  Due to its proximity and its importance for the understanding of active
galaxies and their active nuclei (AGN), Centaurus A has been observed
frequently within the last 150 years in all accessible wavelength bands. Thus a
wealth of data exists which has been compiled into the "NASA Extragalactic
Database" (NED). Missing from this compilation are to date almost completely
the results of recent high energy observations as e.g. obtained by the Compton
Gamma Ray Observatory (CGRO). A combination of those recent high energy results
with all other observations in the NED enables us for the first time to
establish the important spectral energy distributions (SEDs) of this closest
AGN in different emission states. The combined data have been analyzed to
produce SEDs which are from contemporaneous data and in addition an attempt was
made to derive SEDs which are spatially resolved, i.e. SEDs from observations
which can resolve nucleus and jet in Cen A are treated separately.
