Finding Wolf-Rayet Stars in the Local Group
  We summarize past and current surveys for Wolf-Rayet stars among the Local
Group galaxies, emphasizing both the how and the why. Such studies are
invaluable for helping us learn about massive star evolution, and for providing
sensitive tests of the stellar evolution models. But for such surveys to be
useful, the completeness limits must be well understood. We illustrate that
point in this review by following the "evolution" of the observed WC/WN ratio
in nearby galaxies. We end by examining our new survey for WR stars in the
Magellanic Clouds, which has revealed a new type of WN star, never before seen.
