  We work with a UV conformal U(1)' extension of the Standard Model, motivated
by the hierarchy problem and recent collider anomalies. This model admits
fermionic vector portal WIMP dark matter charged under the U(1)' gauge group.
The asymptotically safe boundary conditions can be used to fix the coupling
parameters, which allows the observed thermal relic abundance to constrain the
mass of the dark matter particle. This highly restricts the parameter space,
allowing strong predictions to be made. The parameter space of several UV
conformal U(1)' scenarios will be explored, and both bounds and possible
signals from direct and indirect detection observation methods will be
discussed.
