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A. B. Whiting, N. Suntzeff (CTIO)
Using a new set of type Ia SNe, the best-fitting bulk motion vector and flow-anisotropy tensor are calculated, along with confidence limits. The results are found to be consistent with no overall motion with respect to the cosmic microwave background and no significant departure from anisotropic flow.
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Bulletin of the American Astronomical Society, 34, #4
© 2002. The American Astronomical Soceity.