  During 2001 and 2002, observations of several X-ray bright clusters of
galaxies were conducted using the ACBAR Bolometer Array on the South Pole Viper
telescope. A multi-frequency analysis of these clusters is currently underway.
This multi-frequency analysis includes 150, 220 and 275 GHz data from ACBAR,
X-ray imaging and spectroscopy from Chandra and XMM-Newton, and weak lensing
data from the CTIO 4m Blanco telescope. We describe here how ACBAR can be used
to create fully sampled cluster images and present such images for four of the
clusters in our sample; Abell 3266, Abell 3827, Abell S1063 and 1E0657-56. In
these images, the Sunyaev-Zel'dovich Effect is clearly detected.
