  The results of a search for eclipsing Am star binaries using photometry from
the SuperWASP survey are presented. The light curves of 1742 Am stars fainter
than V = 8.0 were analysed for the presences of eclipses. A total of 70 stars
were found to exhibit eclipses, with 66 having sufficient observations to
enable orbital periods to be determined and 28 of which are newly identified
eclipsing systems. Also presented are spectroscopic orbits for 5 of the
systems. The number of systems and the period distribution is found to be
consistent with that identified in previous radial velocity surveys of
`classical' Am stars.
