Studies of Nearby Blazars with Milagro

Details Studies of Nearby Blazars with Milagro Studies of Nearby Blazars with Milagro

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..499w&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

10

Active And Peculiar Galaxies And Related Systems, Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

We have examined a sample of 47 blazars for evidence of TeV emission in the data collected with Milagro since 2000. Emission is clearly seen from Markarian 421, with the detected flux concentrated in two intervals coinciding with strong X-ray emission. No significant flux is detected from any of the other AGN, and flux limits are presented. For the blazars I Zw 187 and RGB 1725+118 the limits - including the effects of absorption by extragalactic background light (EBL) - exclude the empirical model of Fossati et al. for the flux.

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