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Bezyazeekov, P.A.; Budnev, N.M.; Gress, O.A.; Haungs, A.; Hiller, R.; Huege, T.; Kazarina, Y.; Kleifges, M.; Konstantinov, E.N.; Korosteleva, E.E.; Kostunin, D.; Krömer, O.; Kuzmichev, L.A.; Lubsandorzhiev, N.; Mirgazov, R.R.; Monkhoev, R.; Pakhorukov, A.; Pankov, L.; Prosin, V.V.; Rubtsov, G.I.; Schröder, F.G.; Wischnewski, R.; Zagorodnikov, A.
Journal of cosmology and astroparticle physics, 01/2016, Letnik: 2016, Številka: 1Journal Article
We reconstructed the energy and the position of the shower maximum of air showers with energies E ∼> 100 PeV applying a method using radio measurements performed with Tunka-Rex. An event-to-event comparison to air-Cherenkov measurements of the same air showers with the Tunka-133 photomultiplier array confirms that the radio reconstruction works reliably. The Tunka-Rex reconstruction methods and absolute scales have been tuned on CoREAS simulations and yield energy and X{sub max} values consistent with the Tunka-133 measurements. The results of two independent measurement seasons agree within statistical uncertainties, which gives additional confidence in the radio reconstruction. The energy precision of Tunka-Rex is comparable to the Tunka-133 precision of 15%, and exhibits a 20% uncertainty on the absolute scale dominated by the amplitude calibration of the antennas. For X{sub max}, this is the first direct experimental correlation of radio measurements with a different, established method. At the moment, the X{sub max} resolution of Tunka-Rex is approximately 40 g/cm{sup 2}. This resolution can probably be improved by deploying additional antennas and by further development of the reconstruction methods, since the present analysis does not yet reveal any principle limitations.
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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in: SICRIS
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