  The Milagro gamma-ray observatory employs a water Cherenkov detector to
observe extensive air showers produced by high energy particles interacting in
the Earth's atmosphere. Milagro has a wide field of view (2 sr) and high duty
cycle (> 90%) making it an ideal all-sky monitor of the northern hemisphere in
the 100 GeV to 100 TeV energy range. More than 45 satellite-triggered gamma-ray
bursts (GRBs) have occurred in the field of view of Milagro since January 2000,
with the rate of bursts increasing significantly with the launch of Swift. We
discuss the most recent results of a search for very high energy (VHE) emission
from these GRBs.
