Abstract
We present two-year-long observations of the flux of very-high-energy (∼1012 eV) gamma rays from the active galactic nucleus Mk 501 performed with a Cherenkov detector at the Crimean Astrophysical Observatory. A gamma-ray flux from the object was shown to exist at confidence levels of 11 and 7 standard deviations for 1997 and 1998, respectively. The flux varied over a wide range. The mean flux at energies >1012 eV, as inferred from the 1997 and 1998 data, is (5.0±0.6)×10−11 and (3.7±0.6)×10−11 cm−2 s−1, respectively. The errors are the sum of statistical observational and modeling errors. The mean power released in the form of gamma rays is ∼2×1043 erg s−1 sr−1.
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Translated from Pis 'ma v Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 26, No. 4, 2000, pp. 243–248.
Original Russian Text Copyright © 2000 by Andreeva, Zyskin, Kalekin, Neshpor, Stepanyan, Fomin, Chalenko, Shitov.
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Andreeva, N.A., Zyskin, Y.L., Kalekin, O.R. et al. Observations of the gamma-ray flux from the galaxy Mk 501. Astron. Lett. 26, 199–203 (2000). https://doi.org/10.1134/1.20382
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DOI: https://doi.org/10.1134/1.20382