Mueller et al. (2014) observed the active galactic nucleus of Centaurus A (CenA) approximately every six months at 8.4 GHz with the Australian Long Baseline Array (LBA) and associated telescopes in Antarctica, Chile, New Zealand, and South Africa, complemented by quasi-simultaneous 22.3 GHz observations. The first seven epochs of high-resolution TANAMI VLBI observations are presented, resolving the jet on (sub-)milliarcsecond scales.

ATNF Science Highlights from refereed publications during 2014.