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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2457
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dc.contributor.authorKoul, D. K-
dc.contributor.authorKoul, M. K-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-19T07:15:31Z-
dc.date.available2008-06-19T07:15:31Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 373 - 376en
dc.identifier.urihttp://hdl.handle.net/2248/2457-
dc.description.abstractThe MACE (for Major Atmospheric Cerenkov Experiment), an imaging cerenkov telescope for gamma-ray astronomy investigations in the sub-TeV energy bracket, plans to use a 17 m-diameter high quality reflecter mounted with a high definition imaging camera in its focal plane. The spot size of the MACE has been estimated for, both, on-and off-axis cases, considering an ideal mirror surface. The effect on this spot-size due to surface smoothness errors has been investigated.en
dc.format.extent318892 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..373Ken
dc.subjectAtmospheric Cerenkov Radiationen
dc.subjectGamma Raysen
dc.subjectGraded Focal Lengthen
dc.subjectSpot Sizeen
dc.titleSpot size of 17m-diameter MACE reflector in presence of surface inaccuraciesen
dc.typeArticleen
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