Abstract
While our current cosmological model places galaxy clusters at the nodes of a filament network (the cosmic web), we still struggle to detect these filaments at high redshifts. We perform a weak lensing study for a sample of 16 massive, medium-high redshift (0.4
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Martinet, N., Clowe, D., Durret, F., Adami, C., Acebrón, A., Hernandez-García, L., … Ulmer, M. (2016). Weak lensing study of 16 DAFT/FADA clusters: Substructures and filaments. Astronomy and Astrophysics, 590. https://doi.org/10.1051/0004-6361/201526444
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