Data Processing at the Pierre Auger Observatory

TL;DR

This paper describes the data processing techniques and software used at the Pierre Auger Observatory to analyze ultra-high-energy cosmic-ray air showers, including the use of GRID computing for simulations.

Contribution

It details the data processing pipeline, simulation methods, and physics results, highlighting advancements in handling large datasets and computational challenges.

Findings

Successful processing of extensive air shower data

Implementation of GRID computing for simulations

Achievement of significant physics results

Abstract

Cosmic-ray particles with ultra-high energies (above $10^{18}$ eV) are studied through the properties of extensive air showers which they initiate in the atmosphere. The Pierre Auger Observatory detects these showers with unprecedented exposure and precision and the collected data are processed via dedicated software codes. Monte Carlo simulations of extensive air showers are very computationally expensive, especially at the highest energies and calculations are performed on the GRID for this purpose. The processing of measured and simulated data is described, together with a brief list of physics results which have been achieved.