The VIMOS-VLT Deep Survey: Dependence of galaxy clustering on stellar mass

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dc.creatorMeneux, B.
dc.creatorGuzzo, L.
dc.creatorGarilli, B.
dc.creatorFevre, O. Le
dc.creatorPollo, A.
dc.creatorBlaizot, J.
dc.creatorDe Lucia, G.
dc.creatorBolzonella, M.
dc.creatorLamareille, F.
dc.creatorPozzetti, L.
dc.creatorteam, the VVDS
dc.date2008-05-15
dc.date.accessioned2026-07-07T09:39:07Z
dc.date.available2026-07-07T09:39:07Z
dc.descriptionWe have investigated the dependence of galaxy clustering on their stellar mass at z~1, using the data from the VIMOS-VLT Deep Survey (VVDS). We have measured the projected two-point correlation function of galaxies, wp(rp) for a set of stellar mass selected samples at an effective redshift <z>=0.85. We have control and 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 z~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 respect to low mass galaxies. As expected, massive objects at high redshift are found in the highest pics of the dark matter density field.
dc.description4 pages, 2 figures, 43rd Rencontres de Moriond - March 15-22, 2008 - La Thuile (Val d'Aosta, Italy)
dc.identifierhttps://arxiv.org/abs/0805.2319
dc.identifierhttp://arxiv.org/abs/0805.2319
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/161050
dc.subjectAstrophysics
dc.titleThe VIMOS-VLT Deep Survey: Dependence of galaxy clustering on stellar mass
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