  We construct a no-scale model of inflation with a single modulus whose real
and imaginary parts are fixed by simple power-law corrections to the no-scale
K{\" a}hler potential. Assuming an uplift of the minimum of the effective
potential, the model yields a suitable number of e-folds of expansion and
values of the tilt in the scalar cosmological density perturbations and of the
ratio of tensor and scalar perturbations that are compatible with measurements
of the cosmic microwave background radiation.
