TANAMI (Tracking Active Galactic Nuclei With Austral Milliarcsecond Interferometry)

Details TANAMI (Tracking Active Galactic Nuclei With Austral Milliarcsecond Interferometry) TANAMI (Tracking Active Galactic Nuclei With Austral Milliarcsecond Interferometry)

Jan 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aas...21543423d&link_type=abstract

American Astronomical Society, AAS Meeting #215, #434.23; Bulletin of the American Astronomical Society, Vol. 42, p.378

Astronomy and Astrophysics

Astronomy

Scientific paper

TANAMI (Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry) is a program to image and monitor the parsec-scale structures of relativistic jets in active galactic nuclei of the Southern Hemisphere with the Australian Long Baseline Array. Complementary to ongoing programs in the Northern Hemisphere, TANAMI is tracking the jets of sources south of -30 degrees declination with milliarcsecond resolution at 8.4GHz and 22GHz. TANAMI observations are conducted at regular intervals so the motion of superluminal jets can be observed. Follow up observations of particularly interesting sources, in particular blazars that are found to be flaring at gamma-ray frequencies by Fermi, will also be conducted.

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