Performance and extensions of the central data acquisition system for Phase II of the Pierre Auger Observatory
Paul Filip (for the Pierre Auger Collaboration)

TL;DR
This paper reviews the central data acquisition system of the Pierre Auger Observatory, analyzing its performance during Phase II, discussing challenges, and presenting recent system improvements to enhance data collection and analysis of ultra-high-energy cosmic rays.
Contribution
It provides a detailed assessment of the Phase II data acquisition system's performance and introduces recent software and system updates to improve data collection efficiency.
Findings
Higher event detection rates in Phase II compared to Phase I
Improved data purity and efficiency metrics
System updates streamline data acquisition process
Abstract
The Pierre Auger Observatory is a hybrid detector designed to observe and study ultra-high-energy particles of extraterrestrial origin. With its 27 fluorescence telescopes and over 1600 autonomously operating water-Cherenkov detectors spread over an area of 3000 km, it is world-leading in terms of exposure to cosmic rays and offers an unparalleled window into the physical processes that happen at energy scales unattainable by particle accelerators on Earth. Measurement information of candidate air-shower events from all associated detectors and telescopes is collected at a central data-acquisition system located in the nearby town of Malarg\"ue, and processed for higher-level physics analysis. On top of this, data for monitoring the long-term stability and operation of the observatory is forwarded to the central server as well. In this work, we briefly review the central…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Dark Matter and Cosmic Phenomena · Neutrino Physics Research
