Clustering evolution of galaxies in the VIMOS-VLT Deep Survey

Details Clustering evolution of galaxies in the VIMOS-VLT Deep Survey Clustering evolution of galaxies in the VIMOS-VLT Deep Survey

Dec 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005sf2a.conf..663m&link_type=abstract

SF2A-2005: Semaine de l'Astrophysique Francaise, meeting held in Strasbourg, France, June 27 - July 1, 2005, Edited by F. Casoli

Astronomy and Astrophysics

Astrophysics

Scientific paper

The VIMOS-VLT Deep Survey (VVDS) is an on-going program to map the evolution of galaxies, large scale structures and AGNs from the redshift measurement of more than 100,000 objects down to a magnitude IAB=24, in combination with a multi-wavelength dataset from radio to X-rays. We present here the measurement and the evolution of the correlation function from the first epoch data, dividing the sample per spectral type, up to redshift ˜2.

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