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QSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at z similar to 0.7

dc.contributor.authorBonavera, Laura 
dc.contributor.authorGonzález-Nuevo González, Joaquín 
dc.contributor.authorSuárez Gómez, Sergio Luis 
dc.contributor.authorLapi, A.
dc.contributor.authorBianchini, F.
dc.contributor.authorNegrello, M.
dc.contributor.authorDíez Alonso, Enrique 
dc.contributor.authorSantos Rodríguez, Jesús Daniel 
dc.contributor.authorCos Juez, Francisco Javier de 
dc.date.accessioned2020-01-23T08:17:15Z
dc.date.available2020-01-23T08:17:15Z
dc.date.issued2019
dc.identifier.citationJournal Of Cosmology And Astroparticle Physics, 9, p. 21- (2019); doi:10.1088/1475-7516/2019/09/021
dc.identifier.issn1475-7516
dc.identifier.urihttp://hdl.handle.net/10651/53643
dc.format.extentp. 21-
dc.language.isoeng
dc.relation.ispartofJournal Of Cosmology And Astroparticle Physics
dc.rights©,
dc.sourceWOS:000485743700001
dc.titleQSOs sigposting cluster size halos as gravitational lenses: halo mass, projected mass density profile and concentration at z similar to 0.7
dc.typeinfo:eu-repo/semantics/article
dc.identifier.doi10.1088/1475-7516/2019/09/021
dc.type.dcmitext
dc.relation.publisherversionhttp://dx.doi.org/10.1088/1475-7516/2019/09/021


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