The program of quantizing the gravitational field with the help of affine f
ield variables is continued. For completeness, a review of the selection cr
iteria that singles out the affine fields, the alternative treatment of con
straints, and the choice of the initial (before imposition of the constrain
ts) ultralocal representation of the field operators is initially presented
. As analogous examples demonstrate, the introduction and enforcement of th
e gravitational constraints will cause sufficient changes in the operator r
epresentations so that all vestiges of the initial ultralocal field operato
r representation disappear. To achieve this introduction and enforcement of
the constraints, a well characterized phase space functional integral repr
esentation for the reproducing kernel of a suitably regularized physical Hi
lbert space is developed and extensively analyzed. (C) 2001 American Instit
ute of Physics.