Fig. 5
Comparison of the fractional bias of ξ ± for a survey with limiting magnitude 
and a magnitude cut for the galaxies that are used for shape measurements of rSDSS = 25 (solid lines), to the bias for a survey where 
(dashed lines). For both cases, the HLR criterion with α = 2 was used. Thick curves display the case without seeing, thin curves the case with 
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