  We consider various string-loop, warping and curvature corrections that are
expected to appear in type IIB moduli stabilisation scenarios. It has recently
been argued, in the context of strongly-warped LVS de Sitter vacua, that it is
impossible to achieve parametric suppression in all of these corrections
simultaneously \cite{Junghans:2022exo}. We investigate corrections in the
context of the recently discovered weakly-warped LVS de Sitter vacua, which
represent a distinct branch of solutions in type IIB flux compactifications,
supported by small conifold flux numbers $MK \lesssim 32$. Warping corrections
become less problematic in this regime, and some corrections even help to reach
the weakly-warped regime of parameter space. Other corrections continue to be
dangerous and would require numerical coefficients to be computed -- and found
to be small -- in order not to destroy the consistency of the weakly-warped LVS
de Sitter solution.
