Towards a Cosmic-Ray Energy Scale with the Auger Engineering Radio Array

Pierre Auger Collaboration, Max Büsken, Stijn Buitink

Research output: Contribution to journalConference paper

1 Citation (Scopus)

Abstract

Radio detection of cosmic-ray (CR) induced extensive air showers with digital antenna arrays is
a matured technique by now. At the Pierre Auger Observatory, the Auger Engineering Radio
Array (AERA) has been measuring air-shower signals in conjunction with the particle detectors
of the surface detector (SD) for over ten years. For an absolute determination of the CR energy
with the Auger baseline detectors, the shower size estimator from the SD is calibrated with the
energy scale of the fluorescence detector (FD). However, AERA has an independent access to the
energy scale through the reconstructed radio signals. The hybrid detectors at the Pierre Auger
Observatory offer the unique opportunity to compare the two independent energy scales. In this
contribution, we present our envisaged methodology for cross-checking the agreement between
the energy scales of the FD and AERA using hybrid SD-AERA shower data and simulations.
We show individual steps of our radio signal reconstruction and highlight the key ingredients for
calibrated energy measurements
Original languageEnglish
Article number035
Number of pages8
JournalProceedings of Science
Volume470
Issue numberarena 2024
Publication statusPublished - 7 Nov 2024
Event10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities - William Eckhardt Research Center, Chicago
Duration: 11 Jun 202414 Jun 2024

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