  We fit the data for the binary-lens microlensing event MACHO 98-SMC-1 from 5
different microlensing collaborations and find two distinct solutions
characterized by binary separation d and mass ratio q: (d,q)=(0.54,0.50) and
(d,q)=(3.65,0.36), where d is in units of the Einstein radius. However, the
relative proper motion of the lens is very similar in the two solutions, 1.30
km/s/kpc and 1.48 km/s/kpc, thus confirming that the lens is in the Small
Magellanic Cloud. The close binary can be either rotating or approximately
static but the wide binary must be rotating at close its maximum allowed rate
to be consistent with all the data. We measure limb-darkening coefficients for
five bands ranging from I to V. As expected, these progressively decrease with
rising wavelength. This is the first measurement of limb darkening for a
metal-poor A star.
