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Telescope Array anisotropy summary

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dc.contributor.authorFujii, T.-
dc.contributor.authorIvanov, D.-
dc.contributor.authorJui, C.C.H.-
dc.contributor.authorKawata, K.-
dc.contributor.authorKim, J.H.-
dc.contributor.authorKuznetsov, M.Yu.-
dc.contributor.authorNonaka, T.-
dc.contributor.authorOgio, S.-
dc.contributor.authorRubtsov, G.I.-
dc.contributor.authorSagawa, H.-
dc.contributor.authorThomson, G.B.-
dc.contributor.authorTinyakov, P.G.-
dc.contributor.authorTkachev, I.-
dc.contributor.authorTroitsky, S.-
dc.contributor.authorAbbasi, R.U.-
dc.contributor.authorAbu-Zayyad, T.-
dc.contributor.authorAllen, M.-
dc.contributor.authorArai, Y.-
dc.contributor.authorArimura, R.-
dc.contributor.authorBarcikowski, E.-
dc.contributor.authorBelz, J.W.-
dc.contributor.authorBergman, D.R.-
dc.contributor.authorBlake, S.A.-
dc.contributor.authorBuckland, I.-
dc.contributor.authorCady, R.-
dc.contributor.authorCheon, B.G.-
dc.contributor.authorChiba, J.-
dc.contributor.authorChikawa, M.-
dc.contributor.authorFujisue, K.-
dc.contributor.authorFujita, K.-
dc.contributor.authorFujiwara, R.-
dc.contributor.authorFukushima, M.-
dc.contributor.authorFukushima, R.-
dc.contributor.authorFurlich, G.-
dc.contributor.authorGonzalez, R.-
dc.contributor.authorHanlon, W.-
dc.contributor.authorHayashi, M.-
dc.contributor.authorHayashida, N.-
dc.contributor.authorHibino, K.-
dc.contributor.authorHiguchi, R.-
dc.contributor.authorHonda, K.-
dc.contributor.authorIkeda, D.-
dc.contributor.authorInadomi, T.-
dc.contributor.authorInoue, N.-
dc.contributor.authorIshii, T.-
dc.contributor.authorIto, H.-
dc.contributor.authorIwakura, H.-
dc.contributor.authorIwasaki, A.-
dc.contributor.authorJeong, H.M.-
dc.contributor.authorJeong, S.-
dc.contributor.authorKadota, K.-
dc.contributor.authorKakimoto, F.-
dc.contributor.authorKalashev, O.-
dc.contributor.authorKasahara, K.-
dc.contributor.authorKasami, S.-
dc.contributor.authorKawai, H.-
dc.contributor.authorKawakami, S.-
dc.contributor.authorKawana, S.-
dc.contributor.authorKharuk, I.-
dc.contributor.authorKido, E.-
dc.contributor.authorKim, H.B.-
dc.contributor.authorKim, M.H.-
dc.contributor.authorKim, S.W.-
dc.contributor.authorKimura, Y.-
dc.contributor.authorKishigami, S.-
dc.contributor.authorKubota, Y.-
dc.contributor.authorKurisu, S.-
dc.contributor.authorKuznetsov, M.-
dc.contributor.authorKwon, Y.J.-
dc.contributor.authorLee, K.H.-
dc.contributor.authorLubsandorzhiev, B.-
dc.contributor.authorLundquist, J.P.-
dc.contributor.authorMachida, K.-
dc.contributor.authorMatsumiya, H.-
dc.contributor.authorMatsuyama, T.-
dc.contributor.authorMatthews, J.N.-
dc.contributor.authorMayta, R.-
dc.contributor.authorMinamino, M.-
dc.contributor.authorMukai, K.-
dc.contributor.authorMyers, I.-
dc.contributor.authorNagataki, S.-
dc.contributor.authorNakai, K.-
dc.contributor.authorNakamura, R.-
dc.contributor.authorNakamura, T.-
dc.contributor.authorNakamura, T.-
dc.contributor.authorNakamura, Y.-
dc.contributor.authorNakazawa, A.-
dc.contributor.authorNishio, E.-
dc.contributor.authorOda, H.-
dc.contributor.authorOhnishi, M.-
dc.contributor.authorOhoka, H.-
dc.contributor.authorOku, Y.-
dc.contributor.authorOkuda, T.-
dc.contributor.authorOmura, Y.-
dc.contributor.authorOno, M.-
dc.contributor.authorOnogi, R.-
dc.contributor.authorOshima, A.-
dc.contributor.authorOzawa, S.-
dc.contributor.authorPark, I.H.-
dc.contributor.authorPotts, M.-
dc.contributor.authorPshirkov, M.S.-
dc.contributor.authorRemington, J.-
dc.contributor.authorRodriguez, D.C.-
dc.contributor.authorRubtsov, G.I.-
dc.contributor.authorRyu, D.-
dc.contributor.authorSahara, R.-
dc.contributor.authorSaito, Y.-
dc.contributor.authorSakaki, N.-
dc.contributor.authorSako, T.-
dc.contributor.authorSakurai, N.-
dc.contributor.authorSano, K.-
dc.contributor.authorSato, K.-
dc.contributor.authorSeki, T.-
dc.contributor.authorSekino, K.-
dc.contributor.authorShah, P.D.-
dc.contributor.authorShibasaki, Y.-
dc.contributor.authorShibata, F.-
dc.contributor.authorShibata, N.-
dc.contributor.authorShibata, T.-
dc.contributor.authorShimodaira, H.-
dc.contributor.authorShin, B.K.-
dc.contributor.authorShin, H.S.-
dc.contributor.authorShinto, D.-
dc.contributor.authorSmith, J.D.-
dc.contributor.authorSokolsky, P.-
dc.contributor.authorSone, N.-
dc.contributor.authorStokes, B.T.-
dc.contributor.authorStroman, T.A.-
dc.contributor.authorTakagi, Y.-
dc.contributor.authorTakahashi, Y.-
dc.contributor.authorTakamura, M.-
dc.contributor.authorTakeda, M.-
dc.contributor.authorTakeishi, R.-
dc.contributor.authorTaketa, A.-
dc.contributor.authorTakita, M.-
dc.contributor.authorTameda, Y.-
dc.contributor.authorTanaka, H.-
dc.contributor.authorTanaka, K.-
dc.contributor.authorTanaka, M.-
dc.contributor.authorTanoue, Y.-
dc.contributor.authorThomas, S.B.-
dc.contributor.authorTinyakov, P.-
dc.contributor.authorTkachev, I.-
dc.contributor.authorTokuno, H.-
dc.contributor.authorTomida, T.-
dc.contributor.authorTroitsky, S.-
dc.contributor.authorTsuda, R.-
dc.contributor.authorTsunesada, Y.-
dc.contributor.authorUchihori, Y.-
dc.contributor.authorUdo, S.-
dc.contributor.authorUehama, T.-
dc.contributor.authorUrban, F.-
dc.contributor.authorWong, T.-
dc.contributor.authorYada, K.-
dc.contributor.authorYamamoto, M.-
dc.contributor.authorYamazaki, K.-
dc.contributor.authorYang, J.-
dc.contributor.authorYashiro, K.-
dc.contributor.authorYoshida, F.-
dc.contributor.authorYoshioka, Y.-
dc.contributor.authorZhezher, Y.-
dc.contributor.authorZundel, Z.-
dc.contributor.authorTelescope Array Collaboration-
dc.date.accessioned2023-01-25T09:24:23Z-
dc.date.available2023-01-25T09:24:23Z-
dc.date.issued2022-03-
dc.identifier.issn1824-8039-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182201-
dc.description.abstractIn this talk, we summarise the results of recent anisotropy studies conducted by the Telescope Array (TA) collaboration. At largest scales we test the TA data for the presence of a dipole. On smaller scales, an update on the excess of events in the direction of Ursa Major previously found in the TA data will be presented. These flux variations may trace the distribution of UHECR sources. We will examine the data for correlations with large-scale structures in the nearby Universe, and as a result, hints for the chemical composition of primaries will be provided. We also discuss a related anisotropy of the UHECR spectrum.-
dc.format.extent9-
dc.language영어-
dc.language.isoENG-
dc.titleTelescope Array anisotropy summary-
dc.typeArticle-
dc.identifier.scopusid2-s2.0-85144473382-
dc.identifier.bibliographicCitationProceedings of Science, v.395, pp 1 - 9-
dc.citation.titleProceedings of Science-
dc.citation.volume395-
dc.citation.startPage1-
dc.citation.endPage9-
dc.type.docTypeConference Paper-
dc.description.isOpenAccessY-
dc.description.journalRegisteredClassscopus-
dc.subject.keywordPlusTelescopes-
dc.subject.keywordPlusAnisotropy-
dc.subject.keywordPlusChemical compositions-
dc.subject.keywordPlusFlux variation-
dc.subject.keywordPlusLarge-scale structure-
dc.subject.keywordPlusLarge-scales-
dc.subject.keywordPlusSmall scale-
dc.subject.keywordPlusSpectra's-
dc.subject.keywordPlusTelescope arrays-
dc.identifier.urlhttps://pos.sissa.it/395/392/-
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