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M. Douspis
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Euclid and KiDS-1000: Quantifying the impact of source-lens clustering on cosmic shear analyses⋆
Euclid preparation - LIV. Sensitivity to neutrino parameters
Euclid preparation - LV. Exploring the properties of proto-clusters in the Simulated Euclid Wide Survey
Euclid preparation - LVI. Sensitivity to non-standard particle dark matter models
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