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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1953
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dc.contributor.authorDhar, V. K-
dc.contributor.authorYadav, K. K-
dc.contributor.authorBhattacharyya, S-
dc.contributor.authorKaul, R. K-
dc.contributor.authorBhat, C. L-
dc.contributor.authorKoul, R-
dc.contributor.authorKaul, S. R-
dc.contributor.authorKaul, S. K-
dc.date.accessioned2007-11-13T07:46:46Z-
dc.date.available2007-11-13T07:46:46Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 2, pp. 305 - 308en
dc.identifier.urihttp://hdl.handle.net/2248/1953-
dc.description.abstractAn ultra-sensitive, multi-detector gamma-ray telescope array is being setup at Mt. Abu for cosmic gamma-ray studies in the tens of TeV energy region. Here, we present the essential design features of the Cerenkov radiation detector, proposed to be used in the system, and describe the results of some preliminary simulation studies and prototype testing.en
dc.format.extent370857 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..305Den
dc.subjectGamma rayen
dc.subjectCerenkov detectorsen
dc.subjectTelescopeen
dc.titleDevelopment of a large-area, wide-angle Cerenkov radiation detector for the MYSTIQUE gamma-ray telescopeen
dc.typeArticleen
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