Cosmic ray detection with the LOFAR radio telescope

K. Terveer*, S. Bouma, S. Buitink, A. Corstanje, M. Desmet, H. Falcke, B. M. Hare, J. R. Hörandel, T. Huege, N. Karastathis, P. Laub, K. Mulrey, A. Nelles, O. Scholten, P. Turekova, S. Thoudam, G. Trinh, S. ter Veen

*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceedingConference contributionAcademicpeer-review

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Abstract

The LOw Frequency ARray (LOFAR) has successfully measured cosmic rays for over a decade now. With its dense core of antenna fields in the Netherlands, it is an ideal tool for studying the radio emission from extensive air showers in the 1016 eV to 1018.5 eV range. Every air shower is measured with a small particle detector array and hundreds of antennas, which sets LOFAR apart from other air shower arrays. We present our current achievements and progress in reconstruction, interpolation, and software development during the final phases of measurement of LOFAR 1.0, before the LOFAR array gets a significant upgrade, including also plans for the final data release and refined analyses.

Original languageEnglish
Title of host publication10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities
EditorsAustin Cummings, Cosmin Deaconu, Grant Drager, Tim Huege, Robert Lahmann, Marco Stein Muzio, Anna Nelles, Philipp Windischhofer, Stephanie Wissel
PublisherSISSA
Number of pages8
DOIs
Publication statusPublished - 7-Nov-2024
Event10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2024 - Chicago, United States
Duration: 11-Jun-202414-Jun-2024

Publication series

NameProceedings of Science
Volume470
ISSN (Print)1824-8039

Conference

Conference10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2024
Country/TerritoryUnited States
CityChicago
Period11/06/202414/06/2024

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