We present a class of exact scalar-tensor black holes for a shift-symmetricpart of the Horndeski action. The action includes a higher order scalar tensorinteraction term. We find that for a static and spherically symmetricspace-time, the scalar field, if time dependent, can be non-trivial and regularthus circumventing in an interesting way no-hair arguments for gallileons.Furthermore, within this class we find a stealth Schwarzschild and a partiallyself-tuned de-Sitter Schwarzschild black hole, both exhibiting a non trivialand regular space and time dependent scalar. In the latter solution the bulkvacuum energy is screened from a necessarily smaller geometric effective deSitter vacuum via an integration constant associated to the time dependentscalar field.