Sensitivity and energy resolution estimates of the TACTIC gamma-ray telescope - Inputs from simulation studies (II)

dc.contributor.author	Koul, M. K
dc.contributor.author	Rannot, R. C
dc.contributor.author	Sapru, M. L
dc.contributor.author	Sathyabama, N
dc.contributor.author	Bhat, C. L
dc.contributor.author	Tickoo, A. K
dc.contributor.author	Razdan, A. K
dc.contributor.author	Gandhi, V. N
dc.date.accessioned	2007-11-13T10:06:45Z
dc.date.available	2007-11-13T10:06:45Z
dc.date.issued	1999
dc.identifier.citation	BASI, Vol. 27, No. 2, pp. 315 - 318	en
dc.identifier.uri	http://hdl.handle.net/2248/1955
dc.description.abstract	The 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.extent	325200 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/1999BASI...27..315K	en
dc.subject	Sensitivity	en
dc.subject	TACTIC simulations	en
dc.subject	Gamma-ray	en
dc.subject	Telescope	en
dc.title	Sensitivity and energy resolution estimates of the TACTIC gamma-ray telescope - Inputs from simulation studies (II)	en
dc.type	Article	en