Collected Contributions from the COBE-DMR Group to the Maryland Astrophysics Meeting on Dark Matter

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The three papers summarize the methods employed by the COBE-DMR group to analyze the power spectrum of the two-year DMR anisotropy maps. Results for the slope and normalization of the power spectrum are presented and compared. The implications of these results for various dark matter-based structure formation models are also discussed.
uuencoded file containing 3 separate Postscript files, each with figures and tables included

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