0620015

We propose a long 600 ks INTEGRAL observation with multiwavelength supporting observations to test models for the nuclear jet emission in the nearest radio galaxy Centaurus A by constructing a detailed spectral energy distribution (SED) ranging from radio through gamma ray bands. The emphasis will be to extend present X-ray results into the hundreds of keV and MeV range with high statistical significance by including results from GLAST MeV scanning observations and into the radio range with 8.4 and 22 GHz TANAMI and 4.8 8.6 17 19 38 and 40 GHz ATCA monitoring. The resulting Radio/IR/INTEGRAL/GLAST SED will allow for evaluating nuclear jet models such as the spine-sheath stratified jet model. These detailed results can then be the basis for modeling other more distant radio galaxies and quasars. [truncated! Please see actual data for full text]