Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/12413
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dc.contributor.authorYoshikoshi, T.-
dc.contributor.authorDazeley, S.-
dc.contributor.authorGunji, S.-
dc.contributor.authorHara, S.-
dc.contributor.authorHara, T.-
dc.contributor.authorHolder, J.-
dc.contributor.authorJimbo, J.-
dc.contributor.authorKawachi, A.-
dc.contributor.authorKifune, T.-
dc.contributor.authorKubo, H.-
dc.contributor.authorKushida, J.-
dc.contributor.authorBohec, S.-
dc.contributor.authorMatsubara, Y.-
dc.contributor.authorMizumoto, Y.-
dc.contributor.authorMori, M.-
dc.contributor.authorMoriya, M.-
dc.contributor.authorMuraishi, H.-
dc.contributor.authorMuraki, Y.-
dc.contributor.authorNaito, T.-
dc.contributor.authorNishijima, K.-
dc.contributor.authoret al.-
dc.date.issued1999-
dc.identifier.citationAstroparticle Physics, 1999; 11(1-2):267-269-
dc.identifier.issn0927-6505-
dc.identifier.issn1873-2852-
dc.identifier.urihttp://hdl.handle.net/2440/12413-
dc.description.abstractThe Cherenkov telescope of the CANGAROO II project will start operation in 1999 in Woomera, South Australia, with a 7 m aperture using 60 plastic mirrors. The telescope, which can potentially be extended to a 10 m aperture, will be used to observe gamma-ray sources with an energy threshold of the order of 100 GeV in the southern sky.-
dc.description.urihttp://www.elsevier.com/wps/find/journaldescription.cws_home/523319/description#description-
dc.language.isoen-
dc.publisherELSEVIER SCIENCE BV-
dc.source.urihttp://dx.doi.org/10.1016/s0927-6505(99)00063-8-
dc.titlePresent status of the 7-10 m telescope of CANGAROO II-
dc.typeJournal article-
dc.identifier.doi10.1016/S0927-6505(99)00063-8-
pubs.publication-statusPublished-
dc.identifier.orcidRowell, G. [0000-0002-9516-1581]-
Appears in Collections:Aurora harvest 7
Physics publications

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