  We can think of a lensed quasar as taking the Hubble time, shrinking it by
\~10^{-11}, and then presenting the result to us as a time delay; the shrinking
factor is of the order of fractional sky-area that the lens occupies. This cute
fact is a straightforward consequence of lensing theory, and enables a simple
rescaling of time delays. Observed time delays have a 40-fold range, but after
rescaling the range reduces to 5-fold. The latter range depends on details of
the lens and lensing configuration--for example, quads have systematically
shorter rescaled time delays than doubles--and is as expected from a simple
model. The hypothesis that observed time-delay lenses all come from a
generalized-isothermal family can be ruled out. But there is no indication of
drastically different populations either.
