We propose here an experimental method to estimate the background in the SI
GMA observations. The aim is to apply this method to observations of the Ga
lactic Centre in which the known point sources have been removed to measure
the galactic diffuse gamma-ray emission. We detect a significant excess be
tween 45 and 95 keV keV, described by a power-law with an index 2.2. This l
ain relatively good agreement with previous measurements.