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We present observations of two new single-lined eclipsing binaries, bothconsisting of an Am star and an M-dwarf, discovered by the Wide Angle Searchfor Planets transit photometry survey. Using WASP photometry and spectroscopicmeasurements we find that HD186753B has an orbital period of P=1.9194 days, amass of M=0.24 +/- 0.02 M_sun and radius of R=0.31 +/- 0.06 R_sun; and thatTCY7096-222-1B has an orbital period of P=8.9582 days, a mass between 0.29 and0.54 M_sun depending on eccentricity and radius of R=0.263+0.02-0.07 R_sun. Wefind that the Am stars have relatively low rotational velocities that closelymatch the orbital velocities of the M-dwarfs, suggesting that they have been"spun-down" by the M-dwarfs.

The masses and radii of HD186753B and TYC7096-222-1B: the discovery of two M-dwarfs that eclipse A-type stars