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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/1955
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dc.contributor.authorKoul, M. K-
dc.contributor.authorRannot, R. C-
dc.contributor.authorSapru, M. L-
dc.contributor.authorSathyabama, N-
dc.contributor.authorBhat, C. L-
dc.contributor.authorTickoo, A. K-
dc.contributor.authorRazdan, A. K-
dc.contributor.authorGandhi, V. N-
dc.date.accessioned2007-11-13T10:06:45Z-
dc.date.available2007-11-13T10:06:45Z-
dc.date.issued1999-
dc.identifier.citationBASI, Vol. 27, No. 2, pp. 315 - 318en
dc.identifier.urihttp://hdl.handle.net/2248/1955-
dc.description.abstractThe response of the recently-commissioned TACTIC imaging Cerenkov telescope to atmospheric Cerenkov pulses produced by cosmid gamma-ray and hadron-initiated extensive air-showers has been studied through Monte Carlo simulations, using the CORSIKA code (Capdeville et al., 1992). Preliminary results are presented on the likely performance of 3 different imaging camera sizes : 2.8 degree x 2.8 degree, 4.7 degree x 4.7 degree and 5.9 degree x 5.9 degree, with regard to event calorimetry and characterization.en
dc.format.extent325200 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/1999BASI...27..315Ken
dc.subjectSensitivityen
dc.subjectTACTIC simulationsen
dc.subjectGamma-rayen
dc.subjectTelescopeen
dc.titleSensitivity and energy resolution estimates of the TACTIC gamma-ray telescope - Inputs from simulation studies (II)en
dc.typeArticleen
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