  Jets powered by AGN in the early Universe ($z \gtrsim 6$) have the potential
to not only define the trajectories of the first-forming massive galaxies but
to enable the accelerated growth of their associated SMBHs. Under typical
assumptions, jets could even rectify observed quasars with light seed formation
scenarios; however, not only are constraints on the parameters of the first
jets lacking, observations of these objects are scarce. Owing to the
significant energy density of the CMB at these epochs capable of quenching
radio emission, observations will require powerful, high angular resolution
X-ray imaging to map and characterize these jets. As such, \textit{AXIS} will
be necessary to understand early SMBH growth and feedback.
