CANGAROO-III Search for Gamma Rays from Kepler's Supernova Remnant

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dc.contributor.authorEnomoto, R
dc.contributor.authorHigashi, Y
dc.contributor.authorYoshida, T
dc.contributor.authorTanimori, T
dc.contributor.authorBicknell, Geoffrey
dc.contributor.authorClay, Roger W
dc.contributor.authorEdwards, P G
dc.contributor.authorGunji, S
dc.contributor.authorHara, S
dc.contributor.authorHattori, T
dc.contributor.authorHayashi, S
dc.contributor.authorHirai, Y
dc.date.accessioned2015-12-08T22:17:44Z
dc.date.issued2008
dc.date.updated2015-12-08T08:10:00Z
dc.description.abstractKepler's supernova, discovered in 1604 October, produced a remnant that has been well studied observationally in the radio, infrared, optical, and X-ray bands, and theoretically. Some models have predicted a TeV gamma-ray flux that is detectable with current Imaging Cerenkov Atmospheric Telescopes. We report on observations carried out in 2005 April with the CANGAROO-III Telescope. No statistically significant excess was observed, and limitations on the allowed parameter range in the model are discussed.
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/31032
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Gamma rays: observations; Supernovae: individual (Kepler's SNR)
dc.titleCANGAROO-III Search for Gamma Rays from Kepler's Supernova Remnant
dc.typeJournal article
local.bibliographicCitation.issueAug
local.bibliographicCitation.lastpage388
local.bibliographicCitation.startpage383
local.contributor.affiliationEnomoto, R, University of Tokyo
local.contributor.affiliationHigashi, Y, Kyoto University
local.contributor.affiliationYoshida, T, Ibaraki University
local.contributor.affiliationTanimori, T, Kyoto University
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationClay, Roger W, University of Adelaide
local.contributor.affiliationEdwards, P G, CSIRO, Australia Telescope National Facility
local.contributor.affiliationGunji, S, Yamagata University
local.contributor.affiliationHara, S, Ibaraki Prefectural University of Health Sciences
local.contributor.affiliationHattori, T, Tokai University
local.contributor.affiliationHayashi, S, Konan University
local.contributor.affiliationHirai, Y, Ibaraki Prefectural University of Health Sciences
local.contributor.authoremailu8000061@anu.edu.au
local.contributor.authoruidBicknell, Geoffrey, u8000061
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020106 - High Energy Astrophysics; Cosmic Rays
local.identifier.ariespublicationu4362859xPUB79
local.identifier.citationvolume683
local.identifier.doi10.1086/589912
local.identifier.scopusID2-s2.0-49449112107
local.identifier.thomsonID000258296100032
local.identifier.uidSubmittedByu4362859
local.type.statusPublished Version

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