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Effect of optical properties of FDs on reconstruction analysisopen access

Authors
Sato, DaikiTomida, TakayukiHibi, RyosukeMatuzawa, AoiTameda, YuichiroIkeda, DaisukeAbbasi, 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.Kusumori, Y.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.Tameda, Y.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 - 8
Pages
8
Indexed
SCOPUS
Journal Title
Proceedings of Science
Volume
444
Start Page
1
End Page
8
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/204173
DOI
10.22323/1.444.0227
ISSN
1824-8039
Abstract
The TA experiment uses fluorescence telescopes to observe cosmic ray air showers. The telescope camera uses PMTs as Pixels. The telescope's PMT pointing direction has an uncertainty of 0.1°, and more precise measurements of the telescope's optical properties are needed to more accurately reconstruct the cosmic ray air showers. We have developed the Opt-copter which is a light source mounted on a drone that can be flown within the telescope's field of view. Observational experiments with the Opt-copter have provided a more accurate analysis of the telescope viewing direction. In this study, we estimate the effect of this measurement of accurate telescope viewing direction on the reconstruction of cosmic ray air showers.
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