Testing a Reported Correlation between Arrival Directions of Ultra-high-energy Cosmic Rays and a Flux Pattern from nearby Starburst Galaxies using Telescope Array Data

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초록

The Pierre Auger Collaboration (Auger) recently reported a correlation between the arrival directions of cosmic rays with energies above 39 EeV and the flux pattern of 23 nearby starburst galaxies (SBGs). In this Letter, we tested the same hypothesis using cosmic rays detected by the Telescope Array experiment (TA) in the 9 yr period from 2008 May to 2017 May. Unlike the Auger analysis, we did not optimize the parameter values but kept them fixed to the best-fit values found by Auger, namely 9.7% for the anisotropic fraction of cosmic rays assumed to originate from the SBGs in the list and 12 degrees.9 for the angular scale of the correlations. The energy threshold that we adopted is 43 EeV, corresponding to 39 EeV in Auger when taking into account the energy-scale difference between two experiments. We find that the TA data is compatible with isotropy to within 1.1 sigma and with the Auger result to within 1.4 sigma, meaning that it is not capable to discriminate between these two hypotheses.

키워드

astroparticle physicscosmic raysgalaxies: starburstmethods: data analysisANISOTROPY
제목
Testing a Reported Correlation between Arrival Directions of Ultra-high-energy Cosmic Rays and a Flux Pattern from nearby Starburst Galaxies using Telescope Array Data
저자
Abbasi, R. U.Abe, M.Abu-Zayyad, T.Allen, M.Azuma, R.Barcikowski, E.Belz, J. W.Bergman, D. R.Blake, S. A.Cady, R.Cheon, Byung GuChiba, J.Chikawa, M.di Matteo, A.Fujii, T.Fujita, K.Fukushima, M.Furlich, G.Goto, T.Hanlon, W.Hayashi, M.Hayashi, Y.Hayashida, N.Hibino, K.Honda, K.Ikeda, D.Inoue, N.Ishii, T.Ishimori, R.Ito, H.Ivanov, D.Jeong, H. M.Jeong, S.Jui, C. C. H.Kadota, K.Kakimoto, F.Kalashev, O.Kasahara, K.Kawai, H.Kawakami, S.Kawana, S.Kawata, K.Kido, E.Kim, Hang BaeKim, J. H.Kishigami, S.Kitamura, S.Kitamura, Y.Kuzmin, VKuznetsov, M.Kwon, Y. J.Lee, K. H.Lubsandorzhiev, B.Lundquist, J. P.Machida, K.Martens, K.Matsuyama, T.Matthews, J. N.Mayta, R.Minamino, M.Mukai, K.Myers, INagasawa, K.Nagataki, S.Nakamura, R.Nakamura, T.Nonaka, T.Oda, H.Ogio, S.Ogura, J.Ohnishi, M.Ohoka, H.Okuda, T.Omura, Y.Ono, M.Onogi, R.Oshima, A.Ozawa, S.Park, I. H.Pshirkov, M. S.Remington, J.Rodriguez, D. C.Rubtsov, G.Ryu, D.Sagawa, H.Sahara, R.Saito, K.Saito, Y.Sakaki, N.Sakurai, N.Scott, L. M.Seki, T.Sekino, K.Shah, P. D.Shibata, F.Shibata, T.Shimodaira, H.Shin, B. K.Shin, H. S.Smith, J. D.Sokolsky, P.Stokes, B. T.Stratton, S. R.Stroman, T. A.Suzawa, T.Takagi, Y.Takahashi, Y.Takamura, M.Takeda, M.Takeishi, R.Taketa, A.Takita, M.Tameda, Y.Tanaka, H.Tanaka, K.Tanaka, M.Thomas, S. B.Thomson, G. B.Tinyakov, P.Tkachev, ITokuno, H.Tomida, T.Troitsky, S.Tsunesada, Y.Tsutsumi, K.Uchihori, Y.Udo, S.Urban, F.Wong, T.Yamamoto, M.Yamane, R.Yamaoka, H.Yamazaki, K.Yang, J.Yashiro, K.Yoneda, Y.Yoshida, S.Yoshii, H.Zhezher, Y.Zundel, Z.
DOI
10.3847/2041-8213/aaebf9
발행일
2018-11
유형
Article
저널명
Astrophysical Journal Letters
867
2
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1 ~ 5