Tanami: Parsec Scale AGN Physics in the Multiwavelength Era

Details Tanami: Parsec Scale AGN Physics in the Multiwavelength Era Tanami: Parsec Scale AGN Physics in the Multiwavelength Era

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543424o&link_type=abstract

American Astronomical Society, AAS Meeting #215, #434.24; Bulletin of the American Astronomical Society, Vol. 42, p.378

Astronomy and Astrophysics

Astronomy

Scientific paper

With its broader energy coverage, higher resolution, wider field of view and greater sensitivity, the Large Area Telescope (LAT) of the Fermi Gamma-ray Space Telescope is dramatically increasing our knowledge of AGN gamma-ray emission. However, discriminating between competing theoretical models requires quasi-simultaneous observations across the electromagnetic spectrum. The TANAMI (Tracking AGN with Austral Milliarcsecond Interferometry) and associated programs provide comprehensive radio monitoring for Fermi Gamma-ray Space Telescope sources south of declination -30 degrees. Near simultaneous data from the Swift satellite and ground based optical facilities span the gap from radio to gamma-ray energies. We describe the TANAMI program in the context of this panchromatic suite of observations and present early results.

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