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arXiv · 1904.00300

Search for point sources of ultra-high energy photons with the Telescope Array surface detector

Telescope Array Collaboration·R. U. Abbasi·M. Abe·T. Abu-Zayyad·M. Allen·R. Azuma·E. Barcikowski·J. W. Belz·D. R. Bergman·S. A. Blake·R. Cady·B. G. Cheon·J. Chiba·M. Chikawa·A. diMatteo·T. Fujii·K. Fujita·R. Fujiwara·M. Fukushima·G. Furlich·W. Hanlon·M. Hayashi·Y. Hayashi·N. Hayashida·K. Hibino·K. Honda·D. Ikeda·N. Inoue·T. Ishii·R. Ishimori·H. Ito·D. Ivanov·H. M. Jeong·S. Jeong·C. C. H. Jui·K. Kadota·F. Kakimoto·O. Kalashev·K. Kasahara·H. Kawai·S. Kawakami·S. Kawana·K. Kawata·E. Kido·H. B. Kim·J. H. Kim·S. Kishigami·V. Kuzmin·M. Kuznetsov·Y. J. Kwon·K. H. Lee·B. Lubsandorzhiev·J. P. Lundquist·K. Machida·K. Martens·T. Matsuyama·J. N. Matthews·R. Mayta·M. Minamino·K. Mukai·I. Myers·S. Nagataki·K. Nakai·R. Nakamura·T. Nakamura·T. Nonaka·H. Oda·S. Ogio·M. Ohnishi·H. Ohoka·T. Okuda·Y. Omura·M. Ono·R. Onogi·A. Oshima·S. Ozawa·I. H. Park·M. S. Pshirkov·J. Remington·D. C. Rodriguez·G. Rubtsov·D. Ryu·H. Sagawa·R. Sahara·K. Saito·Y. Saito·N. Sakaki·T. Sako·N. Sakurai·L. M. Scott·T. Seki·K. Sekino·P. D. Shah·F. Shibata·T. Shibata·H. Shimodaira·B. K. Shin·H. S. Shin·J. D. Smith·P. Sokolsky
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Abstract

The surface detector (SD) of the Telescope Array (TA) experiment allows one to indirectly detect photons with energies of order $10^{18}$ eV and higher and to separate photons from the cosmic-ray background. In this paper we present the results of a blind search for point sources of ultra-high energy (UHE) photons in the Northern sky using the TA SD data. The photon-induced extensive air showers (EAS) are separated from the hadron-induced EAS background by means of a multivariate classifier based upon 16 parameters that characterize the air shower events. No significant evidence for the photon point sources is found. The upper limits are set on the flux of photons from each particular direction in the sky within the TA field of view, according to the experiment's angular resolution for photons. Average 95% C.L. upper limits for the point-source flux of photons with energies greater than $10^{18}$, $10^{18.5}$, $10^{19}$, $10^{19.5}$ and $10^{20}$ eV are $0.094$, $0.029$, $0.010$, $0.0073$ and $0.0058$ km$^{-2}$yr$^{-1}$ respectively. For the energies higher than $10^{18.5}$ eV, the photon point-source limits are set for the first time. Numerical results for each given direction in each energy range are provided as a supplement to this paper.

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Telescope Array Collaboration, R. U. Abbasi, M. Abe, T. Abu-Zayyad, M. Allen, R. Azuma, E. Barcikowski, J. W. Belz, D. R. Bergman, S. A. Blake, R. Cady, B. G. Cheon, J. Chiba, M. Chikawa, A. diMatteo, T. Fujii, K. Fujita, R. Fujiwara, M. Fukushima, G. Furlich, W. Hanlon, M. Hayashi, Y. Hayashi, N. Hayashida, K. Hibino, K. Honda, D. Ikeda, N. Inoue, T. Ishii, R. Ishimori, H. Ito, D. Ivanov, H. M. Jeong, S. Jeong, C. C. H. Jui, K. Kadota, F. Kakimoto, O. Kalashev, K. Kasahara, H. Kawai, S. Kawakami, S. Kawana, K. Kawata, E. Kido, H. B. Kim, J. H. Kim, S. Kishigami, V. Kuzmin, M. Kuznetsov, Y. J. Kwon, K. H. Lee, B. Lubsandorzhiev, J. P. Lundquist, K. Machida, K. Martens, T. Matsuyama, J. N. Matthews, R. Mayta, M. Minamino, K. Mukai, I. Myers, S. Nagataki, K. Nakai, R. Nakamura, T. Nakamura, T. Nonaka, H. Oda, S. Ogio, M. Ohnishi, H. Ohoka, T. Okuda, Y. Omura, M. Ono, R. Onogi, A. Oshima, S. Ozawa, I. H. Park, M. S. Pshirkov, J. Remington, D. C. Rodriguez, G. Rubtsov, D. Ryu, H. Sagawa, R. Sahara, K. Saito, Y. Saito, N. Sakaki, T. Sako, N. Sakurai, L. M. Scott, T. Seki, K. Sekino, P. D. Shah, F. Shibata, T. Shibata, H. Shimodaira, B. K. Shin, H. S. Shin, J. D. Smith, P. Sokolsky. 2019-03-30. Search for point sources of ultra-high energy photons with the Telescope Array surface detector. https://doi.org/10.1093/mnras%2Fstz3618

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