A new revolution in GRB observation and theory has begun over the last 1.5 years since the launch of the Fermi gamma-ray space telescope. The new window into high energy gamma-rays opened by the Fermi-LAT is providing insight into prompt emission mechanisms and possibly also afterglow physics. The LAT detected GRBs appear to be a new unique subset of extremely energetic and bright bursts. In this talk, I will discuss the context and recent discoveries from these LAT GRBs, and the large database of broadband observations collected by Swift over the last 5 years and how through comparisons between the Swift, GBM, and LAT GRB samples, we can learn about the unique characteristics and relationships between each population.