An implementation of the Electron Gamma Shower 4 code (EGS4)(1) has be
en developed to allow convenient simulation of typical gamma ray measu
rement systems. Coincidence gamma rays, beta spectra, and angular corr
elations have been added to adequately simulate a complete nuclear dec
ay and provide corrections to experimentally determined detector effic
iencies. This code has been used to strip certain low-background spect
ra for the purpose of extremely low-level assay. Monte Carlo calculati
ons of this sort can be extremely successful since low background dete
ctors are usually free of significant contributions from poorly locali
zed radiation sources, such as cosmic muons, secondary cosmic neutrons
, and radioactive construction or shielding materials. Previously, val
idation of this code has been obtained from a series of comparisons be
tween measurements and blind calculations(2). An example of the applic
ation of this code to an exceedingly low background spectrum stripping
will be presented.