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Upper limit on the flux of photons with energies above 10^19 eV using the Telescope Array surface detector

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arxiv 1304.5614 v2 pith:LURHTBRX submitted 2013-04-20 astro-ph.HE hep-exhep-ph

T. Abu-Zayyad , R. Aida , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J.W. Belz , D.R. Bergman
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S.A. Blake R. Cady B.G. Cheon J. Chiba M. Chikawa E.J. Cho W.R. Cho H. Fujii T. Fujii T. Fukuda M. Fukushima D. Gorbunov W. Hanlon K. Hayashi Y. Hayashi N. Hayashida K. Hibino K. Hiyama K. Honda T. Iguchi D. Ikeda K. Ikuta N. Inoue T. Ishii R. Ishimori D. Ivanov S. Iwamoto C.C.H. Jui K. Kadota F. Kakimoto O. Kalashev T. Kanbe K. Kasahara H. Kawai S. Kawakami S. Kawana E. Kido H.B. Kim H.K. Kim J.H. Kim K. Kitamoto S. Kitamura Y. Kitamura K. Kobayashi Y. Kobayashi Y. Kondo K. Kuramoto V. Kuzmin Y.J. Kwon J. Lan S.I. Lim S. Machida K. Martens T. Matsuda T. Matsuura T. Matsuyama J.N. Matthews M. Minamino K. Miyata Y. Murano I. Myers K. Nagasawa S. Nagataki T. Nakamura S.W. Nam T. Nonaka S. Ogio M. Ohnishi H. Ohoka K. Oki D. Oku T. Okuda A. Oshima S. Ozawa I.H. Park M.S. Pshirkov D.C. Rodriguez S.Y. Roh G.I. Rubtsov D. Ryu H. Sagawa N. Sakurai A.L. Sampson L.M. Scott P.D. Shah F. Shibata T. Shibata H. Shimodaira B.K. Shin J.I. Shin T. Shirahama J.D. Smith P. Sokolsky B.T. Stokes S.R. Stratton T. Stroman S. Suzuki Y. Takahashi M. Takeda A. Taketa M. Takita Y. Tameda H. Tanaka K. Tanaka M. Tanaka S.B. Thomas G.B. Thomson P. Tinyakov I. Tkachev H. Tokuno T. Tomida S. Troitsky Y. Tsunesada K. Tsutsumi Y. Tsuyuguchi Y. Uchihori S. Udo H. Ukai G. Vasiloff Y. Wada T. Wong M. Wood Y. Yamakawa R. Yamane H. Yamaoka K. Yamazaki J. Yang Y. Yoneda S. Yoshida H. Yoshii X. Zhou R. Zollinger Z. Zundel
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keywords photonsabovearraydetectorenergiesfluxsurfacetelescope
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We search for ultra-high energy photons by analyzing geometrical properties of shower fronts of events registered by the Telescope Array surface detector. By making use of an event-by-event statistical method, we derive upper limits on the absolute flux of primary photons with energies above 10^19, 10^19.5 and 10^20 eV based on the first three years of data taken.

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