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We present a summary of the observation strategy of TANAMI (Tracking ActiveGalactic Nuclei with Austral Milliarcsecond Interferometry), a monitoringprogram to study the parsec-scale structure and dynamics of relativistic jetsin active galactic nuclei (AGN) of the Southern Hemisphere with the AustralianLong Baseline Array (LBA) and the trans-oceanic antennas Hartebeesthoek, TIGO,and O'Higgins. TANAMI is focusing on extragalactic sources south of -30 degreesdeclination with observations at 8.4 GHz and 22 GHz every ~2 months atmilliarcsecond resolution. The initial TANAMI sample of 43 sources has beendefined before the launch of the Fermi Gamma Ray Space Telescope to include themost promising candidates for bright gamma-ray emission to be detected with itsLarge Area Telescope (LAT). Since November 2008, we have been adding newsources to the sample, which now includes all known radio- and gamma-ray brightAGN of the Southern Hemisphere. The combination of VLBI and gamma-rayobservations is crucial to understand the broadband emission characteristics ofAGN and the nature of relativistic jets.

TANAMI - Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry