We study the residual gauge freedom within the null quasi-spherical (N
QS) gauge for space-times admitting an expanding shear-free null folia
tion. By constructing the most general NQS coordinates subordinate to
such a foliation, we obtain both a clear picture of the geometric natu
re of the residual coordinate freedom, and an explicit construction of
nontrivial NQS metrics representing some well-known space-times, such
as Schwarzschild, accelerated Minkowski, and Robinson-Trautman. These
examples will be useful in testing numerical evolution codes. The geo
metric gauge freedom consists of an arbitrary boost and rotation at ea
ch coordinate sphere-and this freedom may be used to normalise the coo
rdinate to an ''inertial'' frame. (C) 1997 American Institute of Physi
cs.