TeV-Characteristics of the BL Lac Objects Mkn 501 and Mkn 421 as Measured with the HEGRA Stereoscopic System of Imaging Atmospheric Cherenkov Telescopes

Details TeV-Characteristics of the BL Lac Objects Mkn 501 and Mkn 421 as Measured with the HEGRA Stereoscopic System of Imaging Atmospheric Cherenkov Telescopes TeV-Characteristics of the BL Lac Objects Mkn 501 and Mkn 421 as Measured with the HEGRA Stereoscopic System of Imaging Atmospheric Cherenkov Telescopes

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999icrc....3..350a&link_type=abstract

Proceedings of the 26th International Cosmic Ray Conference. August 17-25, 1999. Salt Lake City, Utah, USA. Under the auspices o

Physics

Scientific paper

The HEGRA system of Imaging Atmospheric Cherenkov Telescopes (IACTs) has been used since the beginning of 1997 for a comprehensive study of the gamma-ray emission from the BL Lac objects Mkn 501 and Mkn 421 in the energy range above 500 GeV. Here we summarize the TeV characteristics of Mkn 501 during its spectacular outburst in 1997 and give an overview of the 1997 and 1998 Mkn 421 results.

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