Latest results from the ARGO-YBJ experiment
Giuseppe Di Sciascio (INFN, Sezione Roma Tor Vergata) (for the, ARGO-YBJ Collaboration)
TL;DR
The ARGO-YBJ experiment, operational for five years at high altitude, collected extensive cosmic ray and gamma-ray data, providing new insights into cosmic ray physics and gamma-ray astronomy.
Contribution
This paper presents the latest results from ARGO-YBJ, highlighting new findings in cosmic ray physics and gamma-ray astronomy based on five years of data.
Findings
Extensive data collection over five years with high duty-cycle.
New insights into cosmic ray energy spectrum and composition.
Results relevant to gamma-ray sources and astrophysical phenomena.
Abstract
The ARGO-YBJ experiment has been in stable data taking for 5 years at the YangBaJing Cosmic Ray Observatory (Tibet, P.R. China, 4300 m a.s.l., 606 g/cm). With a duty-cycle greater than 86\% the detector collected about 510 events in a wide energy range, from few hundreds GeV up to about 10 PeV. A number of open problems in cosmic ray physics has been faced exploiting different analyses. In this paper we summarize the latest results in cosmic ray physics and in gamma-ray astronomy.
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