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We analyze the Gamma Ursae Minoris (GUM) and Mu Pegasii (MuP) scans of theMillimeter-wave Anisotropy eXperiment in the context of cold dark matter (CDM)models of structure formation, paying particular attention to thetwo-dimensional nature of the GUM scan. If all of the structure in the(foreground subtracted) data is attributed to cosmic microwave backgroundanisotropy, then there is a detection in each scan. For a standard CDM model,the amplitudes of the signals are individually compatible with the COsmicBackground Explorer measurement, but marginally inconsistent with each other.Comment: 10 pages in Plain TeX + 3 PS figures, CfPA-93-TH-2

Implications of the millimeter-wave anisotropy experiment for cold dark matter models