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Comparison of LOPES data and CoREAS simulations using a full detector simulation (ICRC2013)

Authors :
Link, K.
Apel, W. D.
Arteaga-Velázquez, J. C.
Bähren, L.
Bekk, K.
Bertaina, M.
Biermann, P. L.
Blümer, J.
Bozdog, H.
Brancus, I. M.
Cantoni, E.
Chiavassa, A.
Daumiller, K.
Souza, V.
Di Pierro, F.
Doll, P.
Engel, R.
Falcke, H.
Fuchs, B.
Fuhrmann, D.
Gemmeke, H.
Grupen, C.
Haungs, A.
Heck, D.
Hörandel, J. R.
Horneffer, A.
Huber, D.
Huege, T.
Isar, P. G.
Kampert, K-H
Kang, D.
Krömer, O.
Kuijpers, J.
Łuczak, P.
Ludwig, M.
Mathes, H. J.
Melissas, M.
Morello, C.
Oehlschläger, J.
Palmieri, N.
Pierog, T.
Rautenberg, J.
Rebel, H.
Roth, M.
Rühle, C.
Saftoiu, A.
Schieler, H.
Schmidt, A.
Schröder, F. G.
Sima, O.
Toma, G.
Gian Carlo Trinchero
Weindl, A.
Wochele, J.
Zabierowski, J.
Zensus, J. A.
Source :
NASA Astrophysics Data System
Publication Year :
2013
Publisher :
arXiv, 2013.

Abstract

The LOPES experiment at the Karlsruhe Institute of Technology, Germany, has been measuring radio emission of air showers for almost 10 years. For a better understanding of the emission process a detailed comparison of data with simulations is necessary. This is possible using a newly developed detector simulation including all LOPES detector components. After propagating a simulated event through this full detector simulation a standard LOPES like event file is written. LOPES data and CoREAS simulations can then be treated equally and the same analysis software can be applied to both. This gives the opportunity to compare data and simulations directly. Furthermore, the standard analysis software can be used with simulations which provide the possibility to check the accuracy regarding reconstruction of air shower parameters. We point out the advantages and present first results using such a full LOPES detector simulation. A comparison of LOPES data and the Monte Carlo code CoREAS based on an analysis using this detector simulation is shown.<br />Comment: 4 pages, presented at the International Cosmic Ray Conference, Rio de Janeiro, 2013, paper ID 0844

Details

Database :
OpenAIRE
Journal :
NASA Astrophysics Data System
Accession number :
edsair.doi.dedup.....41fdbecc62dd673fada5ca8a0e0ea76c
Full Text :
https://doi.org/10.48550/arxiv.1308.2523