  We analyze the Gamma Ursae Minoris (GUM) and Mu Pegasii (MuP) scans of the
Millimeter-wave Anisotropy eXperiment in the context of cold dark matter (CDM)
models of structure formation, paying particular attention to the
two-dimensional nature of the GUM scan. If all of the structure in the
(foreground subtracted) data is attributed to cosmic microwave background
anisotropy, then there is a detection in each scan. For a standard CDM model,
the amplitudes of the signals are individually compatible with the COsmic
Background Explorer measurement, but marginally inconsistent with each other.
