TeV Observations of Gamma-Ray Bursts

Details TeV Observations of Gamma-Ray Bursts TeV Observations of Gamma-Ray Bursts

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aps..apr4a3007m&link_type=abstract

American Physical Society, April Meeting, Jointly Sponsored with the High Energy Astrophysics Division (HEAD) of the American As

Astronomy and Astrophysics

Astrophysics

Scientific paper

Many of the recent advances in our understanding of GRBs has come from the discovery and observations of counterparts at wavelengths other than those traditionally associated with GRBs. Ground based detectors sensitive at energies above 100 GeV play a crucial role in the extension of the observed spectrum of prompt and afterglow emission from gamma-ray bursts to energies above those attainable by satellite based instruments. I will describe current detectors and future prospects for making TeV observations of both the prompt and afterglow phases of gamma-ray bursts and discuss the the scientific questions we hope to address with these observations.

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