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

Open Access

Fig. 5.

Parameter constraints for the KiDS-like set-up using all parameters (lower corner) and with fixed nuisance parameters (upper corner), either for a data vector including SLC (red and pink) or without SLC (dark blue and cyan). Constraints for all sampled parameters can be found in Tables 3 and 4.

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