Revised absolute amplitude calibration of the LOPES experiment

K. Link , T. Huege , W.D. Apel , J.C. Arteaga-Vel\'azquez , L. B\"ahren , K. Bekk , M. Bertaina , P.L. Biermann

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J. Bl\"umer H. Bozdog I.M. Brancus E. Cantoni A. Chiavassa K. Daumiller V. de Souza F. Di Pierro P. Doll R. Engel H. Falcke B. Fuchs H. Gemmeke C. Grupen A. Haungs D. Heck R. Hiller J.R. H\"orandel A. Horneffer D. Huber P.G. Isar K-H. Kampert D. Kang O. Kr\"omer J. Kuijpers P. {\L}uczak M. Ludwig H.J. Mathes M. Melissas C. Morello J. Oehlschl\"ager N. Palmieri T. Pierog J. Rautenberg H. Rebel M. Roth C. R\"uhle A. Saftoiu H. Schieler A. Schmidt S. Schoo F.G. Schr\"oder O. Sima G. Toma G.C. Trinchero A. Weindl J. Wochele J. Zabierowski J.A. Zensus

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classification 🌌 astro-ph.IM astro-ph.HEhep-exphysics.ins-det

keywords lopescalibrationamplituderadiosignalsimulationsabsolutecoreas

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One of the main aims of the LOPES experiment was the evaluation of the absolute amplitude of the radio signal of air showers. This is of special interest since the radio technique offers the possibility for an independent and highly precise determination of the energy scale of cosmic rays on the basis of signal predictions from Monte Carlo simulations. For the calibration of the amplitude measured by LOPES we used an external source. Previous comparisons of LOPES measurements and simulations of the radio signal amplitude predicted by CoREAS revealed a discrepancy of the order of a factor of two. A re-measurement of the reference calibration source, now performed for the free field, was recently performed by the manufacturer. The updated calibration values lead to a lowering of the reconstructed electric field measured by LOPES by a factor of $2.6 \pm 0.2$ and therefore to a significantly better agreement with CoREAS simulations. We discuss the updated calibration and its impact on the LOPES analysis results.

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Revised absolute amplitude calibration of the LOPES experiment

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