COSMOS: Clustering evolution from z=1.5

Astronomy and Astrophysics – Astronomy

Scientific paper

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Scientific paper

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.

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