  We explain how an approximation to the rings formed by the host galaxies in
lensed QSOs can be inferred from the QSO data alone. A simple ring image can be
made from any lens model by a simple piece of computer graphics: just plot a
contour map of the arrival-time surface with closely-spaced contours. We go on
to explain that rings should be (a) sensitive to time-delay ratios between
different pairs of images, but (b) very insensitive to H_0. We illustrate this
for the well-known quads 1115+080 and 1608+656.
