We report a laboratory investigation of weak turbulence of water surface waves in the gravitycapillary crossover. By using time-space resolved profilometry and a bicoherence analysis, we observe that the nonlinear processes involve 3-wave resonant interactions. By studying the solutions of the resonance conditions we show that the nonlinear interaction is dominantly 1D and involves collinear wave vectors. Furthermore taking into account the spectral widening due to weak nonlinearity explains that nonlocal interactions are possible between a gravity wave and high frequency capillary ones. We observe also that nonlinear 3-wave coupling is possible among gravity waves and we raise the question of the relevance of this mechanism for oceanic waves.A large ensemble of nonlinear waves can exchange energy and develop a turbulent state. The statistic properties of such wave turbulence have been described theoretically for weak nonlinearity in the framework of the Weak Turbulence Theory (WTT). In this theory, only resonant waves are able to exchange significant amounts of energy over long times due to the weak nonlinear coupling. The predicted phenomenology of the stationary statistical states resembles that of fluid turbulence: energy is injected at large scales and cascades down scale to wavelengths at which dissipation takes over and absorbs energy into heat. A major difference with fluid turbulence is that analytical predictions for the stationary spectra (and other statistical quantities) can be derived for weak wave turbulence For isotropic systems, the predicted energy spectrum E(k) has the following expressionwhere k = |k| is the wavenumber, P the energy flux, C a dimensional constant that can be calculated and α the spectral exponent. N is the number of waves taking part in the resonances. Usually N − 1 corresponds to the order of the nonlinear coupling term of the wave equation (N = 3 for quadratic nonlinearities, N = 4 for cubic ones,...). The waves have then to satisfy the resonance conditions such as k 1 = k 2 + k 3 and ω 1 = ω 2 + ω 3 (for 3-wave interaction). In some cases, these resonances conditions do not have solutions. This is the case in particular for gravity waves at the surface of water. The dispersion relation (for infinite depth) is ω = √ gk and its negative curvature does not allow for solutions of the resonance conditions for 3 waves. Thus the resonances are expected to involve 4 waves. At small wavelengths, water waves are capillary waves for which the dispersion relation is ω = γ ρ 1/2 k 3/2 whose curvature allows for 3-wave resonances (γ is the surface tension and ρ the density). The predicted spectra for water waves are thus expected to be E(k) ∝ P 1/2 k −7/4 for capillary waves and E(k) ∝ P 1/3 k −5/2 [2] for gravity waves. Laboratory experiments largely fail to reproduce this predictions, in particular for the gravity waves. In large or small waves tanks, the spectral exponent of the gravity waves is seen to vary strongly with the forcing intensity and to be close to the WTT predictions a...