Bibliographic Details
Title: |
Tunka-Rex: energy reconstruction with a single antenna station (ARENA 2016) |
Authors: |
Hiller, R., Bezyazeekov, P. A., Fedorov, N. M. Budnev, Gress, O. A., Haungs, A., Huege, T., Kazarina, Y., Kleifges, M., Korosteleva, E. E., Kostunin, D., Krömer, O., Kungel, V., Kuzmichev, L. A., Lubsandorzhiev, N., Mirgazov, R. R., Monkhoev, R., Osipova, E. A., Pakhorukov, A., Pankov, L., Prosin, V. V., Rubtsov, G. I., Schröder, F. G., Wischnewski, R., Zagorodnikov, A. |
Source: |
EPJ Web of Conferences 135 (2017) 01004 |
Publication Year: |
2016 |
Collection: |
Astrophysics |
Subject Terms: |
Astrophysics - Instrumentation and Methods for Astrophysics, Astrophysics - High Energy Astrophysical Phenomena |
More Details: |
The Tunka-Radio extension (Tunka-Rex) is a radio detector for air showers in Siberia. From 2012 to 2014, Tunka-Rex operated exclusively together with its host experiment, the air-Cherenkov array Tunka-133, which provided trigger, data acquisition, and an independent air-shower reconstruction. It was shown that the air-shower energy can be reconstructed by Tunka-Rex with a precision of 15\% for events with signal in at least 3 antennas, using the radio amplitude at a distance of 120\,m from the shower axis as an energy estimator. Using the reconstruction from the host experiment Tunka-133 for the air-shower geometry (shower core and direction), the energy estimator can in principle already be obtained with measurements from a single antenna, close to the reference distance. We present a method for event selection and energy reconstruction, requiring only one antenna, and achieving a precision of about 20\%. This method increases the effective detector area and lowers thresholds for zenith angle and energy, resulting in three times more events than in the standard reconstruction. |
Document Type: |
Working Paper |
DOI: |
10.1051/epjconf/201713501004 |
Access URL: |
http://arxiv.org/abs/1611.09614 |
Accession Number: |
edsarx.1611.09614 |
Database: |
arXiv |