  The Galactic Bulge region is a rich host of variable high-energy point
sources. These sources include bright and relatively faint X-ray transients,
X-ray bursters, persistent neutron star and black-hole candidate binaries,
X-ray pulsars, etc.. We have a program to monitor the Galactic Bulge region
regularly and frequently with the gamma-ray observatory INTEGRAL. As a service
to the scientific community the high-energy light curves of all the active
sources as well as images of the region are made available through the WWW. We
show the first results of this exciting new program.
