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Fig. 6.

image

Relative difference between the best-fit KV450 two-point shear correlation functions of the fiducial likelihood and the best fit after the iterative calibration of cosmological and nuisance parameters: ξ+ (upper right) and ξ (lower left). Black data points illustrate the relative difference between the observed two-point shear correlation functions and the best fit of the fiducial likelihood.

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