1520035

The survey of the Galactic Plane has continued as one of the main INTEGRAL scientific objectives because of the scientificpotential of both new source discovery and detailed monitoring of already known sources. We propose for a total of 3.0 Ms of observations in AO14 and 3 Ms in AO15 to continue our Key Program covering areas of the Plane with regular scans every orbit. For these AOs we selected a section of the Plane incorporating 2 sky regions that are rich in galactic sources (HMXB and SFXT in particular) and potential MeV/TeV sources.Our purpose is to regularly monitor known systems as well as to dramatically enhance the chances of discovering new systems or new outbursts from known sources. This program will allow a rapid response to bright events and a detailed study of fainttransients and their long term activity. Such a programme will be of high value to a very large fraction of the high-energyastronomy community stimulating science immediately and furthermore contributing greatly to the INTEGRAL legacy.In order to maximise the engagement of the scientific community we will continue to make the observations publicimmediately. The team will make as it has through AO8-12 and now in AO13 the scw-resolution IBIS and JEM-X lightcurves (in two energy bands) and per revolution mosaic images publicly available through the web as soon as possible afterthe observations have been performed. Any interesting source behaviour that emerges from our observations will beannounced promptly so that rapid follow-up by the community is possible as it has been already demonstrated. [truncated! Please see actual data for full text]