Table 4: Clustering length and slope of the correlation function $w_{\rm p}(r_{\rm p})$ for the different samples in the redshift range z=[0.5-1.2]. Values are derived for $0.2\le r_{\rm p}\le 21~h^{-1}$ Mpc. Associated errors have been extrapolated from the variance measured among 40 mocks catalogues for each stellar mass range. Values have not been corrected by underestimate due to stellar mass incompleteness.
Sample $\log~(M/M_\odot)$ r0(h-1 Mpc) $\gamma $
D1 9.0-9.5 $\rm 2.55_{-0.25}^{+0.25}$ $\rm 1.65_{-0.12}^{+0.13}$
D2 9.5-10.0 $\rm 3.45_{-0.31}^{+0.32}$ $\rm 1.79_{-0.14}^{+0.14}$
D3 10.0 -10.5 $\rm 3.54_{-0.34}^{+0.33}$ $\rm 1.88_{-0.15}^{+0.16}$
D4 10.5-11.0 $\rm 4.35_{-0.47}^{+0.46}$ $\rm 1.96_{-0.24}^{+0.27}$
I1 $\ge $9.0 $\rm 2.76_{-0.15}^{+0.17}$ $\rm 1.67_{-0.07}^{+0.08}$
I2 $\ge $9.5 $\rm 3.24_{-0.20}^{+0.21}$ $\rm 1.77_{-0.08}^{+0.09}$
I3 $\ge $10.0 $\rm 3.72_{-0.27}^{+0.29}$ $\rm 1.88_{-0.12}^{+0.12}$
I4 $\ge $10.5 $\rm 4.28_{-0.45}^{+0.43}$ $\rm 2.28_{-0.27}^{+0.28}$


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