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Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/49432
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dc.contributor.authorMori, M.en
dc.contributor.authorClay, R.en
dc.contributor.authorGunji, S.en
dc.contributor.authorHara, S.en
dc.contributor.authorHara, T.en
dc.contributor.authorItoh, C.en
dc.contributor.authorKubo, H.en
dc.contributor.authorMaeda, S.en
dc.contributor.authorYoshikoshi, T.en
dc.date.issued2001en
dc.identifier.citationProceedings of ICRC 2001, 2001 / M.Simon, E.Lorenz and M.Pohl (eds.), pp. 2831-2834en
dc.identifier.issn1340-3745en
dc.identifier.urihttp://hdl.handle.net/2440/49432-
dc.description.abstractWe report on the status of the construction of an array of four 10m atmospheric Cherenkov telescopes for gamma-ray astronomy, near Woomera, in South Australia-the CANGAROO-III project. The first telescope of this array is the upgraded version of the CANGAROO-II 7m telescope and has been in operation since March 2000. The second telescope, an improved version of the first, is being constructed for installation in late 2001. Stereoscopic observation of sub TeV gamma-rays with the two 10m telescopes will begin in 2002 and the full array will be operational in 2004.en
dc.description.urihttp://vesper.icrr.u-tokyo.ac.jp/publications.html#papersen
dc.language.isoenen
dc.publisherCopernicusen
dc.titleThe CANGAROO-III Project: Status reporten
dc.typeConference paperen
pubs.publication-statusPublisheden
dc.identifier.orcidClay, R. [0000-0002-9040-9648]en
Appears in Collections:Aurora harvest
Physics publications

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