Abstract
We review here the unique opportunity provided by the sub-millimeter/millimeter domain to characterize both the warm intra-cluster plasma via the Sunyaev Zel'dovich Effect (SZE) on the cosmic microwave background, and the dust within this plasma via its thermal emission. However, multi-wavelength measurements are needed in order to separate these effects from the foreground galactic dust and the background infrared galaxies.
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