The ARGO-YBJ detector and high energy GRBs

Details The ARGO-YBJ detector and high energy GRBs The ARGO-YBJ detector and high energy GRBs

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999a%26as..138..597b&link_type=abstract

Astronomy and Astrophysics Supplement, v.138, p.597-598

Astronomy and Astrophysics

Astrophysics

6

Gamma-Ray: Bursts

Scientific paper

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 ~ 6500 m(2) 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 GeV /500 TeV. The sensitivity of ARGO-YBJ to detect high energy GRBs is presented.

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