[72.04] COSMOS: Clustering evolution from z=1.5

AAS 205th Meeting, 9-13 January 2005
Session 72 First Results from HST Cosmic Evolution Survey
Special Session, Tuesday, January 11, 2005, 10:00-11:30am, Town and Country

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[72.04] COSMOS: Clustering evolution from z=1.5

O. Le Fevre (LAM- Marseille, France), L. Guzzo (OABr , Milan, Italy), B. Meneux (LAM-Marseille, France), A. Pollo (OABr, Milan, Italy), N. Scoville (Caltech), J.P. Kneib (LAM-Marseille, France), COSMOS Collaboration

We are presenting the evolution of the clustering of galaxies in the HST-COSMOS field, based on deep CFHT and SUBARU photometry. Photometric redshifts have been calibrated with spectroscopic redshifts. The correlation length of galaxies has been derived as a function of luminosity and type over a range of redshifts from z=0 to 1.5.

The author(s) of this abstract have provided an email address for comments about the abstract: olivier.lefevre@oamp.fr

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