Research output: Contribution to conference › Paper › peer-review
Telescope Array Surface Detector Energy and Arrival Direction Estimation Using Deep Learning. / The Telescope Array Collaboration; Калашев, Олег Евгеньевич.
2022. Paper presented at 37th International Cosmic Ray Conference, ICRC 2021, Virtual, Berlin, Germany.Research output: Contribution to conference › Paper › peer-review
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TY - CONF
T1 - Telescope Array Surface Detector Energy and Arrival Direction Estimation Using Deep Learning
AU - The Telescope Array Collaboration
AU - Ivanov, D.
AU - Kuznetsov, M. Yu
AU - Rubtsov, G. I.
AU - Sako, T.
AU - Tsunesada, Y.
AU - Zhezher, Y. V.
AU - Abbasi, R. U.
AU - Abe, M.
AU - Abu-Zayyad, T.
AU - Allen, M.
AU - Arai, Y.
AU - Barcikowski, E.
AU - Belz, J. W.
AU - Bergman, D. R.
AU - Blake, S. A.
AU - Buckland, I.
AU - Cady, R.
AU - Cheon, B. G.
AU - Chiba, J.
AU - Chikawa, M.
AU - Fujii, T.
AU - Fujisue, K.
AU - Fujita, K.
AU - Fujiwara, R.
AU - Fukushima, M.
AU - Fukushima, R.
AU - Furlich, G.
AU - Gonzalez, R.
AU - Hanlon, W.
AU - Hayashi, M.
AU - Hayashida, N.
AU - Hibino, K.
AU - Higuchi, R.
AU - Honda, K.
AU - Ikeda, D.
AU - Inadomi, T.
AU - Inoue, N.
AU - Ishii, T.
AU - Ito, H.
AU - Ivanov, D.
AU - Iwakura, H.
AU - Jeong, H. M.
AU - Jeong, S.
AU - Jui, C. C.H.
AU - Kadota, K.
AU - Kakimoto, F.
AU - Kasahara, K.
AU - Kasami, S.
AU - Kawai, H.
AU - Kawakami, S.
AU - Калашев, Олег Евгеньевич
N1 - The cluster of the Theoretical Division of INR RAS was used for the numerical part of the work. The development and application of the machine learning analysis method is supported by the Russian Science Foundation grant No. 17-72-20291 (INR).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - A novel ultra-high-energy cosmic rays energy and arrival direction reconstruction method for Telescope Array surface detector is presented. The analysis is based on a deep convolutional neural network using detector signal time series as the input and the network is trained on a large Monte-Carlo dataset. This method is compared in terms of statistical and systematic energy and arrival direction determination errors with the standard Telescope Array surface detector event reconstruction procedure.
AB - A novel ultra-high-energy cosmic rays energy and arrival direction reconstruction method for Telescope Array surface detector is presented. The analysis is based on a deep convolutional neural network using detector signal time series as the input and the network is trained on a large Monte-Carlo dataset. This method is compared in terms of statistical and systematic energy and arrival direction determination errors with the standard Telescope Array surface detector event reconstruction procedure.
UR - https://www.scopus.com/inward/record.url?eid=2-s2.0-85144403106&partnerID=40&md5=e9e2462c78541edd1533fda7371a17f4
UR - https://www.mendeley.com/catalogue/7e76eb9d-b554-3d53-af80-6d02b8eb7304/
U2 - 10.22323/1.395.0252
DO - 10.22323/1.395.0252
M3 - Paper
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -
ID: 46054694