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Separation of Noisy Astrophysical Images by Blind Time-Frequency Source Separation Methods

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dc.contributor.authorÖzgen, Mehmet Tankut
dc.contributor.authorD. Herranz
dc.contributor.authorErçan E. Kuruoğlu
dc.contributor.orcid0000-0003-3057-3857
dc.contributor.orcid0000-0003-4540-1417
dc.contributor.orcid0000-0002-2608-8034
dc.date.accessioned2025-11-13T21:24:22Z
dc.date.issued2007-06-01
dc.identifier.doihttps://doi.org/10.1109/siu.2007.4298795
dc.identifier.openalexW2077283366
dc.identifier.urihttps://hdl.handle.net/11421/13311
dc.identifier.urihttps://doi.org/10.1109/siu.2007.4298795
dc.language.isoen
dc.rightsrestrictedAccess
dc.subjectCosmic microwave background
dc.subjectPhysics
dc.subjectSource separation
dc.subjectIndependent component analysis
dc.subjectSynchrotron radiation
dc.subjectNoise (video)
dc.subjectBlind signal separation
dc.subjectGaussian
dc.subjectComponent (thermodynamics)
dc.subjectMicrowave
dc.subjectGaussian noise
dc.subjectImage (mathematics)
dc.subjectComputer science
dc.subjectAlgorithm
dc.subjectOptics
dc.subjectArtificial intelligence
dc.subjectAnisotropy
dc.titleSeparation of Noisy Astrophysical Images by Blind Time-Frequency Source Separation Methods
dc.typeArticle
dspace.entity.typePublication
local.authorid.openalexA5000800849

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