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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2384
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dc.contributor.authorSuthar, R. L-
dc.contributor.authorGuha, S-
dc.contributor.authorBandopadhyay, K-
dc.contributor.authorMishra, V. K-
dc.contributor.authorKoul, R-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-02T10:20:39Z-
dc.date.available2008-06-02T10:20:39Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 223 - 227en
dc.identifier.urihttp://hdl.handle.net/2248/2384-
dc.description.abstractA low-threshold energy, high-sensitivity gamma-ray telescope, MACE (for Major Atmospheric Cerenkov Experiment) is proposed to be built in India for explorations of gamma-ray sky in 100's keV - 10's GeV photon energy range, hitherto inaccessible from ground. This paper outlines the scientific motivation for this major telescope system and focuses on its mechanical design aspects.en
dc.format.extent450063 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..223Sen
dc.subjectGalaxiesen
dc.subjectGamma-Ray Telescopeen
dc.subjectLarge Light Collectoren
dc.subjectEGRET sourcesen
dc.titleSalient mechanical design features of the proposed 17 meter diameter MACE imaging gamma-ray telescopeen
dc.typeArticleen
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