0520001

The Galactic bulge region is a rich host of variable X-ray and gamma-ray point sources.In AO-3 and AO-4 we have been monitoring this region with one hexagonal observation approximately every 3 days whenever it was visible by INTEGRAL. Because of the high scientific return and 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 as well as the mosaic images per hexagonalobservation publicly available through the web as soon as possible after 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 flares etc.) of sources of particular intereston short and long time scales. These sources include bright and relatively faint X-raytransients X-ray bursters persistent neutron star and black-hole candidate binarieshigh-mass X-ray binaries etc.. [truncated! Please see actual data for full text]