Abstract

We have observed the blazar Markarian 421 with the TACTIC γγ-ray telescope at Mt. Abu, India, from 22 November 2009 to 16 May 2010 for 265 hours. Detailed analysis of the data so recorded revealed presence of a TeV γγ-ray signal with a statistical significance of 12.12σσ at Eγ≥E_γ\geq 1 TeV. We have estimated the time averaged differential energy spectrum of the source in the energy range 1.0 - 16.44 TeV. The spectrum fits well with the power law function of the form (dF/dE=f0E−ΓdF/dE=f_0 E^{-Γ}) with f0=(1.39±0.239)×10−11cm−2s−1TeV−1f_0=(1.39\pm0.239)\times 10^{-11}cm^{-2}s^{-1}TeV^{-1} and Γ=2.31±0.14Γ=2.31\pm0.14.

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