“…If there is a certain assumption, constraint or structure that we want to impose on the power spectrum of each source, we can employ a parametric model to represent σ 2 j (n, f ) instead of individually treating σ 2 j (n, f ) as a free parameter, or introduce a properly designed prior distribution over σ 2 j (n, f ). Choices include a Gaussian mixture model (GMM) (Attias, 2003), a hidden Markov model (HMM) (Higuchi and Kameoka, 2015), an autoregressive (AR) model (Déger-ine and Zaïdi, 2004;Yoshioka et al, 2011), a nonnegative matrix/tensor factorization (NMF) model (Ozerov and Févotte, 2010;Arberet et al, 2010;Ozerov et al, 2011;Sawada et al, 2013;Nikunen and Virtanen, 2014;Kitamura et al, 2015), an excitation-filter model (also known as source-filter model) Ozerov et al, 2012), a spectral continuity prior (Duong et al, 2011), a deep neural network (DNN) model (Nugraha et al, 2016), and combinations of different models (Ozerov et al, 2012;Adiloğlu and Vincent, 2016), among others. These models are presented in detail in Section 1.2.1.…”