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dc.contributor.author김항배-
dc.date.accessioned2016-12-07T06:59:06Z-
dc.date.available2016-12-07T06:59:06Z-
dc.date.issued2015-05-
dc.identifier.citationASTROPHYSICAL JOURNAL, v. 804, no. 2, Page. 133-133en_US
dc.identifier.issn0004-637X-
dc.identifier.issn1538-4357-
dc.identifier.urihttp://iopscience.iop.org/article/10.1088/0004-637X/804/2/133/meta;jsessionid=4E3639B027FB636B54FF29C9E3EEDFE4.c1.iopscience.cld.iop.org-
dc.identifier.urihttp://hdl.handle.net/20.500.11754/24719-
dc.description.abstractWe report on the search for steady point-like sources of neutral particles around 10(18) eV between 2008 and 2013 May with the scintillator SD of the Telescope Array experiment. We found overall no significant point-like excess above 0.5 EeV in the northern sky. Subsequently, we also searched for coincidence with the Fermi bright Galactic sources. No significant coincidence was found within the statistical uncertainty. Hence, we set an upper limit on the neutron flux that corresponds to an averaged flux of 0.07 km(-2) yr(-1) for E ˃ 1 EeV in the northern sky at the 95% confidence level. This is the most stringent flux upper limit in a northern sky survey assuming point-like sources. The upper limit at the 95% confidence level on the neutron flux from Cygnus X-3 is also set to 0.2 km(-2) yr(-1) for E ˃ 0.5 EeV. This is an order of magnitude lower than previous flux measurements.en_US
dc.description.sponsorshipThe Telescope Array experiment is supported by the Japan Society for the Promotion of Science through Grants-in-Aids for Scientific Research on Specially Promoted Research (21000002) "Extreme Phenomena in the Universe Explored by Highest Energy Cosmic Rays" and for Scientific Research (19104006), and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the U.S. National Science Foundation awards PHY-0307098, PHY-0601915, PHY-0649681, PHY-0703893, PHY-0758342, PHY0848320, PHY-1069280, PHY-1069286, PHY-1404495 and PHY-1404502; by the National Research Foundation of Korea (2007-0093860, R32-10130, 2012R1A1A2008381, and 2013004883); by the Russian Academy of Sciences, RFBR grants 11-02-01528a and 13-02-01311a (INR), IISN project No. 4.4509.10, and Belgian Science Policy under IUAP VII/37 (ULB). The foundations of Dr. Ezekiel R. and Edna Wattis Dumke, Willard L. Eccles, and the George S. and Dolores Dore Eccles all helped with generous donations. The State of Utah supported the project through its Economic Development Board, and the University of Utah through the Office of the Vice President for Research. The experimental site became available through the cooperation of the Utah School and Institutional Trust Lands Administration (SITLA), U.S. Bureau of Land Management, and the U.S. Air Force. We also wish to thank the people and the officials of Millard County, Utah for their steadfast and warm support. We gratefully acknowledge the contributions from the technical staffs of our home institutions. An allocation of computer time from the Center for High Performance Computing at the University of Utah is gratefully acknowledged.en_US
dc.language.isoenen_US
dc.publisherIOP PUBLISHING LTDen_US
dc.subjectacceleration of particlesen_US
dc.subjectcosmic raysen_US
dc.subjectsurveysen_US
dc.titleA NORTHERN SKY SURVEY FOR POINT-LIKE SOURCES OF EeV NEUTRAL PARTICLES WITH THE TELESCOPE ARRAY EXPERIMENTen_US
dc.typeArticleen_US
dc.relation.volume804-
dc.identifier.doi10.1088/0004-637X/804/2/133-
dc.relation.page133-133-
dc.relation.journalASTROPHYSICAL JOURNAL-
dc.contributor.googleauthorAbbasi, R. U.-
dc.contributor.googleauthorAbe, M-
dc.contributor.googleauthorAbu-Zayyad, T.-
dc.contributor.googleauthorAllen, M.-
dc.contributor.googleauthorAnderson, R.-
dc.contributor.googleauthorAzuma, R.-
dc.contributor.googleauthorBarcikowski, E.-
dc.contributor.googleauthorBelz, J. W.-
dc.contributor.googleauthorBergman, D. R.-
dc.contributor.googleauthorBlake, S. A.-
dc.contributor.googleauthorKim, H. B.-
dc.relation.code2015000890-
dc.sector.campusS-
dc.sector.daehakCOLLEGE OF NATURAL SCIENCES[S]-
dc.sector.departmentDEPARTMENT OF PHYSICS-
dc.identifier.pidhbkim-


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