Wavelet-based Image deconvolution for Wide Field CCD Imagery

dc.contributor.authorMerino, M.T.
dc.contributor.authorFors Aldrich, Octavi
dc.contributor.authorOtazu Porter, Xavier
dc.contributor.authorCardinal, Robert D.
dc.contributor.authorNúñez de Murga, Jorge, 1955-
dc.contributor.authorHildebrand, A.R.
dc.date.accessioned2024-02-15T14:54:51Z
dc.date.available2024-02-15T14:54:51Z
dc.date.issued2006
dc.date.updated2024-02-15T14:54:51Z
dc.description.abstractWe show how a wavelet-based image adaptive deconvolution algorithm can provide significant improvements in the analysis of wide-field CCD images. To illustrate it, we apply our deconvolution protocol to a set of images from a Baker-Nunn telescope. This f/1 instrument has an outstanding field of view of 4.4°x4.4° with high optical quality offering unique properties to study our deconvolution process and results. In particular, we obtain an estimated gain in limiting magnitude of ΔR∼0.6 mag and in limiting resolution of Δρ∼3.9 arcsec. These results increase the number of targets and the efficiency of the underlying scientific project.
dc.format.extent4 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec552858
dc.identifier.issn0004-6280
dc.identifier.urihttps://hdl.handle.net/2445/207632
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.isformatofReproducció del document publicat a:
dc.relation.ispartofPublications of the Astronomical Society of the Pacific, 2006, vol. 351, p. 153-156
dc.rights(c) Merino, M.T. et al., 2006
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationProcessament d'imatges
dc.subject.classificationAstronomia
dc.subject.classificationTelescopis espacials
dc.subject.otherImage processing
dc.subject.otherAstronomy
dc.subject.otherSpace telescopes
dc.titleWavelet-based Image deconvolution for Wide Field CCD Imagery
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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