  We present first results from the Survey for Transiting Extrasolar Planets in
Stellar Systems (STEPSS). Our goal is to assess the frequency of close-in
extrasolar planets around main-sequence stars in several open clusters. By
concentrating on main-sequence stars in clusters of known (and varied) age,
metallicity, and stellar density, we will gain insight into how these various
properties affect planet formation, migration, and survival. We show
preliminary results from our 19 night photometric campaign of the old, solar
metallicity cluster NGC 1245. Taking into account the photometric precision,
observational window function, transit probability, and total number of stars
monitored, we estimate that we should be able to probe planetary companion
fractions of <1% for separations of a<0.03 AU. If 1% of the stars in the
cluster have Jupiter-sized companions evenly distributed in log(a) between 0.03
and 0.3 AU, we expect to find ~2 transits. A preliminary search of our light
curve data has revealed a transit with a depth ~4%. Based on its shape, it is
likely to be a grazing binary eclipse rather than a planetary transit,
emphasizing the need for high temporal resolution in transit surveys.
