Fig. 5
Top three lines: the expected r.m.s. fluctuation of the curvature parameter, 
, for geometries resembling the 2dFGRS, the SDSS, and a full sky. The two lowest lines are the expected rms fluctuations of the parameters 
and 
for a full-sky survey extending to the respective redshift. The curvature fluctuations turn out to be higher than all other fluctuations.
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