0420001

The Galactic bulge region is a rich host of variable X-ray and gamma-ray point sources.In AO-3 we have been monitoring this region with one hexagonal observation approximatelyevery 3 days whenever it was visible by INTEGRAL. Because of the high scientific returnand to preserve the continuity with respect to past observations of this ever-changing regionwe suggest to continue our successful observing program. As a service to the scientificcommunity we make the IBIS/ISGRI and JEM-X light curves both in two energy bands perscience window and per hexagonal observation publicly available through the web as soon as theobservations have been performed. Any interesting source behaviour which emerges from ourobservations will be announced promptly so that rapid follow-up by the community ispossible. Our team consists of scientists with expertise on a large range of topics. We alsointend to do a more in-depth analysis (spectra bursts etc.) of sources of particular intereston short and long time scales. These sources include bright and relatively faint X-raytransients X-ray bbursters persistent neutron star and black-hole candidate binarieshiogh-mass X-ray binaries etc.. [truncated! Please see actual data for full text]