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In a recent publication, we reported results of a multi-frequency VLBIcampaign of observations of the Active Galactic Nucleus (AGN) in galaxy M\,81,phase-referenced to the supernova SN\,1993J. We were able to extract preciseinformation on the relative astrometry of the AGN radio emission at differentepochs and frequencies. We found strong evidence of precession in the AGN jet(i.e., a systematic evolution in the jet inclination at each frequency) coupledto changes in the overall flux density at the different frequencies. In theseproceedings, we summarise the main contents of our previous publication and wereport on (preliminary) new results from our follow-up VLBI observations, nowphase-referenced to the young supernova SN2008iz. We also briefly discuss howthese results match the picture of our previously-reported precession model.

Jet precession in the active nucleus of M81. Ongoing VLBI monitoring