0720001

The Galactic bulge region is a rich host of variable X-ray and gamma-ray point sources.In AO-3 AO-4 AO-5 and AO-6 we have been monitoring this region with one hexagonal pattern approximately every 3 days whenever it was visible by INTEGRAL. Due to the high scientific return and to preserve the continuity with respect to past observations of this ever-changing region we suggest to continue our successful observing program. Because of the new format of AO-7 and as a service to the scientific community we ask the observations to be made public immediately. Moreover 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 hexagonal pattern publicly available through the web as soon as possible after the observations have been performed. Any interesting source behaviour which emerges from our observations will be announced promptly so that rapid follow-up by the community is possible. Our team consists of scientists with expertise on a large range of topics. We also intend to do a more in-depth analysis (spectra bursts flares etc.) of sources of particular interest on 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]