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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2462
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dc.contributor.authorMajumdar, P-
dc.contributor.authorAcharya, B. S-
dc.contributor.authorBhat, P. N-
dc.contributor.authorChitnis, V. R-
dc.contributor.authorRahman, M. A-
dc.contributor.authorSingh, B. B-
dc.contributor.authorVishwanath, P. R-
dc.date.accessioned2008-06-19T12:17:42Z-
dc.date.available2008-06-19T12:17:42Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 389 -395en
dc.identifier.urihttp://hdl.handle.net/2248/2462-
dc.description.abstractPachmarhi Array of Cverenkov Telescopes (PACT), consisting of a distributed array of 25 telescopes is used to sample the atmospheric Cverenkov Photon showers. The shower front is fitted to a plane and the direction of arrival of primary particle is obtained. The accuracy in the estimation of the arrival direction of showers has been estimated to be ~ 0o.1 using 'split' array method. The angular resolution is expected to be even better when a spherical front is used for direction reconstruction or correction for the curvature of the front is applied. This is the best angular resolution among all the currently operating atmospheric Cverenkov telescopes in the world.en
dc.format.extent633652 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..389Men
dc.subjectPachmarhi Array of Cverenkov Telescopes (PACT)en
dc.subjectCverenkov Photon Showersen
dc.titleAngular resolution of Pachmarhi array of Cverenkov telescopesen
dc.typeArticleen
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