  Constraining dark matter models necessitates accurate predictions for large
set of observables originating from collider physics, cosmology and
astrophysics. We consider two classes of top-philic dark matter models where
the dark sector is coupled to the Standard Model via the top quark and study
the complementarity of dark matter relic density, direct and indirect detection
and collider searches in exploring the model parameter space. We moreover
investigate how higher-order corrections affect the results.
