The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (Tibet, P.R. China, 4300 m a.s.l.) and full coverage with Resistive Plate Counters, resulting in an energy threshold of a few hundred GeV. The large eld of view (2 sr) and high duty cycle allow the continuous monitoring of the Northern sky, searching for unknown sources and unpredictable events, such as ares in blazar emissions or high energy Gamma Ray Bursts. In this paper I will present some results obtained in -ray astronomy with the ARGO-YBJ experiment.

Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2010). Gamma-ray astronomy with the ARGO-YBJ experiment. JOURNAL OF PHYSICS. CONFERENCE SERIES, 203, 012119-012121 [10.1088/1742-6596/203/1/012119].

Gamma-ray astronomy with the ARGO-YBJ experiment

BUSSINO, Severino Angelo Maria;MARI, Stefano Maria;Montini P;Ruggieri F;
2010-01-01

Abstract

The ARGO-YBJ experiment is an Extensive Air Shower detector which combines high altitude location (Tibet, P.R. China, 4300 m a.s.l.) and full coverage with Resistive Plate Counters, resulting in an energy threshold of a few hundred GeV. The large eld of view (2 sr) and high duty cycle allow the continuous monitoring of the Northern sky, searching for unknown sources and unpredictable events, such as ares in blazar emissions or high energy Gamma Ray Bursts. In this paper I will present some results obtained in -ray astronomy with the ARGO-YBJ experiment.
Aielli, G., Bacci, C., Bartoli, B., Bernardini, P., Bi, X.j., Bleve, C., et al. (2010). Gamma-ray astronomy with the ARGO-YBJ experiment. JOURNAL OF PHYSICS. CONFERENCE SERIES, 203, 012119-012121 [10.1088/1742-6596/203/1/012119].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/117723
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