  In this paper, we study static post-Newtonian limits in non-projectable
Ho\v{r}ava-Lifshitz gravity with an extra U(1) symmetry. After obtaining all
static spherical solutions in the infrared, we apply them to the solar system
tests, and obtain the Eddington-Robertson-Schiff parameters in terms of the
coupling constants of the theory. These parameters are well consistent with
observations for the physically viable coupling constants. In contrast to the
projectable case, this consistence is achieved without taking the gauge field
and Newtonian prepotential as part of the metric.
