The ARGO-YBJ Detector and high energy GRBs
Astrophysics
2007-05-23 v1
Abstract
ARGO-YBJ ia a detector optimized to study small size air showers. It consists of a layer of Resistive Plate counters (RPCs) covering an area of about 6500 m^2 and will be located in the Yangbajing Laboratory (Tibet, China) at 4300 m above the sea level. 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.
Cite
@article{arxiv.astro-ph/9904373,
title = {The ARGO-YBJ Detector and high energy GRBs},
author = {YBJ collaboration},
journal= {arXiv preprint arXiv:astro-ph/9904373},
year = {2007}
}
Comments
3 pages, 1 figure, accepted for publication in Astronomy and Astrophysics, Suppl. Series, proc. of the workshop "Gamma Ray Bursts in the Afterglow Era"