GP-40
Milagro is a TeV observatory with a field of view of
1 sr that
operates 24 hours/day. On average 3 BATSE-detected bursts are within
Milagro's field of view each month. This new technique for TeV astronomy
was proven with a smaller detector, Milagrito, which operated from Feb 1997
to April 1998. Milagrito observed Mrk 501 (Atkins et al. Ap J in press),
the shadow of the moon, and searched 54 BATSE-detected bursts
for TeV emission (McEnery et al this symposium). Milagro began
operation within the last few months and should have over a factor of 5
greater sensitivity than Milagrito.
Fifth Huntsville Gamma Ray Burst Symposium
Hunsville, Alabama, USA
18-22 October, 1999