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The Microwave Anisotropy eXperiment (MAX) is a balloon borne degree scale anisotropy experiment which is a collaboration between UC Santa Barbara and UC Berkeley. It flew for the fifth time on June, 1994, and observed two low dust regions and a relatively high dust region near the star Mu Pegasi. An attempt was made to observe the latter region in the same orientation as reported in Meinhold et al. (1992) Preliminary results are presented.