Fig. 14

Normalised cosmic variance
as a function of n1 for samples selected in
B-band luminosity. The inverted triangles are
those samples without a luminosity ratio imposed, and the triangles are those with a
luminosity ratio applied (Table 8). Points at
the same number density are offset when needed to avoid overlap. The dashed line
marks the error-weighted average of
,
. The coloured area
shows its 68% confidence interval. The grey area marks the 15% uncertainty expected
from our parametrisation of the cosmic variance. A colour version of this plot is
available in the electronic edition.
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