The ARGO-YBJ experiment has been designed to decrease the energy threshold of typical Extensive Air Shower arrays by exploiting the high altitute location (Tibet, P. R. of China, 4300 m a.s.l.) and the full coverage.The lower energy limit of the detector (a few GeV) is reached with the single particle technique recording the counting rate at fixed time intervals. We present first results concerning the search for emission from Gamma-Ray Burst in coincidence with satellite detection.

Searching for emission from GRBs with the ARGO-YBJ detector

DE MITRI, IVAN
2006

Abstract

The ARGO-YBJ experiment has been designed to decrease the energy threshold of typical Extensive Air Shower arrays by exploiting the high altitute location (Tibet, P. R. of China, 4300 m a.s.l.) and the full coverage.The lower energy limit of the detector (a few GeV) is reached with the single particle technique recording the counting rate at fixed time intervals. We present first results concerning the search for emission from Gamma-Ray Burst in coincidence with satellite detection.
Cosmic Ray; Array Detector; Gamma Astronomy; Gamma Ray Burst; Extensive Air Shower
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.12571/802
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