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We present a Wiener filtered map of the Cosmic Microwave Background (CMB)fluctuations in a disk with 15 degree diameter, centered at the North CelestialPole. The map is based on the 1993-1995 data from the Saskatoon (SK)experiment, with an angular resolution around 1 degree in the frequency range27.6-44.1 GHz. The signal-to-noise ratio in the map is of order two, and someindividual hot and cold spots are significant at the 5 sigma level. The spatialfeatures are found to be consistent from year to year, reenforcing theconclusion that the SK results are not dominated by residual atmosphericcontamination or other non-celestial signals.

A High-Resolution Map of the Cosmic Microwave Background around the North Celestial Pole