The BL Lac object H1426+428 (z≡0.129) is an established source of TeV
γ-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 γ-ray
production mechanisms in the AGN jets. We have observed this source for about
244h in 2004, 2006 and 2007 with the TACTIC γ-ray telescope located at
Mt. Abu, India. Detailed analysis of these data do not indicate the presence of
any statistically significant TeV γ-ray signal from the source
direction. Accordingly, we have placed an upper limit of
≤1.18×10−12photonscm−2s−1 on the integrated
γ-ray flux at 3σ significance level.Comment: 11 pages, 5 figures accepted for publication in Journal of Physics G:
Nuclear and Particle Physic