Jinn-Ouk Gong - February 2, 2016 Features in the primordial spectra I will discuss the features potentially present in the correlation functions of the primordial perturbation produced during cosmic inflation. After addressing the importance of features that can reflect non-trivial inflationary dynamics, I will discuss how features can arise and how we can compute the correlation functions with analytic control. Then I will present the model independent correlation between the power spectrum and bispectrum, and suggest where the signal of the bispectrum would be maximized based on the CMB temperature anisotropy data.