Fig. 3

Clustering strength,
as a function of redshift for all galaxies with errors based on a bootstrap
estimate. The populations are split by mass, with triangles showing the
108.6 < M [h-1 M⊙] ≤
109.6 samples, squares 109.6 < M [h-1 M⊙] ≤
1010.6, ×’s 1010.6 < M [h-1 M⊙] ≤
1011 and circles M [h-1 M⊙]
> 1011. The curves give the
results of the galform model for the observed mass ranges, as indicated in
the legend. Results from Foucaud et al. (2010, grey
asterisks and crosses connected by dashed lines) and Wake et al. (2011, grey stars connected by dashed lines) are
also plotted.
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