INDICATIONS OF INTERMEDIATE-SCALE ANISOTROPY OF COSMIC RAYS WITH ENERGY GREATER THAN 57 EeV IN THE NORTHERN SKY MEASURED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT
DC Field | Value | Language |
---|---|---|
dc.contributor.author | Abbasi, RU | - |
dc.contributor.author | Abe, M | - |
dc.contributor.author | Abu-Zayyad, T | - |
dc.contributor.author | Allen, M | - |
dc.contributor.author | Anderson, R | - |
dc.contributor.author | Azuma, R | - |
dc.contributor.author | Barcikowski, E | - |
dc.contributor.author | Belz, JW | - |
dc.contributor.author | Bergman, DR | - |
dc.contributor.author | Blake, SA | - |
dc.contributor.author | Cady, R | - |
dc.contributor.author | Chae, MJ | - |
dc.contributor.author | Cheon, BG | - |
dc.contributor.author | Chiba, J | - |
dc.contributor.author | Chikawa, M | - |
dc.contributor.author | Cho, WR | - |
dc.contributor.author | Fujii, T | - |
dc.contributor.author | Fukushima, M | - |
dc.contributor.author | Goto, T | - |
dc.contributor.author | Hanlon, W | - |
dc.contributor.author | Hayashi, Y | - |
dc.contributor.author | Hayashida, N | - |
dc.contributor.author | Hibino, K | - |
dc.contributor.author | Honda, K | - |
dc.contributor.author | Ikeda, D | - |
dc.contributor.author | Inoue, N | - |
dc.contributor.author | Ishii, T | - |
dc.contributor.author | Ishimori, R | - |
dc.contributor.author | Ito, H | - |
dc.contributor.author | Ivanov, D | - |
dc.contributor.author | Jui, CCH | - |
dc.contributor.author | Kadota, K | - |
dc.contributor.author | Kakimoto, F | - |
dc.contributor.author | Kalashev, O | - |
dc.contributor.author | Kasahara, K | - |
dc.contributor.author | Kawai, H | - |
dc.contributor.author | Kawakami, S | - |
dc.contributor.author | Kawana, S | - |
dc.contributor.author | Kawata, K | - |
dc.contributor.author | Kido, E | - |
dc.contributor.author | Kim, HB | - |
dc.contributor.author | Kim, JH | - |
dc.contributor.author | Kim, JH | - |
dc.contributor.author | Kitamura, S | - |
dc.contributor.author | Kitamura, Y | - |
dc.contributor.author | Kuzmin, V | - |
dc.contributor.author | Kwon, YJ | - |
dc.contributor.author | Lan, J | - |
dc.contributor.author | Lim, SI | - |
dc.contributor.author | Lundquist, JP | - |
dc.contributor.author | Machida, K | - |
dc.contributor.author | Martens, K | - |
dc.contributor.author | Matsuda, T | - |
dc.contributor.author | Matsuyama, T | - |
dc.contributor.author | Matthews, JN | - |
dc.contributor.author | Minamino, M | - |
dc.contributor.author | Mukai, K | - |
dc.contributor.author | Myers, I | - |
dc.contributor.author | Nagasawa, K | - |
dc.contributor.author | Nagataki, S | - |
dc.contributor.author | Nakamura, T | - |
dc.contributor.author | Nonaka, T | - |
dc.contributor.author | Nozato, A | - |
dc.contributor.author | Ogio, S | - |
dc.contributor.author | Ogura, J | - |
dc.contributor.author | Ohnishi, M | - |
dc.contributor.author | Ohoka, H | - |
dc.contributor.author | Oki, K | - |
dc.contributor.author | Okuda, T | - |
dc.contributor.author | Ono, M | - |
dc.contributor.author | Oshima, A | - |
dc.contributor.author | Ozawa, S | - |
dc.contributor.author | Park, IH | - |
dc.contributor.author | Pshirkov, MS | - |
dc.contributor.author | Rodriguez, DC | - |
dc.contributor.author | Rubtsov, G | - |
dc.contributor.author | Ryu, D | - |
dc.contributor.author | Sagawa, H | - |
dc.contributor.author | Sakurai, N | - |
dc.contributor.author | Sampson, AL | - |
dc.contributor.author | Scott, LM | - |
dc.contributor.author | Shah, PD | - |
dc.contributor.author | Shibata, F | - |
dc.contributor.author | Shibata, T | - |
dc.contributor.author | Shimodaira, H | - |
dc.contributor.author | Shin, BK | - |
dc.contributor.author | Smith, JD | - |
dc.contributor.author | Sokolsky, P | - |
dc.contributor.author | Springer, RW | - |
dc.contributor.author | Stokes, BT | - |
dc.contributor.author | Stratton, SR | - |
dc.contributor.author | Stroman, TA | - |
dc.contributor.author | Suzawa, T | - |
dc.contributor.author | Takamura, M | - |
dc.contributor.author | Takeda, M | - |
dc.contributor.author | Takeishi, R | - |
dc.contributor.author | Taketa, A | - |
dc.contributor.author | Takita, M | - |
dc.contributor.author | Tameda, Y | - |
dc.contributor.author | Tanaka, H | - |
dc.contributor.author | Tanaka, K | - |
dc.contributor.author | Tanaka, M | - |
dc.contributor.author | Thomas, SB | - |
dc.contributor.author | Thomson, GB | - |
dc.contributor.author | Tinyakov, P | - |
dc.contributor.author | Tkachev, I | - |
dc.contributor.author | Tokuno, H | - |
dc.contributor.author | Tomida, T | - |
dc.contributor.author | Troitsky, S | - |
dc.contributor.author | Tsunesada, Y | - |
dc.contributor.author | Tsutsumi, K | - |
dc.contributor.author | Uchihori, Y | - |
dc.contributor.author | Udo, S | - |
dc.contributor.author | Urban, F | - |
dc.contributor.author | Vasiloff, G | - |
dc.contributor.author | Wong, T | - |
dc.contributor.author | Yamane, R | - |
dc.contributor.author | Yamaoka, H | - |
dc.contributor.author | Yamazaki, K | - |
dc.contributor.author | Yang, J | - |
dc.contributor.author | Yashiro, K | - |
dc.contributor.author | Yoneda, Y | - |
dc.contributor.author | Yoshida, S | - |
dc.contributor.author | Yoshii, H | - |
dc.contributor.author | Zollinger, R | - |
dc.contributor.author | Zundel, Z | - |
dc.date.accessioned | 2022-07-07T05:26:10Z | - |
dc.date.available | 2022-07-07T05:26:10Z | - |
dc.date.created | 2021-05-12 | - |
dc.date.issued | 2014-08 | - |
dc.identifier.issn | 2041-8205 | - |
dc.identifier.uri | https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/143338 | - |
dc.description.abstract | We have searched for intermediate-scale anisotropy in the arrival directions of ultrahigh-energy cosmic rays with energies above 57 EeV in the northern sky using data collected over a 5 yr period by the surface detector of the Telescope Array experiment. We report on a cluster of events that we call the hotspot, found by oversampling using 20 degrees radius circles. The hotspot has a Li-Ma statistical significance of 5.1 sigma, and is centered at R. A. = 146 degrees 7, decl. = 43 degrees 2. The position of the hotspot is about 19 degrees off of the supergalactic plane. The probability of a cluster of events of 5.1 sigma significance, appearing by chance in an isotropic cosmic-ray sky, is estimated to be 3.7 x 10(-4) (3.4 sigma). | - |
dc.language | 영어 | - |
dc.language.iso | en | - |
dc.publisher | IOP PUBLISHING LTD | - |
dc.title | INDICATIONS OF INTERMEDIATE-SCALE ANISOTROPY OF COSMIC RAYS WITH ENERGY GREATER THAN 57 EeV IN THE NORTHERN SKY MEASURED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT | - |
dc.type | Article | - |
dc.contributor.affiliatedAuthor | Cheon, BG | - |
dc.contributor.affiliatedAuthor | Kim, HB | - |
dc.identifier.doi | 10.1088/2041-8205/790/2/L21 | - |
dc.identifier.scopusid | 2-s2.0-84904703537 | - |
dc.identifier.wosid | 000339897100007 | - |
dc.identifier.bibliographicCitation | ASTROPHYSICAL JOURNAL LETTERS, v.790, no.2, pp.1 - 5 | - |
dc.relation.isPartOf | ASTROPHYSICAL JOURNAL LETTERS | - |
dc.citation.title | ASTROPHYSICAL JOURNAL LETTERS | - |
dc.citation.volume | 790 | - |
dc.citation.number | 2 | - |
dc.citation.startPage | 1 | - |
dc.citation.endPage | 5 | - |
dc.type.rims | ART | - |
dc.type.docType | Article | - |
dc.description.journalClass | 1 | - |
dc.description.isOpenAccess | Y | - |
dc.description.journalRegisteredClass | scie | - |
dc.description.journalRegisteredClass | scopus | - |
dc.relation.journalResearchArea | Astronomy & Astrophysics | - |
dc.relation.journalWebOfScienceCategory | Astronomy & Astrophysics | - |
dc.subject.keywordPlus | GALACTIC MAGNETIC-FIELD | - |
dc.subject.keywordPlus | ARRIVAL DIRECTIONS | - |
dc.subject.keywordPlus | PROPAGATION | - |
dc.subject.keywordPlus | SPECTRUM | - |
dc.subject.keywordAuthor | acceleration of particles | - |
dc.subject.keywordAuthor | cosmic rays | - |
dc.subject.keywordAuthor | large-scale structure of universe | - |
dc.subject.keywordAuthor | surveys | - |
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