The ARGO-YBJ Detector and high energy GRBs
| dc.creator | YBJ collaboration | |
| dc.date | 1999-04-27 | |
| dc.date.accessioned | 2026-07-07T02:31:25Z | |
| dc.date.available | 2026-07-07T02:31:25Z | |
| dc.description | 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. | |
| dc.description | 3 pages, 1 figure, accepted for publication in Astronomy and Astrophysics, Suppl. Series, proc. of the workshop "Gamma Ray Bursts in the Afterglow Era" | |
| dc.identifier | https://arxiv.org/abs/astro-ph/9904373 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/9904373 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/14143 | |
| dc.subject | Astrophysics | |
| dc.title | The ARGO-YBJ Detector and high energy GRBs | |
| dc.type | text |