CFHTLenS: a Gaussian likelihood is a sufficient approximation for a cosmological analysis of third-order cosmic shear statistics

P. Simon^*, E. Semboloni, L. van Waerbeke, H. Hoekstra, T. Erben, L. Fu, J. Harnois-Deraps, C. Heymans, H. Hildebrandt, M. Kilbinger, T. D. Kitching, L. Miller, T. Schrabback

^*Corresponding author for this work