dc.date.accessioned | 2020-03-11T20:36:13Z | |
dc.date.accessioned | 2022-10-18T23:03:00Z | |
dc.date.available | 2020-03-11T20:36:13Z | |
dc.date.available | 2022-10-18T23:03:00Z | |
dc.date.created | 2020-03-11T20:36:13Z | |
dc.date.issued | 2011 | |
dc.identifier | http://hdl.handle.net/10533/240899 | |
dc.identifier | 15010003 | |
dc.identifier | WOS:000288549900046 | |
dc.identifier | no scielo | |
dc.identifier | eid=2-s2.0-79952722400 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/4472238 | |
dc.description.abstract | We 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.language | eng | |
dc.relation | https://doi.org/10.1111/j.1365-2966.2010.17988.x | |
dc.relation | 10.1111/j.1365-2966.2010.17988.x | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.rights | Atribución-NoComercial-SinDerivadas 3.0 Chile | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/3.0/cl/ | |
dc.title | The nature of assembly bias - I. Clues from a ΛCDM cosmology | |
dc.type | Articulo | |