Evolutionary Behaviour in the HOD from the VVDS Data

Details Evolutionary Behaviour in the HOD from the VVDS Data Evolutionary Behaviour in the HOD from the VVDS Data

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aas...20917106a&link_type=abstract

2007 AAS/AAPT Joint Meeting, American Astronomical Society Meeting 209, #171.06; Bulletin of the American Astronomical Society,

Astronomy and Astrophysics

Astronomy

Scientific paper

In the standard halo model, galaxy clustering can be explained in terms of the halo occupation model (HOD). The observed clustering of galaxies at different redshifts exhibits a 'break' in the traditional power-law slope. Using the language of the halo model, this departure from a power law can be succinctly described in terms of the one-halo and two-halo terms. We present the best fit HOD parameters of the clustering of galaxies in the Vimos-VLT Deep Survey (VVDS) upto redshift 1.5.

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