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dc.contributor.authorCroston, J.H.
dc.contributor.authorArnaud, M.
dc.contributor.authorPointecouteau, E.
dc.contributor.authorPratt, G.W.
dc.date.accessioned2008-09-29T09:00:40Z
dc.date.available2008-09-29T09:00:40Z
dc.date.issued2006
dc.identifier.citationCroston , J H , Arnaud , M , Pointecouteau , E & Pratt , G W 2006 , ' An improved deprojection and PSF-deconvolution technique for galaxy-cluster x-ray surface-brightness profiles ' , Astronomy & Astrophysics , vol. 459 , no. 3 , pp. 1007-1019 . https://doi.org/10.1051/0004-6361:20065795
dc.identifier.issn0004-6361
dc.identifier.otherPURE: 152187
dc.identifier.otherPURE UUID: 82981417-a1e8-4997-9b98-80d264dc8b33
dc.identifier.otherdspace: 2299/2401
dc.identifier.otherScopus: 36049020704
dc.identifier.urihttp://hdl.handle.net/2299/2401
dc.descriptionOriginal article can be found at: http://www.aanda.org/ Copyright The European Southern Observatory
dc.language.isoeng
dc.relation.ispartofAstronomy & Astrophysics
dc.subjectscaling properties
dc.subjectpoor clusters
dc.subjectmass profile
dc.subjectChandra
dc.titleAn improved deprojection and PSF-deconvolution technique for galaxy-cluster x-ray surface-brightness profilesen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1051/0004-6361:20065795
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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