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The radio loud galaxy NGC 1052 is being studied in an intensive multi-bandcampaign including X-ray brigthness monitoring and spectroscopic observations,single-dish radio brightness monitoring at centimetre wavelengths, and ahigh-frequency very-long-baseline interferometry monitoring program. Here wepresent a progress report on our studies from this program. The final goal ofour observations is to relate the findings from the high-resolution radioimages with the observed variations in the X-ray regime, to address theaccretion processes and their relationship with the radio jet activity.

High-resolution studies of the twin jet in NGC 1052