The TeV spectrum of Mkn 501 as measured during the high state in 1997 by the HEGRA stereoscopic system of imaging air Cherenkov telescopes

Details The TeV spectrum of Mkn 501 as measured during the high state in 1997 by the HEGRA stereoscopic system of imaging air Cherenkov telescopes The TeV spectrum of Mkn 501 as measured during the high state in 1997 by the HEGRA stereoscopic system of imaging air Cherenkov telescopes

1999-01-08

arxiv.org/abs/astro-ph/9901093v1

Astropart.Phys. 11 (1999) 135-139

Astronomy and Astrophysics

Astrophysics

presented at the VERITAS Workshop on TeV Astrophysics of Extragalactic Sources, eds. M. Catanese, J. Quinn, and T. Weekes, to

Scientific paper

10.1016/S0927-6505(99)00037-7

The BL Lac object Mkn 501 has shown very high emission in TeV gamma-rays from March to October, 1997. During this period the source was continuously monitored with the HEGRA stereoscopic system of 4 imaging air Cherenkov telescopes for a total exposure time of 110 hours. The unprecedented statistics of about 38,000 TeV photons, combined with the good energy resolution of ~20 % over the entire energy range and with detailed simulations of the detector response, allowed a determination of the average energy spectrum from 500 GeV to 24 TeV. Although the gamma-ray flux varied strongly with time, the daily energy spectra remained rather constant in their shape. Therefore it is justified to derive a time averaged spectrum and thus to extend, for the first time, the spectral measurement well beyond 10 TeV. This TeV spectrum of Mkn 501 shows a gradual steepening which could be caused by a number of physical processes, such as a limited energy range of the radiating particles, intrinsic gamma-ray absorption inside the source, the Klein-Nishina effect (in the case of an inverse Compton origin of the radiation) and finally, an absorption of the TeV gamma-rays propagating in the intergalactic medium.

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