Milagro Search for VHE Emission from GRBs in the Swift Era

Details Milagro Search for VHE Emission from GRBs in the Swift Era Milagro Search for VHE Emission from GRBs in the Swift Era

2006-11-14

arxiv.org/abs/astro-ph/0611457v1

Nuovo Cim.B121:1573-1575,2006

Astronomy and Astrophysics

Astrophysics

Proceedings of Conference: "Swift and GRBs: Unveiling the relativistic Universe", held in Venice, 5-9 June 2006. To appear in

Scientific paper

10.1393/ncb/i2007-10301-3

Since its launch, in late 2004, Swift has been locating gamma-ray bursts (GRBs) at a rate of $\sim$100 per year. The rapid localization and follow-up in many wavelengths is providing new insights and revealing new, and unexpected phenomena, such as bright X-ray flares. Very high energy (VHE) emission ($>$100 GeV) is predicted by several models. Here, we present the results of a search for VHE emission from the most recent GRBs to fall within the Milagro field of view.

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