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  • Schmitz, M. A.; Starck, J.-L.; Ngole Mboula, F.; Auricchio, N.; Brinchmann, Jarle; Capobianco, R. I. Vito; Clédassou, Rodolphe; Conversi, L.; Corcione, L.; Fourmanoit, N.; Frailis, M.; Garilli, B.; Hormuth, F.; Hu, D.; Israel, H.; Kermiche, S.; Kitching, Thomas D.; Kubik, B.; Kunz, Martin; Ligori, S.; Lilje, Per Barth; Lloro, Ivan; Mansutti, O.; Marggraf, O.; Massey, R. J.; Pasian, F.; Pettorino, V.; Raison, F.; Rhodes, Jason D.; Roncarelli, M.; Saglia, R. P.; Schneider, Peter; Serrano, S.; Taylor, A. N.; Toledo-Moreo, Rafael; Valenziano, L.; Vuerli, C.; Zoubian, J. (Journal article / Tidsskriftartikkel / PublishedVersion; Peer reviewed, 2020)
    Context. Future weak lensing surveys, such as the Euclid mission, will attempt to measure the shapes of billions of galaxies in order to derive cosmological information. These surveys will attain very low levels of statistical ...