Email this article Chemical Composition of Ultrahigh-Energy Cosmic Rays from the Telescope Array Surface Detector Data
- Authors: Zhezher Y.V.1,2
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Affiliations:
- Institute for Nuclear Research, Russian Academy of Sciences
- Faculty of Physics, Moscow State University
- Issue: Vol 83, No 8 (2019)
- Pages: 1008-1009
- Section: Article
- URL: https://journals.rcsi.science/1062-8738/article/view/187501
- DOI: https://doi.org/10.3103/S1062873819080409
- ID: 187501
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Abstract
Results are presented from investigating the chemical composition of ultrahigh-energy cosmic rays using data from the Telescope Array experiment, obtained at its surface detector array over nine years. The analysis is based on the boosted decision tree approach, which uses 14 observables sensitive to the composition of cosmic rays.
About the authors
Ya. V. Zhezher
Institute for Nuclear Research, Russian Academy of Sciences; Faculty of Physics, Moscow State University
Author for correspondence.
Email: zhezher.yana@physics.msu.ru
Russian Federation, Moscow, 142190; Moscow, 119991
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