Abstract

The BL Lac object H1426+428 (z≡0.129z\equiv 0.129) is an established source of TeV γγ-rays and detections of these photons from this object also have important implications for estimating the Extragalactic Background Light (EBL) in addition to the understanding of the particle acceleration and γγ-ray production mechanisms in the AGN jets. We have observed this source for about 244h in 2004, 2006 and 2007 with the TACTIC γγ-ray telescope located at Mt. Abu, India. Detailed analysis of these data do not indicate the presence of any statistically significant TeV γγ-ray signal from the source direction. Accordingly, we have placed an upper limit of ≤1.18×10−12\leq1.18\times10^{-12} photonsphotons cm−2cm^{-2} s−1s^{-1} on the integrated γγ-ray flux at 3σσ significance level.

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