  We combine kinematic and gravitational lensing data to construct the Radial
Acceleration Relation (RAR) of galaxies over a large dynamic range. We improve
on previous weak-lensing studies in two ways. First, we compute stellar masses
using the same stellar population model as for the kinematic data. Second, we
introduce a new method for converting excess surface density profiles to radial
accelerations. This method is based on a new deprojection formula which is
exact, computationally efficient, and gives smaller systematic uncertainties
than previous methods. We find that the RAR inferred from weak-lensing data
smoothly continues that inferred from kinematic data by about
$2.5\,\mathrm{dex}$ in acceleration. Contrary to previous studies, we find that
early- and late-type galaxies lie on the same joint RAR when a sufficiently
strict isolation criterion is adopted and their stellar and gas masses are
estimated consistently with the kinematic RAR.
