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Upcoming Weak Lensing (WL) surveys can be used to constrain Dark Energy (DE)properties, namely if tomographic techniques are used to improve theirsensitivity. In this work, we use a Fisher matrix technique to compare thepower of CMB anisotropy and polarization data with tomographic WL data, inconstraining DE parameters. Adding WL data to available CMB data improves thedetection of all cosmological parameters, but the impact is really strong whenDE--DM coupling is considered, as WL tomography can then succeed to reduce theerrors on some parameters by factors >10.

Gravitational Lensing Constraints on Dynamical and Coupled Dark Energy