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M. Tegmark (University of Pennsylvania)
I describe the sharp constraints on cosmological paramaters placed by recent measurements of the cosmic microwave background, galaxy clustering, supernovae, etc., and how different types of measurements now allow powerful cross-checks to be made. I also comment on outstanding puzzles in the emerging cosmological ``standard model'' and upcoming measurements that may resolve them.
Support for this work is provided by NSF grant AST00-71213, NASA grant NAG5-9194 and the University of Pennsylvania Research Foundation.
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