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A. Amara
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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 - LVI. Sensitivity to non-standard particle dark matter models
Euclid preparation - LVII. Observational expectations for redshift z < 7 active galactic nuclei in the Euclid Wide and Deep surveys
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