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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2460
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dc.contributor.authorTickoo, A. K-
dc.contributor.authorDhar, V. K-
dc.contributor.authorVenugopal, K-
dc.contributor.authorYadav, K. K-
dc.contributor.authorKaul, S. K-
dc.contributor.authorKoul, R-
dc.contributor.authorKothari, M. K-
dc.contributor.authorGoyal, H. C-
dc.contributor.authorChandra, P-
dc.contributor.authorBhatt, N-
dc.contributor.authorBhat, C. L-
dc.date.accessioned2008-06-19T11:41:50Z-
dc.date.available2008-06-19T11:41:50Z-
dc.date.issued2002-
dc.identifier.citationBASI, Vol. 30, No. 1, pp. 381 - 384en
dc.identifier.urihttp://hdl.handle.net/2248/2460-
dc.description.abstractThe imaging element of the 4-element TACTIC telescope array has been in operation at Mt. Abu since 1997, for carrying out detailed investigations of gamma-ray sources in the TeV energy range. In order to characterize the progenitor particle (gamma-ray / cosmic ray), a relative gain calibration system, based on a high intensity LED, has been in operation. However, for calorimetric purposes, an absolute gain calibration system is necessary and has been developed for on-line calibration of 4 out of 349- pixels of its imaging camera, using Am241 -based light pulsers. The details of the scheme followed and the results obtained so far are presented in this paper.en
dc.format.extent403303 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2002BASI...30..381Ten
dc.subjectPMT Detectorsen
dc.subjectAbsolute Gain Calibrationen
dc.subjectTACTIC Telescopeen
dc.titleTowards absolute gain calibration of the TACTIC imaging elementen
dc.typeArticleen
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