The first Gamma-Ray Burst (GRB) catalog presented by the Fermi-Large Area
Telescope (LAT) collaboration includes 28 GRBs, detected above 100 MeV over the
first three years since the launch of the Fermi mission. However, more than 100
GRBs are expected to be found over a period of six years of data collection
thanks to a new detection algorithm and to the development of a new LAT event
reconstruction, the so-called "Pass 8." Our aim is to provide revised prospects
for GRB alerts in the CTA era in light of these new LAT discoveries. We focus
initially on the possibility of GRB detection with the Large Size Telescopes
(LSTs). Moreover, we investigate the contribution of the Middle Size Telescopes
(MSTs), which are crucial for the search of larger areas on short post trigger
timescales. The study of different spectral components in the prompt and
afterglow phase, and the limits on the Extragalactic background light are
highlighted. Different strategies to repoint part of - or the entire array -
are studied in detail
