TY - JOUR
T1 - Hotspot Update, and a new Excess of Events on the Sky Seen by the Telescope Array Experiment
AU - Telescope Array Collaboration
AU - Kim, Jihyun
AU - Ivanov, Dmitri
AU - Kawata, Kazumasa
AU - Sagawa, Hiroyuki
AU - Thomson, Gordon
AU - Abbasi, R. U.
AU - Abu-Zayyad, T.
AU - Allen, M.
AU - Arai, Y.
AU - Arimura, R.
AU - Barcikowski, E.
AU - Belz, J. W.
AU - Bergman, D. R.
AU - Blake, S. A.
AU - Buckland, I.
AU - Cady, R.
AU - Cheon, B. G.
AU - Chiba, J.
AU - Chikawa, M.
AU - Fujii, T.
AU - Fujisue, K.
AU - Fujita, K.
AU - Fujiwara, R.
AU - Fukushima, M.
AU - Fukushima, R.
AU - Furlich, G.
AU - Gonzalez, R.
AU - Hanlon, W.
AU - Hayashi, M.
AU - Hayashida, N.
AU - Hibino, K.
AU - Higuchi, R.
AU - Honda, K.
AU - Ikeda, D.
AU - Inadomi, T.
AU - Inoue, N.
AU - Ishii, T.
AU - Ito, H.
AU - Ivanov, D.
AU - Iwakura, H.
AU - Iwasaki, A.
AU - Jeong, H. M.
AU - Jeong, S.
AU - Jui, C. C.H.
AU - Kadota, K.
AU - Kakimoto, F.
AU - Kalashev, O.
AU - Kasahara, K.
AU - Kasami, S.
AU - Kwon, Y. J.
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The Telescope Array (TA) experiment, the largest observatory studying ultrahigh energy cosmic rays in the northern hemisphere, has reported an excess in the arrival direction distribution for events with energies above 5.7 × 1019 eV, called the hotspot. We report here the latest results of the TA hotspot using the most recent data measured by the TA surface detector array, which is more than doubled exposure since the first publication; the hotspot still exists with 3 sigma post-trial significance. By using an oversampling search with a 20◦-circle, similar to the study of the hotspot, we find an additional excess of events at slightly lower energies. The Perseus-Pisces supercluster lies at the location of the new excess. Assuming this structure is responsible for the excess, we conducted a statistical analysis to verify the correlation between observed events and the members of the Perseus-Pisces supercluster.
AB - The Telescope Array (TA) experiment, the largest observatory studying ultrahigh energy cosmic rays in the northern hemisphere, has reported an excess in the arrival direction distribution for events with energies above 5.7 × 1019 eV, called the hotspot. We report here the latest results of the TA hotspot using the most recent data measured by the TA surface detector array, which is more than doubled exposure since the first publication; the hotspot still exists with 3 sigma post-trial significance. By using an oversampling search with a 20◦-circle, similar to the study of the hotspot, we find an additional excess of events at slightly lower energies. The Perseus-Pisces supercluster lies at the location of the new excess. Assuming this structure is responsible for the excess, we conducted a statistical analysis to verify the correlation between observed events and the members of the Perseus-Pisces supercluster.
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M3 - Conference article
AN - SCOPUS:85145262606
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 328
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -