Recent highlights from ARGO-YBJ
Di Sciascio Giuseppe (on behalf of the ARGO-YBJ Collaboration) (INFN -, Sezione Roma Tor Vergata, Roma, Italy)

TL;DR
This paper summarizes recent results from the ARGO-YBJ experiment, which has collected extensive data over five years to address open questions in cosmic ray physics and gamma-ray astronomy.
Contribution
It provides an overview of the latest findings from ARGO-YBJ in gamma-ray astronomy and cosmic ray physics, highlighting new insights gained from five years of data.
Findings
Detection of gamma-ray sources in the TeV range
Measurements of cosmic ray energy spectra
Insights into cosmic ray composition and origin
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^2). With a duty-cycle greater than 86% the detector collected about 5 X 10^{11} events in a wide energy range, from few hundreds GeV up to the 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 gamma-ray astronomy and in cosmic ray physics
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Particle Accelerators and Free-Electron Lasers
