LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low

Cosmic-ray air shower detection with the low-frequency part of the Square Kilometre Array (SKA) radio telescope is envisioned to yield very high precision measurements of the particle composition of cosmic rays between 1016 and 1018 eV. This is made possible by the extreme antenna density of the core of SKA-Low, surpassing the current most dense radio air shower observatory LOFAR by over an order of magnitude. In order to make these measurements, the technical implementation of this observation mode and the development of reconstruction methods have to happen hand in hand. As a first lower limit of what is obtainable, we apply the current most precise reconstruction methods as used at LOFAR to a first complete simulation of air shower signals for the SKA-Low array. We describe this simulation setup and discuss the obtainable accuracy and resolution. A special focus is put on effects of the dynamic range of the system, beam-forming methods to lower the energy threshold, as well as the limits to the mass composition accuracy given by statistical and systematic uncertainties.

Authors

Institutions

Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-06-22
DOI
https://doi.org/10.1103/l8mt-994v
Citations
2
Primary Topic
Astrophysics and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
3.74

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low

T. Huege, O. Schölten, S. Thoudam, M. Desmet et al.
2 citations
Physical review. D/Physical review. D.
Astrophysics and Cosmic Phenomena
3.74
article

LOFAR-style reconstruction of cosmic-ray air showers with SKA-Low

T. Huege, O. Schölten, S. Thoudam, M. Desmet, P. Laub, Sjoerd Bouma, A. Corstanje, K. Terveer, A. Nelles, Katharine Mulrey, S. Buitink, J.R. Hörandel, K. Watanabe
article en
2 citations

Abstract

Cosmic-ray air shower detection with the low-frequency part of the Square Kilometre Array (SKA) radio telescope is envisioned to yield very high precision measurements of the particle composition of cosmic rays between 1016 and 1018 eV. This is made possible by the extreme antenna density of the core of SKA-Low, surpassing the current most dense radio air shower observatory LOFAR by over an order of magnitude. In order to make these measurements, the technical implementation of this observation mode and the development of reconstruction methods have to happen hand in hand. As a first lower limit of what is obtainable, we apply the current most precise reconstruction methods as used at LOFAR to a first complete simulation of air shower signals for the SKA-Low array. We describe this simulation setup and discuss the obtainable accuracy and resolution. A special focus is put on effects of the dynamic range of the system, beam-forming methods to lower the energy threshold, as well as the limits to the mass composition accuracy given by statistical and systematic uncertainties.

Physical review. D/Physical review. D.Vol. 112(2)
Karlsruhe Institute of Technology (DE), Vrije Universiteit Brussel (BE), Radboud University Nijmegen (NL), University of Groningen (NL), Khalifa University of Science and Technology (AE), Friedrich-Alexander-Universität Erlangen-Nürnberg (DE), Deutsches Elektronen-Synchrotron DESY (DE), National Institute for Subatomic Physics (NL)
Deutsche Forschungsgemeinschaft, Bundesministerium für Bildung und Forschung, Fonds Wetenschappelijk Onderzoek, Ministerium für Wissenschaft, Forschung und Kunst Baden-Württemberg, Khalifa University of Science, Technology and Research
Sustainable cities and communities, Climate action
Openalex Percentile: Top 8%
Astrophysics and Cosmic Phenomena
3.74
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.