We evaluate the electronic self-energy Sigma(E) at an Al(111) surface
using the GW space-time method. This self-energy automatically include
s the image potential V-im not present in any local-density approximat
ion for exchange and correlation. We solve the energy-dependent quasip
article equations and calculate the effective local potential experien
ced by electrons in the near-surface region. The relative contribution
of exchange proves to be very different for states above the Fermi le
vel. The image-plane position for interacting electrons is closer to t
he surface than for the purely electrostatic effects felt by test char
ges, and, like its classical counterpart, is drawn inwards by the effe
cts of atomic structure.