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

Static post-Newtonian limits in non-projectable Ho\v{r}ava-Lifshitz gravity with an extra U(1) symmetry