Evolution of clustering length , large-scale bias , and host halo mass at 2 < z < 5 in the VIMOS Ultra Deep Survey ( VUDS ) ,

Abstract

We investigate the evolution of galaxy clustering for galaxies in the redshift range 2.0 < z < 5.0 using the VIMOS Ultra Deep Survey (VUDS). We present the projected (real-space) two-point correlation function wp(rp) measured by using 3022 galaxies with robust spectroscopic redshifts in two independent fields (COSMOS and VVDS-02h) covering in total 0.8 deg… (More)

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