A Search for TeV Gamma-Ray Emission from Selected AGN Using Milagro

Details A Search for TeV Gamma-Ray Emission from Selected AGN Using Milagro A Search for TeV Gamma-Ray Emission from Selected AGN Using Milagro

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2649b&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

The Milagro gamma-ray observatory, located near Los Alamos, NM, employs a water-Cherenkov technique to continuously monitor the northern sky for astrophysical gammaray emission near 1 TeV. Milagro's high duty-cycle (˜95%) and wide aperture (˜2 sr) allow for the detection of flaring behavior associated with TeV AGN, even during daytime transits. Results are presented from a search of the Milagro 2000-2001 data set for TeV emission from selected AGN, including the bright flare of Mrk421 in early 2001.

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