The VIMOS-VLT deep survey: History of the galaxy clustering in the universe

Agnieszka Pollo, U. Abbas, B. Meneux, L. Guzzo, O. Le Fèvre, S. De La Torre, A. Cappi, B. Garilli, C. Marinoni, D. Bottini, V. Le Brun, D. Maccagni, M. Scodeggio, L. Tresse, G. Vettolani, A. Zanichelli, C. Adami, S. Arnouts, S. Bardelli, M. BolzonellaS. Charlot, P. Ciliegi, T. Contini, S. Foucaud, P. Franzetti, I. Gavignaud, O. Ilbert, A. Iovino, H. J. McCracken, A. Mazure, R. Merighi, S. Paltani, R. Pellò, L. Pozzetti, D. Vergani, G. Zamorani, E. Zucca

Producción científica: Contribución a los tipos de informe/libroContribución a la conferenciarevisión exhaustiva

Resumen

Star formation in galaxies and their evolution depends on their local environment and, more precisely, their location in the large scale structure. The data from the VIMOS-VLT Deep Survey (VVDS) has enabled us to investigate the history of the galaxy clustering and the relation between the evolution of galaxies themselves and the galaxy clustering back to z∼1. We analyzed the evolution of the projected two-point correlation function for particular galaxy classes, with different intrinsic luminosities and stellar masses. We concluded that the properties of central and satellite galaxies in the dark matter haloes could have changed significantly between z∼1 and now.

Idioma originalInglés
Título de la publicación alojadaHunting for the Dark
Páginas169-170
Número de páginas2
Volumen1240
DOI
EstadoPublicada - 2010
EventoInternational Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation" - Qawra, Malta
Duración: 19 oct. 200923 oct. 2009

Otros

OtrosInternational Conference "Hunting for the Dark: The Hidden Side of Galaxy Formation"
País/TerritorioMalta
CiudadQawra
Período19/10/0923/10/09

Áreas temáticas de ASJC Scopus

  • Física y Astronomía General

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