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Aida, R.; Allen, M.; Anderson, R.; Barcikowski, E.; Belz, J.W.; Bergman, D.R.; Blake, S.A.; Chiba, J.; Chikawa, M.; Cho, E.J.; Cho, W.R.; Fujii, H.; Fujii, T.; Fukuda, T.; Fukushima, M.; Hanlon, W.; Hayashi, Y.; Hayashida, N.; Hibino, K.; Hiyama, K.; Honda, K.; Iguchi, T.; Inoue, N.; Ishii, T.; Ishimori, R.; Ivanov, D.; Iwamoto, S.; Jui, C.C.H.; Kakimoto, F.; Kalashev, O.; Kanbe, T.; Kasahara, K.; Kawai, H.; Kawakami, S.; Kido, E.; Kim, J.H.; Kitamoto, K.; Kitamura, S.; Kobayashi, Y.; Kondo, Y.; Kuramoto, K.; Kuzmin, V.; Kwon, Y.J.; Machida, S.; Martens, K.; Matsuda, T.; Matsuyama, T.; Matthews, J.N.; Myers, I.; Miyata, K.; Murano, Y.; Nakamura, T.; Nonaka, T.; Ogio, S.; Ohoka, H.; Oki, K.; Oshima, A.; Ozawa, S.; Pshirkov, M.S.; Roh, S.Y.; Ryu, D.; Sakurai, N.; Sampson, A.L.; Shah, P.D.; Shibata, F.; Shibata, T.; Shimodaira, H.; Shin, B.K.; Smith, J.D.; Sokolsky, P.; Springer, R.W.; Stokes, B.T.; Stratton, S.R.; Stroman, T.A.; Suzuki, S.; Takahashi, Y.; Takeda, M.; Taketa, A.; Thomas, S.B.; Thomson, G.B.; Tinyakov, P.; Tkachev, I.; Tokuno, H.; Tomida, T.; Troitsky, S.; Tsunesada, Y.; Tsutsumi, K.; Uchihori, Y.; Ukai, H.; Wada, Y.; Wong, T.; Wood, M.; Yamakawa, Y.; Yamane, R.; Yamaoka, H.; Yamazaki, K.; Yoshida, S.; Yoshii, H.; Zollinger, R.; Zundel, Z.
Astroparticle physics, 12/2012, Letnik: 39-40Journal Article
► We show the first physics results from the Middle Drum detector for Telescope Array. ► We quantify a spectral and energy scale comparison between Middle Drum and HiRes-1. ► We quantify a comparison between Middle Drum monocular and hybrid observation. ► We justify the transfer of the HiRes energy scale to all of Telescope Array. The Telescope Array’s Middle Drum fluorescence detector was instrumented with telescopes refurbished from the High Resolution Fly’s Eye’s HiRes-1 site. The data observed by Middle Drum in monocular mode was analyzed via the HiRes-1 profile-constrained geometry reconstruction technique and utilized the same calibration techniques enabling a direct comparison of the energy spectra and energy scales between the two experiments. The spectrum measured using the Middle Drum telescopes is based on a three-year exposure collected between December 16, 2007 and December 16, 2010. The calculated difference between the spectrum of the Middle Drum observations and the published spectrum obtained by the data collected by the HiRes-1 site allows the HiRes-1 energy scale to be transferred to Middle Drum. The HiRes energy scale is applied to the entire Telescope Array by making a comparison between Middle Drum monocular events and hybrid events that triggered both Middle Drum and the Telescope Array’s scintillator ground array.
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Leto | Faktor vpliva | Izdaja | Kategorija | Razvrstitev | ||||
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JCR | SNIP | JCR | SNIP | JCR | SNIP | JCR | SNIP |
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Povezave do osebnih bibliografij avtorjev | Povezave do podatkov o raziskovalcih v sistemu SICRIS |
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Vir: Osebne bibliografije
in: SICRIS
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