  The compatibility between the de Sitter Swampland conjecture and
Ho\v{r}ava--Lifshitz $F(\bar{R})$ theories with a flat FLRW metric is studied.
We first study the standard $f(R)$ theories and show that the only way in which
the dS conjecture can be made independent of $R$ is by considering a power law
of the form $f(R)\sim R^{\gamma}$. The conjecture and the consistency of the
theory puts restrictions on $\gamma$ to be greater but close to one. For
$F(\bar{R})$ theories described by its two parameters $\lambda$ and $\mu$, we
use the equations of motion to construct the function starting with an ansatz
for the scale factor in the Jordan frame of the power law form. By performing a
conformal transformation on the three metric to the Einstein frame, we can
obtain an action of gravity plus a scalar field by relating the parameters of
the theory. The non-projectable and projectable cases are studied and the
differences are outlined. The obtained $F(\bar{R})$ function consists of terms
of the form $\bar{R}^{\gamma}$ with the possibility of having negative power
terms. The dS conjecture leads to inequalities for the $\lambda$ parameter; in
both versions, it becomes restricted to be greater but close to $1/3$. We can
also study the general case in which $\mu$ and $\lambda$ are considered as
independent. The obtained $F$ function has the same form as before. The
consistency of the theory and the dS conjecture lead to a set of inequalities
on both parameters that are studied numerically. In all cases, $\lambda$ is
restricted by $\mu$ around $1/3$, and we obtain $\lambda\to1/3$ if $\mu\to0$.
We consider the $f(R)$ limit $\mu,\lambda \to 1$ and we obtain consistent
results. Finally, we study the case of a constant Hubble parameter. The dS
conjecture can be fulfilled by restricting the parameters of the theory;
however, the constraint makes this compatibility exclusive to these kinds of
theories.
