-
dc.identifier.urihttp://hdl.handle.net/2248/3837-
dc.description.abstractA simple maximum entropy method algorithm for deconvolving polarized images obtained from synthesis observations has been described here. A general purpose Fortran program is also developed. it demonstrated that although the a priori positivity conditions is imposed on the total intensity image only, the polarized component images also get improved remarkably.en
dc.language.isoenen
dc.publisherThe European Southern Observatoryen
dc.relation.urihttp://adsabs.harvard.edu/abs/1987A%26A...176..159Sen
dc.subjectImage processingen
dc.subjectmaximum entropyen
dc.subjectRadio astronomyen
dc.subjectStokes parametersen
dc.subjectPolarized imagesen
dc.titleMaximum Entropy Method for Polarized Imagesen
dc.typeArticleen
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