  We cross-correlate the Saskatoon Q-Band data with different spatial template
maps to quantify possible foreground contamination. We detect a correlation
with the Diffuse Infrared Background Experiment (DIRBE) 100 microm map, which
we interpret as being due to Galactic free-free emission. Subtracting this
foreground power reduces the Saskatoon normalization of the Cosmic Microwave
Background (CMB) power spectrum by roughly 2%.
