The nature of assembly bias - I. Clues from a ΛCDM cosmology

dc.date.accessioned2020-03-11T20:36:13Z
dc.date.accessioned2022-10-18T23:03:00Z
dc.date.available2020-03-11T20:36:13Z
dc.date.available2022-10-18T23:03:00Z
dc.date.created2020-03-11T20:36:13Z
dc.date.issued2011
dc.identifierhttp://hdl.handle.net/10533/240899
dc.identifier15010003
dc.identifierWOS:000288549900046
dc.identifierno scielo
dc.identifiereid=2-s2.0-79952722400
dc.identifier.urihttps://repositorioslatinoamericanos.uchile.cl/handle/2250/4472238
dc.description.abstractWe present a new proxy for the overdensity peak height for which the large-scale clustering of haloes of a given mass does not vary significantly with the assembly history. The peak height, usually taken to be well represented by the virial mass, can inst
dc.languageeng
dc.relationhttps://doi.org/10.1111/j.1365-2966.2010.17988.x
dc.relation10.1111/j.1365-2966.2010.17988.x
dc.rightsinfo:eu-repo/semantics/openAccess
dc.rightsAtribución-NoComercial-SinDerivadas 3.0 Chile
dc.rightshttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/
dc.titleThe nature of assembly bias - I. Clues from a ΛCDM cosmology
dc.typeArticulo


Este ítem pertenece a la siguiente institución