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The formation of powerful extragalactic jets is not well understood at present as well as the associated key question:“What makes an AGN radio loud?”. Here we discuss how the combination of VLBI and X-ray spectroscopic observations allows the inter-relation between the accretion flow and the formation of relativistic jets in AGN to be explored.

Probes of Jet-Disk-Coupling in AGN from Combined VLBI and X-Ray Observations