Table 4: Number of galaxies and mean B rest-frame absolute magnitude (h=1) of the sample separated using the color bimodality. The number of "red'' and "blue'' galaxies classified as early (T1&2) and late (T3&4) spectral types are identified. We note that the populations of "red'' and T1&2 as well as the populations of "blue'' and T3&4 galaxies are mostly the same, except for a significant cross-over population which could explain the observed difference in clustering (see text).

Redshift	Red		Blue
range	T1&2	T3&4	T1&2	T3&4
0.2-0.5	221	49	86	895
	-18.181	-16.403	-18.701	-17.411
0.5-0.7	253	24	121	1044
	-18.892	-17.646	-19.215	-18.467
0.7-0.9	313	42	77	965
	-19.713	-18.468	-19.748	-19.138
0.9-1.2	283	13	88	1016
	-20.263	-19.314	-20.557	-19.679
1.2-2.0	41	0	94	480
	-20.926	0	-21.078	-20.567