  Observation of Gamma Ray Bursts (GRBs) in the Very High Energy (VHE) domain
will provide important information on the physical conditions in GRB outflows.
The MAGIC telescope is the best suited Imaging Atmospheric Cherenkov Telescope
(IACT) for these observations. Thanks to its fast repositioning time and low
energy threshold, MAGIC is able to start quickly the follow-up observation,
triggered by an alert from the GRB Coordinates Network (GCN), and observe the
prompt emission and early afterglow phase from GRBs. In the last two years of
operation several GRB follow-up observations were performed by MAGIC, however,
until now without successful detection of VHE gamma rays above threshold
energies >100 GeV. In this paper we revise the expectations for the GRB
observations with MAGIC, based on the experience from the last years of
operation.

Astrophysics