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tokens: The authors would like to thank the anonymous referee for useful comments and their colleagues of the SL2S and SLACS collaborations for many useful discussions as well as stimulating exchanges within the Euclid Strong Lensing Science Working Group. R.G. also acknowledges E. Bertin for valuable discussions about massive model fitting. This work was supported by the Centre National d’Études Spatiales (CNES) and the Programme National Cosmologie et Galaxies (PNCG). This research is based on observations obtained with MegaPrime/MegaCam, a joint project of CFHT and CEA/DAPNIA, a joint project of CFHT, Taiwan, Korea, Canada and France, at the Canada-France-Hawaii Telescope (CFHT) which is operated by the National Research Council (NRC) of Canada, the Institut National des Sciences de l’Univers of the Centre National de la Recherche Scientifique (CNRS) of France, and the University of Hawaii. This work is based in part on data products produced at TERAPIX and the Canadian Astronomy Data Centre.