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Astrophysical image separation by blind time–frequency source separation methods

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dc.contributor.authorÖzgen, Mehmet Tankut
dc.contributor.authorErçan E. Kuruoğlu
dc.contributor.authorD. Herranz
dc.contributor.orcid0000-0003-3057-3857
dc.contributor.orcid0000-0002-2608-8034
dc.contributor.orcid0000-0003-4540-1417
dc.date.accessioned2025-11-13T11:16:38Z
dc.date.issued2008-01-17
dc.identifier.doihttps://doi.org/10.1016/j.dsp.2007.12.003
dc.identifier.endpage369
dc.identifier.issn1051-2004
dc.identifier.issue2
dc.identifier.openalexW2003713214
dc.identifier.startpage360
dc.identifier.urihttps://hdl.handle.net/11421/6270
dc.identifier.urihttps://doi.org/10.1016/j.dsp.2007.12.003
dc.identifier.volume19
dc.language.isoen
dc.relation.ispartofDigital Signal Processing
dc.rightsrestrictedAccess
dc.subjectCosmic microwave background
dc.subjectIndependent component analysis
dc.subjectBlind signal separation
dc.subjectComponent (thermodynamics)
dc.subjectPhysics
dc.subjectGaussian
dc.subjectSource separation
dc.subjectMicrowave
dc.subjectSynchrotron radiation
dc.subjectAlgorithm
dc.subjectImage (mathematics)
dc.subjectNoise (video)
dc.subjectSeparation (statistics)
dc.subjectComputer science
dc.subjectAstrophysics
dc.subjectComputational physics
dc.subjectArtificial intelligence
dc.subjectOptics
dc.titleAstrophysical image separation by blind time–frequency source separation methods
dc.typeArticle
dspace.entity.typePublication
local.authorid.openalexA5000800849

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