ARGO-YBJ Highlights
G. Di Sciascio (on behalf of the ARGO-YBJ collaboration)
TL;DR
The ARGO-YBJ experiment, a high-altitude full-coverage detector, has been operational since 2007, providing significant results in gamma-ray astronomy and cosmic ray physics over three years.
Contribution
This paper presents the main findings from ARGO-YBJ's three years of data, highlighting its contributions to gamma-ray and cosmic ray studies.
Findings
Significant gamma-ray sources identified
Cosmic ray spectrum measurements obtained
Advancements in high-altitude detector performance
Abstract
The ARGO-YBJ experiment is a multipurpose detector exploiting the full-coverage approach at very high altitude. The apparatus is in stable data taking since November 2007 at the YangBaJing Cosmic Ray Laboratory (Tibet, P.R. China, 4300 m a.s.l., 606 g/cm). In this paper we report the main results in Gamma-Ray Astronomy and Cosmic Ray Physics after about 3 years of operations.
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