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Using the Haystack Observatory 37-m radio telescope we have undertaken asearch for emission in the 2(0)-3(1)E rotational transition of methanol in itsfirst torsionally excited state (v_t=1) at 44.9 GHz. We examined seven galacticsources -- six strong emitters of Class II methanol maser lines and Orion KL,the only source where this line had been previously detected. We confirm (at alevel of 5\sigma) the previous detection and report two new detections -- areliable (9\sigma) detection in W3(OH) and a marginal (3.5\sigma) detection inNGC 6334F. Upper limits for other sources are presented. Although we did notsee obvious signatures of maser amplification in this transition in any source,arguments in favor of weak masing in W3(OH) are presented.Comment: 7 pages, 2 figures, 1 table. Accepted for publication in A&A, aa.cls  is include

Torsionally excited methanol at 44.9 GHz