The need for accurate and complete maps of the galaxy at radio frequen
cies is made evident not only by the importance of the data in the stu
dy of galactic dynamics and structure formation but also in the analys
is of cosmic background radiation data. A summary of the existing radi
o surveys of our galaxy is presented along with their limitations. A n
ew program, the Galactic Emission Mapping (GEM) project, to obtain cal
ibrated and complete maps of the galaxy in the 400 to 1400 MHz range,
is outlined.