  We present a correlation between the ACME/SP94 CMB anisotropy data at 25 to
45 GHz with the IRAS/DIRBE data and the Haslam 408 MHz data. We find a marginal
correlation between the dust and the Q-band CMB data but none between the CMB
data and the Haslam map. While the amplitude of the correlation with the dust
is larger than that expected from naive models of dust emission it does not
dominate the sky emission.
