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Systematic uncertainty in the analysis of the TA fluorescence detector from fluorescence yield modelsopen access

Authors
Komori, KoheiTameda, YuichiroSato, ShomaTakagi, YutaroKusumori, YukiIwagami, HiraiOgio, ShoichiFujita, KeitaroTomida, TakayukiAbbasi, R.U.Abe, Y.Abu-Zayyad, T.Allen, M.Arai, Y.Arimura, R.Barcikowski, E.Belz, J.W.Bergman, D.R.Blake, S.A.Buckland, I.Cheon, B.G.Chikawa, M.Fedynitch, A.Fujii, T.Fujisue, K.Fujita, K.Fujiwara, R.Fukushima, M.Furlich, G.Gerber, Z.Globus, N.Hanlon, W.Hayashida, N.He, H.Hibi, R.Hibino, K.Higuchi, R.Honda, K.Ikeda, D.Inoue, N.Ishii, T.Ito, H.Ivanov, D.Iwasaki, A.Jeong, H.M.Jeong, S.Jui, C.C.H.Kadota, K.Kakimoto, F.Kalashev, O.Kasahara, K.Kasami, S.Kawakami, S.Kawata, K.Kharuk, I.Kido, E.Kim, H.B.Kim, J.H.Kim, J.H.Kim, S.W.Kimura, Y.Komae, I.Komori, K.Kuznetsov, M.Kwon, Y.J.Lee, K.H.Lee, M.J.Lubsandorzhiev, B.Lundquist, J.P.Matsuyama, T.Matthews, J.A.Matthews, J.N.Mayta, R.Miyashita, K.Mizuno, K.Mori, M.Murakami, M.Myers, I.Nagataki, S.Nakai, K.Nakamura, T.Nishio, E.Nonaka, T.Ogio, S.Ohoka, H.Okazaki, N.Oku, Y.Okuda, T.Omura, Y.Onishi, M.Ono, M.Oshima, A.Oshima, H.Ozawa, S.Park, I.H.Park, K.Y.Potts, M.Pshirkov, M.S.Remington, J.Rodriguez, D.C.Rott, C.Rubtsov, G.I.Ryu, D.Sagawa, H.Saito, R.Sakaki, N.Sako, T.Sakurai, N.Sato, D.Sato, K.Sato, S.Sekino, K.Shah, P.D.Shibata, N.Shibata, T.Shikita, J.Shimodaira, H.Shin, B.K.Shin, H.S.Shinto, D.Smith, J.D.Sokolsky, P.Stokes, B.T.Stroman, T.A.Takagi, Y.Takahashi, K.Takamura, M.Takeda, M.Takeishi, R.Taketa, A.Takita, M.Tanaka, K.Tanaka, M.Thomas, S.B.Thomson, G.B.Tinyakov, P.Tkachev, I.Tokuno, H.Tomida, T.Troitsky, S.Tsuda, R.Tsunesada, Y.Udo, S.Urban, F.Vaiman, I.A.Warren, D.Wong, T.Yamazaki, K.Yashiro, K.Yoshida, F.Zhezher, Y.Zundel, Z.
Issue Date
Sep-2024
Citation
Proceedings of Science, v.444, pp 1 - 10
Pages
10
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
444
Start Page
1
End Page
10
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/204180
DOI
10.22323/1.444.0330
ISSN
1824-8039
Abstract
Currently, ultra-high energy cosmic rays (UHECRs) are being measured by the Telescope Array (TA) and Pierre Auger (Auger) experiments. There are differences in the energy spectra measured by TA and Auger. One reason for this difference is systematic uncertainty in the energy determination. The fluorescence yield model, which consists of fluorescence emission efficiencies and spectra, is one of the most significant components of this systematic uncertainty. Fluorescence emission efficiencies and spectra have been measured by various experiments, and different measurements are currently used to determine the energy of the TA and Auger experiments. In this study, we estimate the influence of the fluorescence yield model on the systematic uncertainty in the energy determination of the TA fluorescence detector.
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