  We present the first results of a MOS campaign to follow up cluster
candidates located via weak lensing. Our main goals are to search for spatial
concentrations of galaxies that are plausible optical counterparts of the weak
lensing signals, and to determine the cluster redshifts from those of member
galaxies. Around each of 36 targeted cluster candidates, we obtain 15-32 galaxy
redshifts. For 28 of these targets, we confirm a secure cluster identification.
This includes three cases where two clusters at different redshifts are
projected along the same line-of-sight. In 6 of the 8 unconfirmed targets, we
find multiple small galaxy concentrations at different redshifts. In both the
remaining two targets, a single small galaxy concentration is found. We
evaluate the weak lensing mass of confirmed clusters. For a subsample of our
most cleanly measured clusters, we investigate the statistical relation between
their weak lensing mass and the velocity dispersion of their member galaxies,
comparing our sample with optically and X-ray selected samples from the
literature. Our lensing-selected clusters are consistent with
sigma_v=sigma_sis, with a similar scatter to the optically and X-ray selected
clusters. We thus find no evidence of selection bias compared to these other
techniques. We also derive an empirical relation between the cluster mass and
the galaxy velocity dispersion, which is in reasonable agreement with the
prediction of N-body simulations in the LCDM cosmology.
