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