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Fig. 12.


Additive bias, estimated as the mean ellipticity, for the entire galaxy sample (All) and for the five different tomographic bins (B1 through B5). Identical selection criteria has been applied to both the KV-450 data and to the simulations. The c1 terms are expected to differ due to the detector effects in the OmegaCAM data which are excluded in the simulations.

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