TANAMI (Tracking Active Galactic Nuclei with Austral Milliarcsecond Interferometry) is a monitoring program to study the parsec-scale structures and dynamics of relativistic jets in active galactic nuclei (AGN) of the Southern Hemisphere with the Long Baseline Array and associated telescopes. Extragalactic jets south of -30 degrees declination are observed at 8.4 GHz and 22 GHz every two months at milliarcsecond resolution. The initial TANAMI sample is a hybrid radio and gamma-ray selected sample since the combination of VLBI and gamma-ray observations is crucial to understand the broadband emission characteristics of AGN.
@article{arxiv.0912.0686,
title = {The TANAMI Program},
author = {Cornelia Mueller and Matthias Kadler and Roopesh Ojha and M. Boeck and R. Booth and M. S. Dutka and P. Edwardsk and A. L. Fey and L. Fuhrmann and H. Hase and S. Horiuchi and D. L. Jauncey and K. J. Johnston and U. Katz and M. Lister and J. E. J. Lovell and C. Ploetz and J. F. H. Quick and E. Ros and G. B. Taylor and D. J. Thompson and S. J. Tingay and G. Tosti and A. K. Tzioumisk and J. Wilms and J. A. Zensus},
journal= {arXiv preprint arXiv:0912.0686},
year = {2015}
}