Table 5: Measured values of the linear bias for the VVDS and SDSS samples, within 3 stellar mass ranges (see text).
Sample $\log~(M/M_\odot)$ b(z)

SDSS ( $z\sim 0.15$ ) VVDS ( ${z\sim 0.85}$ )

D2 9.5-10.0 $1.26\pm 0.03$ $1.29\pm 0.10$

D3 10.0-10.5 $1.37\pm 0.03$ $1.32\pm 0.12$

D4 10.5-11.0 $1.40\pm 0.03$ $1.62\pm 0.18$

**Table 5:** Measured values of the linear bias for the VVDS and SDSS samples, within 3 stellar mass ranges (see text).
Sample	$\log~(M/M_\odot)$	b(z)
		SDSS ( $z\sim 0.15$ )	VVDS ( ${z\sim 0.85}$ )
D2	9.5-10.0	$1.26\pm 0.03$	$1.29\pm 0.10$
D3	10.0-10.5	$1.37\pm 0.03$	$1.32\pm 0.12$
D4	10.5-11.0	$1.40\pm 0.03$	$1.62\pm 0.18$

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