PoS - Proceedings of Science
Volume 362 - Multifrequency Behaviour of High Energy Cosmic Sources - XIII (MULTIF2019) - Astrophysics of High Energy Cosmic Sources
The Highlights of the Pierre Auger Observatory
L. Caccianiga*  on behalf of the Pierre Auger Collaboration
Full text: pdf
Pre-published on: November 23, 2020
Published on: December 03, 2020
The Pierre Auger Observatory, in Argentina, is the largest cosmic ray detector ever built. It has actively been taking data for more than 15 years now, and thanks to this detector we have a better understanding of the most energetic particles in the universe. We can now start to answer some of the most important questions, such as where do they come from? What are they? How do they interact with the atmosphere? In this proceedings a selection of the most important results of Auger from the past few years is presented, with particular focus on those of astrophysical interest.
DOI: https://doi.org/10.22323/1.362.0042
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