  Gamma-ray bursts (GRBs) have been detected up to GeV energies and are
predicted by many models to emit in the very high energy (VHE, > 100 GeV)
regime too. Detection of such emission would allow us to constrain GRB models.
Since its launch, in late 2004, the Swift satellite has been locating GRBs at a
rate of approximately 100 per year. The rapid localization and follow-up in
many wavelengths has revealed new and unexpected phenomena, such as delayed
emission in the form of bright X-ray flares. The Milagro gamma-ray observatory
is a wide field of view (2 sr) instrument employing a water Cherenkov detector
to continuously ($>$ 90% duty cycle) observe the overhead sky in the 100 GeV to
100 TeV energy range. Over 100 GRBs are known to have been in the field of view
of Milagro since January 2000, including 57 since the launch of Swift (through
May 2007). We discuss the results of the searches for prompt emission from
these bursts, as well as for delayed emission from the X-ray flares observed in
some of the Swift bursts.
