  The Smithsonian Hectospec Lensing Survey (SHELS) combines a large deep
complete redshift survey with a weak lensing map from the Deep Lens Survey
(Wittman et al. 2002; 2005). We use maps of the velocity dispersion based on
systems identified in the redshift survey to compare the three-dimensional
matter distribution with the two-dimensional projection mapped by weak lensing.
We demonstrate directly that the lensing map images the three-dimensional
matter distribution obtained from the kinematic data.
