  Astrophysical neutrinos detected by the IceCube observatory can be of
Galactic or extragalactic origin. The collective contribution of all the
detected neutrinos allows us to measure the total diffuse neutrino Galactic and
extragalactic signal. In this work, we describe a simulation package that makes
use of this diffuse Galactic contribution information to simulate a population
of Galactic sources distributed in a manner similar to our own galaxy. This is
then compared with the sensitivities reported by different IceCube data samples
to estimate the number of sources that IceCube can detect. We provide the
results of the simulation that allows us to make statements about the nature of
the sources contributing to the IceCube diffuse signal.
