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dc.creatorAndreon, S.
dc.creatorWillis, J.
dc.creatorQuintana, H.
dc.date.accessioned2020-08-04T21:50:54Z
dc.date.available2020-08-04T21:50:54Z
dc.date.issued2004
dc.identifier.urihttp://hdl.handle.net/10533/242517
dc.description.abstractThe XMM–LSS project is detecting distant clusters of low mass, quite comparablein mass to the ones in the local universe. This allows a direct comparison of galaxy propertiesat different redshifts in “similar” clusters. We present here first results on the
dc.language.isoeng
dc.relationinstname: ANID
dc.relationreponame: Repositorio Digital RI2.0
dc.relation.urihttps://www.researchgate.net/publication/1799110_Galaxy_evolution_in_clusters_from_z1_to_z0
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleGalaxy evolution in clusters from z=1 to z=0
dc.typeCapitulo de libro
dc.bibliographicCitation.stpage367
dc.bibliographicCitation.endpage371
dc.identifier.folio15010003
dc.description.conicytprogramFONDAP
dc.rights.driverinfo:eu-repo/semantics/openAccess
dc.type.driverinfo:eu-repo/semantics/bookPart
dc.description.shortconicytprogramFONDAP
dc.title.libroIAU Colloquium 195
dc.publisher.editorDiaferio, A.
dc.description.centroCENASTRO


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