High Energy Observations of Blazars: the Future

Details High Energy Observations of Blazars: the Future High Energy Observations of Blazars: the Future

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006aspc..350..215m&link_type=abstract

Blazar Variability Workshop II: Entering the GLAST Era ASP Conference Series, Vol. 350, Proceedings of the Conference Held 10-12

Astronomy and Astrophysics

Astronomy

Scientific paper

This paper briefly summarizes the observations of active galaxies in the high energy band, juxtaposing the isotropic emission against that attributable to the blazar phenomenon, which is presumably associated with the relativistic jet. It briefly describes the main features of the currently popular leptonic models for radiation processes believed to be dominant in the AGN jets, and closes with the description of the GLAST γ-ray, as well as the Suzaku and NuSTAR X-ray sensitive, satellite - based instruments, all three bound to significantly improve our understanding of structure of blazars.

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