  In this paper, we give a systematic procedure for building locally stable dS
vacua in $\mathcal{N}=1$ supergravity models motivated by string theory. We
assume that one of the superfields has a Kahler potential of no-scale type and
impose a hierarchy of supersymmetry breaking conditions. In the no-scale
modulus direction the supersymmetry breaking is not small, in all other
directions it is of order $\epsilon$. We establish the existence of an
abundance of vacua for large regions in the parameter space spanned by
$\epsilon$ and the cosmological constant. These regions exist regardless of the
details of the other moduli, provided the superpotential can be tuned such that
the off-diagonal blocks of the mass matrix are parametrically small. We test
and support this general dS landscape construction by explicit analytic
solutions for the STU model. The Minkowski limits of these dS vacua either
break supersymmetry or have flat directions in agreement with a no-go theorem
that we prove, stating that a supersymmetric Minkowski vacuum without flat
directions cannot be continuously deformed into a non-supersymmetric vacuum. We
also describe a method for finding a broad class of stable supersymmetric
Minkowski vacua that can be F-term uplifted to dS vacua and which have an
easily controllable SUSY breaking scale.
