Cosmic Ray Measurements with LOPES: Status and Recent Results (ARENA 2012)
F.G. Schr\"oder, W.D. Apel, J.C. Arteaga, L. B\"ahren, K. Bekk, M., Bertaina, P.L. Biermann, J. Bl\"umer, H. Bozdog, I.M. Brancus, A. Chiavassa,, K. Daumiller, V. de Souza, F. Di Pierro, P. Doll, R. Engel, H. Falcke, B., Fuchs, D. Fuhrmann, H. Gemmeke, C. Grupen, A. Haungs

TL;DR
LOPES is a digital radio array that measures cosmic-ray air showers, providing key data on arrival directions, energy, and shower development, with ongoing improvements and potential for future high-precision measurements.
Contribution
This paper updates the status of LOPES and demonstrates its capability to reconstruct primary cosmic-ray properties, highlighting the potential for next-generation experiments.
Findings
Arrival direction reconstructed with at least 0.65° precision
Energy reconstructed with at least 20% precision
Radio lateral distribution slope sensitive to shower development
Abstract
LOPES is a digital antenna array at the Karlsruhe Institute of Technology, Germany, for cosmic-ray air-shower measurements. Triggered by the co-located KASCADE-Grande air-shower array, LOPES detects the radio emission of air showers via digital radio interferometry. We summarize the status of LOPES and recent results. In particular, we present an update on the reconstruction of the primary-particle properties based on almost 500 events above 100 PeV. With LOPES, the arrival direction can be reconstructed with a precision of at least 0.65{\deg}, and the energy with a precision of at least 20 %, which, however, does not include systematic uncertainties on the absolute energy scale. For many particle and astrophysics questions the reconstruction of the atmospheric depth of the shower maximum, Xmax, is important, since it yields information on the type of the primary particle and its…
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