  We present the weak lensing mass reconstructions of three clusters of
galaxies from data taken on the ESO Wide Field Imager. We detect a lensing
signal in all three clusters over a range of 1' < r < 17' (~0.1 h^-1 Mpc < r <
2 h^-1 Mpc). We measure the best fitting SIS and NFW profiles for each cluster
and show that in two of the three clusters the NFW profile is preferred to the
SIS with marginal significance (~95%).
