  The prompt emission of Gamma Ray Bursts (GRBs) is still an outstanding
question in the study of these cataclysmic events. Part of what makes GRBs
difficult to study is how unique each event seems to be. However, aggregating
many GRB observations and analyzing the population allows us to obtain a better
understanding of the emission mechanism that produces the observed prompt
emission. In this review, we outline some of the most prevalent correlations
that have emerged from GRB prompt emission observations and how these
correlations are interpreted in relation to GRB physical properties and prompt
emission models.
