Observation of the Gamma-ray Emission of the Blazar Markarian 421 Above 250 GeV with the CAT Cherenkov Telescope

Details Observation of the Gamma-ray Emission of the Blazar Markarian 421 Above 250 GeV with the CAT Cherenkov Telescope Observation of the Gamma-ray Emission of the Blazar Markarian 421 Above 250 GeV with the CAT Cherenkov Telescope

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.428p&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

The gamma-ray emission of the blazar Markarian 421 above 250 GeV was observed by the CAT imaging Cherenkov telescope during two periods: December 1996 - May 1997 and December 1997 - May 1998; results on the source variability are presented on the basis of data selected by requiring good atmospheric conditions, representing 77 hours of ``on-source'' observations and 33 hours of ``off-source'' data. The energy spectrum of the source for the flaring periods is given above 350 GeV.

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