  We study a regularization by noise phenomenon for the continuous parabolic
Anderson model with a potential shifted along paths of fractional Brownian
motion. We demonstrate that provided the Hurst parameter is chosen sufficiently
small, this shift allows to establish well-posedness and stability to the
corresponding problem - without the need of renormalization - in any dimension.
We moreover provide a robustified Feynman-Kac type formula for the unique
solution to the regularized problem building upon regularity estimates for the
local time of fractional Brownian motion as well as non-linear Young
integration.
