  We use data from the Tenerife 10, 15 and 33 GHz beamswitching experiments
along with the COBE 53 and 90 GHz data to separate the cosmic microwave
background (CMB) signal from the Galactic signal and create two maps at high
Galactic latitude. The new multi-MEM technique is used to obtain the best
reconstruction of the two channels. The two maps are presented and known
features are identified within each. We find that the Galactic contribution to
both the 15 and 33 GHz Tenerife data is small enough to be ignored when
compared to the errors in the data and the magnitude of the CMB signal.
