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

On the incidence of eclipsing Am binary systems in the SuperWASP survey