A Transient Sub-Eddington Black Hole X-Ray Binary Candidate in the Dust Lanes of Centaurus A (Burke et al. 2012 ApJ 749, 112)

Long-Term Monitoring of the Dynamics and Particle Acceleration of Knots in the Jet of Centaurus A (Goodger et al. 2010 ApJ 708, 675)

High-energy particle acceleration at the radio-lobe shock of Centaurus A Croston et al. 2009 MNRAS 395, 1999)

Evidence for Nonhydrostatic Gas Motions in the Hot Interstellar Medium of Centaurus A (Kraft et al. ApJ 677, L97)

New Results on Particle Acceleration in the Centaurus A Jet and Counterjet from a Deep Chandra Observation (Hardcastle et al. 2007 ApJ 670, L81)
Centaurus A is the closest active galaxy to us so studying it gives us unique insights into the dynamics and energy transport from the supermassive black hole at the core to the giant radio lobes that stretch to 10 degrees across the sky.

I am the principal investigator for the radio monitoring of the jet in Cen A and I am involved in the Chandra Cen A VLP. Specifically I have investigated the knots within the jet; how they form, evolve and transport energy to the lobes.