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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2458
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dc.contributor.authorKamath, K-
dc.contributor.authorBhattacharyya, S-
dc.contributor.authorDhar, V. K-
dc.contributor.authorDarzi, M. A-
dc.contributor.authorKaul, S. R-
dc.contributor.authorKaul, R. K-
dc.contributor.authorKoul, R-
dc.contributor.authorSahayanathan, S-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorWani, A. M-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-19T07:27:17Z-
dc.date.available2008-06-19T07:27:17Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 377 - 380en
dc.identifier.urihttp://hdl.handle.net/2248/2458-
dc.description.abstractAn ultra-sensitive, multidetector wide angle atmospheric Cerenkov telescope array is being set up at Mt. Abu for cosnic gamma-ray studies in tens of TeV energy region. The design features of the Cerenkov light detector, along with its efficiency, based on simulation and prototype testing studies, are presented in this paper.en
dc.format.extent354096 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..377Ken
dc.subjectGamma-Rayen
dc.subjectMYSTIQUE Telescopeen
dc.subjectLAWA detectoren
dc.titleLarge-Area Wide Angle (LAWA) cerenkov detector for MYSTIQUE arrayen
dc.typeArticleen
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