The vimos-vlt deep survey: the dependence of clustering on galaxy stellar mass at 2~1

B. Mcneux, L. Guzzo, B. Gariili, O. Le Fevre, A. Polio, J. Blaizot, G. De Lucia, M. Boizoncila, F. Larnarcillc, L. Pozzetti, A. Cappi, A. Iovino, C. Marinoni, H. J. Mccrackcn, S. De La Torre, D. Bottini, V. Le Brun, D. Maccagnl, J. P. Picat, R. ScaramellaM. Scodeggio, L. Tressc, G. Vcttolani, U. Abbas, S. Arnouts, S. Bardclli, A. Bongiomo, S. Chariot, P. Ciliegi, T. Contini, O. Cucciatl, S. Foucaud, P. Ftanzetti, I. Gavignaud, O. Ilbert, B. Marano, A. Manure, R. Mcrighi, S. Paltani, R. Pello, M. Radovich, D. Vcrgani, G. Zamorani, E. Zucca

Resultado de la investigación: Contribución a los distintos tipos de conferenciaArtículorevisión exhaustiva

Resumen

We have investigated the dependence of galaxy clustering on their stellar mass at z~l, using the data from the VIMOS-VLT Deep Survey (WDS). We have measured the projected two- point correlation function of galaxies, tnP{rp) for a set of stellar mass selected samples at an effective redshift < z >= 0.85. We have control aud quantify all effects on galaxy clustering due to the incompleteness of our low mass samples. We find that more massive galaxies are more clustered When compared to similar results at ∗ ~ 0.1 in the SDSS: we observed no evolution of the projected correlation function for massive galaxies. These objects present a stronger linear bias at z ~ 1 with rcspcct to low mass galaxies. As expcctcd, massive objects at high redshift arc found in the highest pics of the dark matter density field.

Idioma originalInglés
Páginas223-226
Número de páginas4
EstadoPublicada - 1 ene 2018
Evento2008 43rd Rencontres de Moriond on Cosmology - La Thuile Val d'Aosta, Italia
Duración: 15 mar 200822 mar 2008

Conferencia

Conferencia2008 43rd Rencontres de Moriond on Cosmology
País/TerritorioItalia
CiudadLa Thuile Val d'Aosta
Período15/03/0822/03/08

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica

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