The VIMOS Ultra Deep Survey : luminosity and stellar mass dependence of galaxy clustering at z \sim 3

We present the study of the dependence of galaxy clustering on luminosity and stellar mass in the redshift range 2$ $L)=1.92+25.36(L/L$^*$)$^{7.01}$. We conclude our study with measurements of stellar-to-halo mass ratio (SHMR) of the stellar mass selected sub-samples.