Constraints on Primordial non-Gaussianity from the Large-Scale Structure
Sefusatti, Emiliano (IPhT CEA/Saclay)

I will discuss how future large-scale structure observations can confirm or improve CMB contraints from Planck on primordial non-Gaussianity. I will focus on a complete analysis of galaxy correlators, that is a joint analysis of the galaxy power spectrum and bispectrum, taking into account different models for the primordial curvature bispectrum.