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Paper detail

The TANAMI Program

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.

preprint2009arXivOpen access
Cornelia MuellerMatthias KadlerRoopesh OjhaM. BoeckR. BoothM. S. DutkaP. EdwardskA. L. FeyL. FuhrmannH. HaseS. HoriuchiD. L. JaunceyK. J. JohnstonU. KatzM. ListerJ. E. J. LovellC. PloetzJ. F. H. QuickE. RosG. B. TaylorD. J. ThompsonS. J. TingayG. TostiA. K. TzioumiskJ. WilmsJ. A. Zensus
astro-ph.GAastro-ph.HE
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Open access26 authors2 topics
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Cornelia MuellerMatthias KadlerRoopesh OjhaM. BoeckR. BoothM. S. DutkaP. EdwardskA. L. FeyL. FuhrmannH. HaseS. HoriuchiD. L. JaunceyK. J. JohnstonU. KatzM. ListerJ. E. J. LovellC. PloetzJ. F. H. QuickE. RosG. B. TaylorD. J. ThompsonS. J. TingayG. TostiA. K. TzioumiskJ. WilmsJ. A. Zensus

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