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The tidal disruption of a star by a black hole provides a unique opportunity tostudy accretion physics. Recently delayed radio flares have been discovered inseveral TDEs peaking years after their optical emission has faded. Variousexplanations have been proposed including off-axis jets entering our line ofsight delayed accretion disk formation or a state change in the accretionflow. To elucidate the origin(s) of these flares it has become crucial toacquire radio and X-ray observations of these events at late-times (virgul months toyears post-discovery) to study this previously unexplored phase in the lifetimeof TDEs. [truncated! Please see actual data for full text]