This survey combines 9 years of INTEGRAL IBIS observations from December 2002 through January 2011 into a single Galactic Plane image. A total of 135 megaseconds of exposure is included in the observations used. Survey data is generated for the Galactic plane in the region |b| %3C= 17.5. The original flux data has been convolved with 5' seeing kernel. To minimize loss of resolution in transformations, the Lanczos sampler is suggested as the default, but may be overriden by the user. The exposure and sensitivity vary considerably over the coverage region, but 90% of the field has a limiting sensitivity better than 2.2 x 10-11ergs s-1cm-2 or about 1.56 mCrab. Further details of the survey construction are given in the reference. The flux map use the PSF convolved maps from the survey. The flux maps are in millicrab units. See Krivonos, R. et al. in 2012 A&A (2012A&A...545A..27K).Original acknowledgement for data: Based on observations with INTEGRAL, an ESA project with instruments and science data centre funded by ESA member states (especially the PI countries: Denmark, France, Germany, Italy, Switzerland and Spain), Poland, and participation of Russia and the USA. Obtained through SkyView NASA/HEASARC. HiPSized by CDS.