Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses

Open Access

Fig. 3.

Fractional difference between ξ₊ modelled with HMCode-2020 (red, dashed) and the EuclidEmulator (black, dash-dotted) to the measurements in the FS2 for sources at 0.9 < z < 1.2. The blue area corresponds to the KiDS-1000 uncertainty and the yellow area to the Euclid uncertainty. The correlation function is binned here in 10 logarithmic bins between 1 $\overset{'}{.}$ $\overset{\prime }{.}$ 25 and 83′.

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