Search for 10 TeV gamma-ray emission from active galactic nuclei with the Tibet air shower array

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Active Galactic Nuclei, Continuous Radiation, Cosmic Rays, Flux Density, Gamma Rays, Markarian Galaxies, Northern Sky, Quasars, Computerized Simulation, Fourier Transformation, Monte Carlo Method, Scintillation Counters, Tibet

Scientific paper

A search for 10 Tera eV gamma-ray emission from 15 active galactic nuclei (AGNs) which were detected by energetic gamma-ray experiment telescope (EGRET) was made with the Tibet air shower array installed at an elevation of 4300 m above sea level. The data set, taken in the period from 18 Jun. 1990 - 29 Sep. 1992 has been used to search for continuous emission as well as emission on the timescale of 1 day. No evidence for emission from any of the AGNs on any of the time scales examined was found. The 95% confidence level upper limit to the continuous flux is presented on each source, and in particular the result for Markarian 421 is compared with other experiments. Further observation of gamma-rays at energies around 10 TeV from nearby AGNs will provide reliable information on the strength of the intergalactic backgroud photon field.

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