ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimized to study small size air showers. It consists of a layer of Resistive Plate Counters (RPCs) covering an area of $\sim$ 6500 m2 and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m a.s.l. ARGO-YBJ will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics in the range $10~{\rm GeV} \div 500~{\rm TeV}$.The sensitivity of ARGO-YBJ to detect high energy GRBs is presented.

The ARGO-YBJ Detector and High Energy GRBs

BARONE, Fabrizio;
1999-01-01

Abstract

ARGO-YBJ (Astrophysical Radiation with Ground-based Observatory at YangBaJing) is a detector optimized to study small size air showers. It consists of a layer of Resistive Plate Counters (RPCs) covering an area of $\sim$ 6500 m2 and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m a.s.l. ARGO-YBJ will be devoted to a wide range of fundamental issues in cosmic rays and astroparticle physics, including in particular gamma-ray astronomy and gamma-ray bursts physics in the range $10~{\rm GeV} \div 500~{\rm TeV}$.The sensitivity of ARGO-YBJ to detect high energy GRBs is presented.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11386/1064374
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