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We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginalcorrelation between the dust and the Q-band CMB data but none between the CMBdata and the Haslam map. While the amplitude of the correlation with the dustis larger than that expected from naive models of dust emission it does notdominate the sky emission.Comment: 6 pages, 4 figures. Accepted for publication in Astronomy and  Astrophysic

Correlation of the South Pole 94 data with $\mathsf{100 \mu}$m and 408 MHz maps