Cosmic ray detection with the LOFAR radio telescope

Terveer K, Bouma S, Buitink S, Corstanje A, Desmet M, Falcke H, Hare BM, Hörandel JR, Huege T, Karastathis N, Laub P, Mulrey K, Nelles A, Scholten O, Turekova P, Thoudam S, Trinh G, ter Veen S (2024)


Publication Type: Conference contribution

Publication year: 2024

Journal

Publisher: Sissa Medialab Srl

Book Volume: 470

Conference Proceedings Title: Proceedings of Science

Event location: Chicago, IL US

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.

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How to cite

APA:

Terveer, K., Bouma, S., Buitink, S., Corstanje, A., Desmet, M., Falcke, H.,... ter Veen, S. (2024). Cosmic ray detection with the LOFAR radio telescope. In Proceedings of Science. Chicago, IL, US: Sissa Medialab Srl.

MLA:

Terveer, Karen, et al. "Cosmic ray detection with the LOFAR radio telescope." Proceedings of the 10th International Workshop on Acoustic and Radio EeV Neutrino Detection Activities, ARENA 2024, Chicago, IL Sissa Medialab Srl, 2024.

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