Early Observations of Gamma-ray Blazars with Fermi LAT

Details Early Observations of Gamma-ray Blazars with Fermi LAT Early Observations of Gamma-ray Blazars with Fermi LAT

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21346808r&link_type=abstract

American Astronomical Society, AAS Meeting #213, #468.08; Bulletin of the American Astronomical Society, Vol. 41, p.417

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The Large Area Telescope (LAT), one of two instruments on the Fermi Gamma-ray Space Telescope (formerly GLAST, launched June 11, 2008) is a pair conversion detector designed to study the gamma-ray sky in the energy range 20 MeV to >300; GeV. Because of its improved sensitivity with respect to previous missions, Fermi LAT will revamp our understanding of gamma-ray blazars as: i)sources of high-energy radiation, and ii) as a cosmological population. In this poster we present science highlights from the first few months of blazar observations.

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