Project Goals
Image anisotropy of the CMB at angular
scales spanning the 1st three acoustic
peaks  (140 < l < 900) to determine the
cosmology which describes our universe
detailed high signal to noise images
cover 10% of the sky
use interferometrry:
   complementary & unique technique for CMB obs.
Image Sunyaev-Zel’dovich Effect in
nearby galaxy clusters
investigate S-Z effect / x-ray systematics with nearby
clusters,  eg., gas clumping, temperature gradients
complement high redshift BIMA/OVRO
observations