PoS - Proceedings of Science
Volume 301 - 35th International Cosmic Ray Conference (ICRC2017) - Session Cosmic-Ray Indirect. CRI-instrumentation EAS
ALPAQUITA Array in the ALPACA Project
K. Kawata*, T. Asaba, K. Hibino, N. Hotta, M. Kataoka, Y. Katayose, C. Kato, H. Kojima, R. Mayta, P. Miranda, K. Munakata, Y. Nakamura, M. Nishizawa, S. Ogio, M. Ohnishi, A. Oshima, M. Raljevich, H. Rivera, T. Saito, T.K. Sako, T. Sasaki, S. Shibata, A. Shiomi, M. Subieta, M. Suzuki, N. Tajima, M. Takita, Y. Tameda, K. Tanaka, R. Ticona, H. Tsuchiya, Y. Tsunesada, S. Udo, M. Wakamatsua  on behalf of the ALPACA collaborationet al. (click to show)
Full text: pdf
Pre-published on: August 16, 2017
Published on: August 03, 2018
We are now proposing a new project which consists of a large air shower array (83,000 m^2) and a muon detector array (5,400 m^2) located at the altitude of 4,740 m near La Paz in Bolivia to observe 100 TeV gamma rays in the southern sky. The ALPAQUITA array is a prototype air shower array which will be constructed at the ALPACA site. This array consists of 45 scintillation counters of 1 m^2 in area each, and its effective area is approximately 8,000 m^2 (1/10 of ALPACA air shower array). In the present paper, we report on the current status and the performance of the ALPAQUITA array
DOI: https://doi.org/10.22323/1.301.0437
How to cite

Metadata are provided both in "article" format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in "proceeding" format which is more detailed and complete.

Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.