The mask design for JEM-X is now finalized regarding the hole pattern and m
echnical support structure. The engineering model of the detectors with col
limators is under construction. The JEM-X sensitivities for source detectio
n in various circumstances are reviewed with proper regard to the way INTEG
RAL will carry out its pointed observations. An important fraction of the I
NTEGRAL observation time will be used for scans along the galactic plane an
d observations of the central region of our galaxy. The JEM-X performance f
or this type of observations is discussed.
The software tools used to carry out the detailed observation simulations a
re described.