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The measurements of the cosmic ray energy spectrum and the depth of maximum shower development of Telescope Array Hybrid trigger events

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dc.contributor.authorShin, H.-
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.authorFujii, T.-
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.authorIvanov, D.-
dc.contributor.authorIwakura, H.-
dc.contributor.authorIwasaki, A.-
dc.contributor.authorJeong, H.M.-
dc.contributor.authorJeong, S.-
dc.contributor.authorJui, C.C.H.-
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.authorKawata, K.-
dc.contributor.authorKharuk, I.-
dc.contributor.authorKido, E.-
dc.contributor.authorKim, H.B.-
dc.contributor.authorKim, J.H.-
dc.contributor.authorKim, J.H.-
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.authorKuzmin, V.-
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.authorNonaka, T.-
dc.contributor.authorOda, H.-
dc.contributor.authorOgio, S.-
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.authorSagawa, H.-
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.authorThomson, G.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.authorthe Telescope Array Collaboration-
dc.date.accessioned2023-01-25T09:32:27Z-
dc.date.available2023-01-25T09:32:27Z-
dc.date.created2023-01-05-
dc.date.issued2022-03-
dc.identifier.issn1824-8039-
dc.identifier.urihttps://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/182204-
dc.description.abstractThe Telescope Array experiment is an ultra-high energy cosmic ray observatory located in Millard County, Utah, USA. The observatory consists of 3 fluorescence detector (FD) stations and 507 surface detectors (SD) that cover an area of 700 km2. Hybrid trigger is an external trigger system for the SD arrays that prompts the SD to perform data acquisition when an FD detects a shower-like event. In comparison with the SD autonomous trigger, hybrid trigger allows the SD to collect the data of an air shower that has primary energy below 1018.5 eV, where the efficiency of SD autonomous trigger decreases rapidly. We present the measurements of the cosmic ray energy spectrum and the depth of maximum shower development of hybrid trigger events observed from October 2010 to September 2014.-
dc.language영어-
dc.language.isoen-
dc.publisherSissa Medialab Srl-
dc.titleThe measurements of the cosmic ray energy spectrum and the depth of maximum shower development of Telescope Array Hybrid trigger events-
dc.typeArticle-
dc.contributor.affiliatedAuthorCheon, B.G.-
dc.identifier.scopusid2-s2.0-85144390405-
dc.identifier.bibliographicCitationProceedings of Science, v.395, pp.1 - 10-
dc.relation.isPartOfProceedings of Science-
dc.citation.titleProceedings of Science-
dc.citation.volume395-
dc.citation.startPage1-
dc.citation.endPage10-
dc.type.rimsART-
dc.type.docTypeConference Paper-
dc.description.journalClass1-
dc.description.isOpenAccessN-
dc.description.journalRegisteredClassscopus-
dc.subject.keywordPlusCosmic rays-
dc.subject.keywordPlusCosmology-
dc.subject.keywordPlusData acquisition-
dc.subject.keywordPlusFinite difference method-
dc.subject.keywordPlusFluorescence-
dc.subject.keywordPlusTelescopes-
dc.subject.keywordPlusObservatories-
dc.subject.keywordPlusAir showers-
dc.subject.keywordPlusCosmic ray energy spectrum-
dc.subject.keywordPlusDetector arrays-
dc.subject.keywordPlusDetector stations-
dc.subject.keywordPlusFluorescence detector-
dc.subject.keywordPlusMeasurements of-
dc.subject.keywordPlusSurface detectors-
dc.subject.keywordPlusTelescope arrays-
dc.subject.keywordPlusTrigger systems-
dc.subject.keywordPlusUltra high-energy cosmic rays-
dc.identifier.urlhttps://pos.sissa.it/395/305/-
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