Benefits of Image Deconvolution in CCD Imagery

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dc.contributor.authorFors Aldrich, Octavi
dc.contributor.authorMerino, M.T.
dc.contributor.authorOtazu Porter, Xavier
dc.contributor.authorCardinal, Robert D.
dc.contributor.authorNúñez de Murga, Jorge, 1955-
dc.contributor.authorHildebrand, A.R.
dc.date.accessioned2026-03-19T12:15:41Z
dc.date.available2026-03-19T12:15:41Z
dc.date.issued2006-01
dc.date.updated2026-03-19T12:15:43Z
dc.description.abstractWe show how wavelet-based image deconvolution can provide to wide-field CCD telescopes an increase in limiting magnitude of Δ R ∼ 0.6 and significant deblending improvement. Astrometric accuracy is not distorted, therefore, the feasibility of the technique for astrometric projects is validated. We apply the deconvolution process to a set of images from the recently refurbished Baker-Nunn camera at Rothney Astrophysical Observatory.
dc.format.extent2 p.
dc.format.mimetypeapplication/pdf
dc.identifier.idgrec552860
dc.identifier.issn0185-1101
dc.identifier.urihttps://hdl.handle.net/2445/228315
dc.language.isoeng
dc.publisherInstituto de Astronomi?a, Universidad Nacional Auto?noma de Me?xico.
dc.relation.isformatofReproducció del document publicat a: https://astronomia.unam.mx/journals/rmxac/article/view/2006rmxac..25...50f
dc.relation.ispartofRevista Mexicana de Astronomía y Astrofísica, 2006, vol. 25, p. 50-52
dc.relation.urihttps://astronomia.unam.mx/journals/rmxac/article/view/2006rmxac..25...50f
dc.rights(c) Instituto de Astronomía, Universidad Nacional Autónoma de México, 2006
dc.rights.accessRightsinfo:eu-repo/semantics/openAccess
dc.sourceArticles publicats en revistes (Física Quàntica i Astrofísica)
dc.subject.classificationRefracció astronòmica
dc.subject.classificationFotometria astronòmica
dc.subject.classificationTelescopis
dc.subject.otherAstronomical refraction
dc.subject.otherAstronomical photometry
dc.subject.otherTelescopes
dc.titleBenefits of Image Deconvolution in CCD Imagery
dc.typeinfo:eu-repo/semantics/article
dc.typeinfo:eu-repo/semantics/publishedVersion

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