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Cosmic ray detection with the LOFAR radio telescope

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arxiv 2410.07681 v1 pith:DCOVWCB5 submitted 2024-10-10 astro-ph.HE

K. Terveer , S. Bouma , S. Buitink , A. Corstanje , M. Desmet , H. Falcke , B. M. Hare , J. R. Hörandel
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T. Huege N. Karastathis P. Laub K. Mulrey A. Nelles O. Scholten P. Turekova S. Thoudam G. Trinh S. ter Veen
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keywords lofararraycosmicfinalmeasuredradioshowerachievements
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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 $10^{16}$ eV to $10^{18.5}$ 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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