  I expand on the results of a recent work in which a novel weighting algorithm
was shown to substantially increase the accuracy of an old, non-Bayesian
computational approach for inferring the source direction of a gravitational
wave from the output of a two-detector network. While that work was limited to
the consideration of circularly polarized gravitational waves, the current
analysis shows that the same approach is even more successful when applied to
the generic case of elliptically polarized gravitational waves.
