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The gamma-ray blazar PKS 0208-512 has shown strong periods of flaring, at allfrequencies from radio to gamma-ray. This has led to its inclusion in theTANAMI project, which tracks the jets of southern AGN using VLBI as well assupporting flux density monitoring programs. Time series analysis of the lightcurves generated by such monitoring is presented and discussed and VLBI maps ofthe source are used to show the evolution in the jet. A frequency dependent lagis observed between flaring at different radio frequencies which does notappear to correspond to purely optical depth effects. Major flaring atgamma-ray frequencies appears to be preceded by a new component in the jet seenin our VLBI data.

The Gamma-Ray Blazar PKS 0208-512, a Multi-Wavelength Investigation